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Pagina:Nicolai Copernici torinensis De revolutionibus orbium coelestium.djvu/391
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>in maximis à ſole diſtãtἤs matutinis & ueſpertinis,ut diximus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Inuenitq Veneris latitudines Boreas maiores triẽte unius gradus,quàm Auſtrinas<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Mercurἤ uero Auſtrinas ſeſqui gradu ferè maiores quàm Boreas<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sed difficultati & labori calculationǔ conſulere uolens,accepit ſecundum mediam quandam rationẽ ſeſtertia graduum in diuerſas partes latitudinis,quos gradus ad zodiacum rectlo circa terram Iatitudines ipſæ ſubtendunt, p quem latitudines definiuntur,præfertim quòd non euidentem propterea errorem profuturum exiſtimauit,pro ut etiam mox oſtendemus.Quod ſi modo grad<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>II</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>s<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>tanq à ſignorum circulo abſceſſus hinc inde æqles capiamus , excludamusq interim deuiationem,erunt demonſtrationes noſtræ ſimpliciores acfa eiliores,donec inflexionum latitudines determinauerimus.Oſtendendũ igitur eſt primum,quòd huius latitudinis excurſus
<div style="text-align:right;">[[File:CLXXXIX.png|300px]]</div>
circa contactus circuli eccentri maximus contingat,ubietiam lõgitudinis proſtha phæreles ſunt maximæ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Eſto enim cõmutris sectio planorũ zodiaci & circuli eccentri ſiue Veneris,ſiue Mercurἤ,per apogęum & pcrigæũ,in qua capiatur <small>A</small> terræ locus,atq <small>B</small> centrũ eccẽtri,<small>C D E F G</small> circuli ad ſigniferũ obliqui,ut uidelicet rectæ lineæ quæcũq ad regios angulos ipſi <small>C G</small>.ductæ angulos côpræhcndant æquales obliquitati:aganturq <small>A E</small> quidẽ contingens circuLum <small>A D</small> utrũq ſecans,ducãtur etiã à <small>D</small>,<small>E</small>,<small>F</small> ſignis perpendiculares,in <small>C G</small> quidē ipſæ <small>D H</small>,<small>E K</small>,<small>F L</small>,in ſubiectũ uero ſigniferi planum ipſæ <small>D M</small>,<small>E N</small>,<small>F O</small>,& coniungantur <small>M H</small>,<small>N K</small>,<small>O L</small>,& inſuper <small>A N</small>,<small>A O</small>,<small>A M</small>,ipſæ em̃ <small>A O M</small> recta eſt, cũ tria eius ſigna in duob<sup><small>9</small></sup>ſint planis,nempe medἤ ſignorum circuli & ipſius <small>A D M</small>,recto ad planum ſigniferi<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniam igitur in propoſita obliquatio ne longitudinis quidem anguli,qui ſub <small>H A M</small>,& <small>K A N</small>,proſthaphæreſes harũ ſtellarũ cõpræhendũt<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Latitudinis aũt excurſus,<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>in maximis à ſole diſtãtἤs matutinis & ueſpertinis,ut diximus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Inuenitq Veneris latitudines Boreas maiores triẽte unius gradus,quàm Auſtrinas<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Mercurἤ uero Auſtrinas ſeſqui gradu ferè maiores quàm Boreas<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sed difficultati & labori calculationǔ conſulere uolens,accepit ſecundum mediam quandam rationẽ ſeſtertia graduum in diuerſas partes latitudinis,quos gradus ad zodiacum rectlo circa terram Iatitudines ipſæ ſubtendunt, p quem latitudines definiuntur,præfertim quòd non euidentem propterea errorem profuturum exiſtimauit,pro ut etiam mox oſtendemus.Quod ſi modo grad<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>II</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>s<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>tanq à ſignorum circulo abſceſſus hinc inde æqles capiamus , excludamusq interim deuiationem,erunt demonſtrationes noſtræ ſimpliciores acfa eiliores,donec inflexionum latitudines determinauerimus.Oſtendendũ igitur eſt primum,quòd huius latitudinis excurſus
<div style="text-align:right;">[[File:CLXXXIX.png|300px]]</div>
circa contactus circuli eccentri maximus contingat,ubietiam lõgitudinis proſtha phæreles ſunt maximæ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Eſto enim cõmutris sectio planorũ zodiaci & circuli eccentri ſiue Veneris,ſiue Mercurἤ,per apogęum & pcrigæũ,in qua capiatur <small>A</small> terræ locus,atq <small>B</small> centrũ eccẽtri,<small>C D E F G</small> circuli ad ſigniferũ obliqui,ut uidelicet rectæ lineæ quæcũq ad regios angulos ipſi <small>C G</small>.ductæ angulos côpræhcndant æquales obliquitati:aganturq <small>A E</small> quidẽ contingens circulum <small>A D</small> utrũq ſecans,ducãtur etiã à <small>D</small>,<small>E</small>,<small>F</small> ſignis perpendiculares,in <small>C G</small> quidē ipſæ <small>D H</small>,<small>E K</small>,<small>F L</small>,in ſubiectũ uero ſigniferi planum ipſæ <small>D M</small>,<small>E N</small>,<small>F O</small>,& coniungantur <small>M H</small>,<small>N K</small>,<small>O L</small>,& inſuper <small>A N</small>,<small>A O</small>,<small>A M</small>,ipſæ em̃ <small>A O M</small> recta eſt, cũ tria eius ſigna in duob<sup><small>9</small></sup>ſint planis,nempe medἤ ſignorum circuli & ipſius <small>A D M</small>,recto ad planum ſigniferi<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniam igitur in propoſita obliquatio ne longitudinis quidem anguli,qui ſub <small>H A M</small>,& <small>K A N</small>,proſthaphæreſes harũ ſtellarũ cõpræhendũt<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Latitudinis aũt excurſus,<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>parte ſui orbis ſtella fuerit<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> At in Mercurio cum ſtatuerimus angulum <small><small>B A G</small></small> dodrantem unius gradus, & <small><small>A D</small></small> ad <small><small>B G</small></small>,ut <small>1</small>oooo ad <small>131</small>.atq <small><small>A B C</small></small>, <small>13573</small>. & reliquum <small><small>A E</small></small>,<small>6827</small>. habebit qui ſub <small><small>C A D</small></small> angulus ſcrup.
<div style="text-align:left;">[[File:CLXXXXIIABCDEFGHK.png|300px|]]</div>
<small>XXXIII</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> <small><small>E A F</small></small> autẽ,ſcrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> prope <small>LXX</small>.Deſunt igitur illic ſcrup.<small>XII</small>.hic abundant ſcrup. xv<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> attamen hæ differentiæ ſub radἤs Solis ferè abſumūtur,priuſquam conſpectui noſtro emergat Mercurius,quamobrem apparentem ſolummodo eius deuiationẽ ſecuti ſunt priſci, quaſi ſimplicem<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Si quis nihilominus etiam latentes illos ſub Sole meatus laboris minime pteſus exactã rationẽ ſequi uoluerit.qmodo id fiat hoc modo oſtendemus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Id autem exempli gratia in Mercurio,eo q inſigniorē faciat deuiationē quã Venus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit em̃ <small><small>A B</small></small> recta linea in ſectiõe cõmunt orbis ſtellæ & ſigniferi, dũ terra quæſita fuerit in apogæo uel perigæo orbis ſtellę<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Ponamus aũt <small><small>A B</small></small> lineam abſq diſcrimine part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>10000</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> quaſi longitudinem mediã inter maximam minimamq,ut circa obliquationem fecimus. Deſcribatur anutẽ circulus <small><small>D E F</small></small>,in <small><small>C</small></small> centro,orbi eccentro parallelus ſecundū <small><small>C B</small></small> diſtantiam, in quo parallelo ſtella tũc maximam deuiationem facere intelligatur,& ſit dimetiens eius <small><small>D C F</small></small>,quam etiã oportebat eſſe ad <small><small>A B</small></small>, & ambæ lineæ in eodẽ plano, ad orbem ſtellæ recto<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Aſſumatur ergo <small><small>E F</small></small> circũferẽtia part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>uerbi gratia,<small><small>X L V</small></small>.ad quã ſcrutamur ſtellæ deuiationem, & agãtur perpēdicularcs <small><small>E G</small></small> ipſi <small><small>C F</small></small>,& ad ſubiectũ orbis planũ <small><small>E K</small></small>,<small><small>G K</small></small>,cõnexaq <small><small>H K</small></small>, cõpleatur parallelogrammũ rectangulum,& cõiungantur <small><small>A E</small></small>,<small><small>A K</small></small>,<small><small>E C</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Cum ergo <small><small>B C</small></small> fuerit in Mercurio ſecundum maximam deuiationem part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>131</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>qualiũ ſit <small><small>A B</small></small>, <small>1</small>oooo, quarũ eſt etiam <small><small>C E</small></small>,<small>3573</small>,eſtq triangulũ rectangulū datorũ angulo<small>R</small>, erit etiã latus <small><small>E G</small></small>,ſiue <small><small>K H</small></small> earundem <small>2526</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>ſed ablata <small><small>B H</small></small>, quæ æqualis eſt ipſi <small><small>E G</small></small>,ſiue <small><small>C G</small></small>,relinqtur <small><small>A H</small></small>,<small>7474</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Trianguliigic ah k, datoru Iateru retftu h angulum coprehcndentiu erit fubtefa a k 7SS<?*fedxqualis ipfi cB,fiueg H,cfttaliufjf Jgitur&fatrian<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>parte ſui orbis ſtella fuerit<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> At in Mercurio cum ſtatuerimus angulum <small><small>B A G</small></small> dodrantem unius gradus, & <small><small>A D</small></small> ad <small><small>B G</small></small>,ut <small>1</small>oooo ad <small>131</small>.atq <small><small>A B C</small></small>, <small>13573</small>. & reliquum <small><small>A E</small></small>,<small>6827</small>. habebit qui ſub <small><small>C A D</small></small> angulus ſcrup.
<div style="text-align:left;">[[File:CLXXXXIIABCDEFGHK.png|300px|]]</div>
<small>XXXIII</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> <small><small>E A F</small></small> autẽ,ſcrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> prope <small>LXX</small>.Deſunt igitur illic ſcrup.<small>XII</small>.hic abundant ſcrup. xv<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> attamen hæ differentiæ ſub radἤs Solis ferè abſumūtur,priuſquam conſpectui noſtro emergat Mercurius,quamobrem apparentem ſolummodo eius deuiationẽ ſecuti ſunt priſci, quaſi ſimplicem<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Si quis nihilominus etiam latentes illos ſub Sole meatus laboris minime pteſus exactã rationẽ ſequi uoluerit.qmodo id fiat hoc modo oſtendemus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Id autem exempli gratia in Mercurio,eo q inſigniorē faciat deuiationē quã Venus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit em̃ <small><small>A B</small></small> recta linea in ſectiõe cõmunt orbis ſtellæ & ſigniferi, dũ terra quæſita fuerit in apogæo uel perigæo orbis ſtellę<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Ponamus aũt <small><small>A B</small></small> lineam abſq diſcrimine part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>10000</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> quaſi longitudinem mediã inter maximam minimamq,ut circa obliquationem fecimus. Deſcribatur anutẽ circulus <small><small>D E F</small></small>,in <small><small>C</small></small> centro,orbi eccentro parallelus ſecundū <small><small>C B</small></small> diſtantiam, in quo parallelo ſtella tũc maximam deuiationem facere intelligatur,& ſit dimetiens eius <small><small>D C F</small></small>,quam etiã oportebat eſſe ad <small><small>A B</small></small>, & ambæ lineæ in eodẽ plano, ad orbem ſtellæ recto<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Aſſumatur ergo <small><small>E F</small></small> circũferẽtia part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>uerbi gratia,<small><small>X L V</small></small>.ad quã ſcrutamur ſtellæ deuiationem, & agãtur perpēdicularcs <small><small>E G</small></small> ipſi <small><small>C F</small></small>,& ad ſubiectũ orbis planũ <small><small>E K</small></small>,<small><small>G K</small></small>,cõnexaq <small><small>H K</small></small>, cõpleatur parallelogrammũ rectangulum,& cõiungantur <small><small>A E</small></small>,<small><small>A K</small></small>,<small><small>E C</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Cum ergo <small><small>B C</small></small> fuerit in Mercurio ſecundum maximam deuiationem part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>131</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>qualiũ ſit <small><small>A B</small></small>, <small>1</small>oooo, quarũ eſt etiam <small><small>C E</small></small>,<small>3573</small>,eſtq triangulũ rectangulū datorũ angulo<small>R</small>, erit etiã latus <small><small>E G</small></small>,ſiue <small><small>K H</small></small> earundem <small>2526</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>ſed ablata <small><small>B H</small></small>, quæ æqualis eſt ipſi <small><small>E G</small></small>,ſiue <small><small>C G</small></small>,relinqtur <small><small>A H</small></small>,<small>7474</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Trianguli igit̆ <small><small>A H K</small></small>, datorũ laterū rectū <small><small>H</small></small> angulum coprehendentiū erit ſubtẽſa <small><small>A K</small></small> <small>7889</small><sub>•</sub>ſed æqualis ipſi <small><small>C B</small></small>,ſiue <small><small>G H</small></small>,eſt taliũ 131<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Jgitur&fatrian<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>parte ſui orbis ſtella fuerit<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> At in Mercurio cum ſtatuerimus angulum <small><small>B A G</small></small> dodrantem unius gradus, & <small><small>A D</small></small> ad <small><small>B G</small></small>,ut <small>1</small>oooo ad <small>131</small>.atq <small><small>A B C</small></small>, <small>13573</small>. & reliquum <small><small>A E</small></small>,<small>6827</small>. habebit qui ſub <small><small>C A D</small></small> angulus ſcrup.
<div style="text-align:left;">[[File:CLXXXXIIABCDEFGHK.png|300px|]]</div>
<small>XXXIII</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> <small><small>E A F</small></small> autẽ,ſcrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> prope <small>LXX</small>.Deſunt igitur illic ſcrup.<small>XII</small>.hic abundant ſcrup. xv<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> attamen hæ differentiæ ſub radἤs Solis ferè abſumūtur,priuſquam conſpectui noſtro emergat Mercurius,quamobrem apparentem ſolummodo eius deuiationẽ ſecuti ſunt priſci, quaſi ſimplicem<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Si quis nihilominus etiam latentes illos ſub Sole meatus laboris minime pteſus exactã rationẽ ſequi uoluerit.qmodo id fiat hoc modo oſtendemus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Id autem exempli gratia in Mercurio,eo q inſigniorē faciat deuiationē quã Venus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit em̃ <small><small>A B</small></small> recta linea in ſectiõe cõmunt orbis ſtellæ & ſigniferi, dũ terra quæſita fuerit in apogæo uel perigæo orbis ſtellę<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Ponamus aũt <small><small>A B</small></small> lineam abſq diſcrimine part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>10000</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> quaſi longitudinem mediã inter maximam minimamq,ut circa obliquationem fecimus. Deſcribatur anutẽ circulus <small><small>D E F</small></small>,in <small><small>C</small></small> centro,orbi eccentro parallelus ſecundū <small><small>C B</small></small> diſtantiam, in quo parallelo ſtella tũc maximam deuiationem facere intelligatur,& ſit dimetiens eius <small><small>D C F</small></small>,quam etiã oportebat eſſe ad <small><small>A B</small></small>, & ambæ lineæ in eodẽ plano, ad orbem ſtellæ recto<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Aſſumatur ergo <small><small>E F</small></small> circũferẽtia part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>uerbi gratia,<small><small>X L V</small></small>.ad quã ſcrutamur ſtellæ deuiationem, & agãtur perpēdicularcs <small><small>E G</small></small> ipſi <small><small>C F</small></small>,& ad ſubiectũ orbis planũ <small><small>E K</small></small>,<small><small>G K</small></small>,cõnexaq <small><small>H K</small></small>, cõpleatur parallelogrammũ rectangulum,& cõiungantur <small><small>A E</small></small>,<small><small>A K</small></small>,<small><small>E C</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Cum ergo <small><small>B C</small></small> fuerit in Mercurio ſecundum maximam deuiationem part<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub><small>131</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>qualiũ ſit <small><small>A B</small></small>, <small>1</small>oooo, quarũ eſt etiam <small><small>C E</small></small>,<small>3573</small>,eſtq triangulũ rectangulū datorũ angulo<small>R</small>, erit etiã latus <small><small>E G</small></small>,ſiue <small><small>K H</small></small> earundem <small>2526</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>ſed ablata <small><small>B H</small></small>, quæ æqualis eſt ipſi <small><small>E G</small></small>,ſiue <small><small>C G</small></small>,relinqtur <small><small>A H</small></small>,<small>7474</small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Trianguli igit̆ <small><small>A H K</small></small>, datorũ laterū rectū <small><small>H</small></small> angulum coprehendentiū erit ſubtẽſa <small><small>A K</small></small> <small>7889</small><sub>•</sub>ſed æqualis ipſi <small><small>C B</small></small>,ſiue <small><small>G H</small></small>,eſt taliũ 131<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Igitur & {{Hws|trian|triangulo}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>gulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small>K E</small> datis,<small><small>K</small></small> rectũ cõprehcndentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alqs Si circa Venere faciemus, cofigna bimuscy in Canone fubfcris bendo. Quibus fic expolitis, pro eis quae inter hos funt li« mites deuiationibus tam Ve neri quam Mercurio Sexage* limas fiue ferup .proportionu adaptabimus. Sit enim circu« lus a b corbis eccetri Veneris uel Mercuri), fintep a c nodi hui9 latitudinis motus, b lineg maximae deuiationis, quo fa*
<?io centro circulus paruus de= feribatur d f g,cuius dimeties dbf (itpertranfuerfum,per quem contingatlibratio deuiatio= nis.Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small>K E</small> datis,<small><small>K</small></small> rectũ cõprehcndentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alqs Si circa Venere faciemus, cofigna bimuscy in Canone fubfcris bendo. Quibus fic expolitis, pro eis quae inter hos funt li« mites deuiationibus tam Ve neri quam Mercurio Sexage* limas fiue ferup .proportionu adaptabimus. Sit enim circu« lus a b corbis eccetri Veneris uel Mercuri), fintep a c nodi hui9 latitudinis motus, b lineg maximae deuiationis, quo fa*
<?io centro circulus paruus de= feribatur d f g,cuius dimeties dbf (itpertranfuerfum,per quem contingatlibratio deuiatio= nis.Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehcndentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alqs Si circa Venere faciemus, cofigna bimuscy in Canone fubfcris bendo. Quibus fic expolitis, pro eis quae inter hos funt li« mites deuiationibus tam Ve neri quam Mercurio Sexage* limas fiue ferup .proportionu adaptabimus. Sit enim circu« lus a b corbis eccetri Veneris uel Mercuri), fintep a c nodi hui9 latitudinis motus, b lineg maximae deuiationis, quo fa*
<?io centro circulus paruus de= feribatur d f g,cuius dimeties dbf (itpertranfuerfum,per quem contingatlibratio deuiatio= nis.Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus fic expolitis, pro eis quae inter hos funt li« mites deuiationibus tam Ve neri quam Mercurio Sexage* limas fiue ferup .proportionu adaptabimus. Sit enim circu« lus a b corbis eccetri Veneris uel Mercuri), fintep a c nodi hui9 latitudinis motus, b lineg maximae deuiationis, quo fa*
<?io centro circulus paruus de= feribatur d f g,cuius dimeties dbf (itpertranfuerfum,per quem contingatlibratio deuiatio= nis.Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circu« lus a b corbis eccetri Veneris uel Mercuri), fintep a c nodi hui9 latitudinis motus, b lineg maximae deuiationis, quo fa*
<?io centro circulus paruus de= feribatur d f g,cuius dimeties dbf (itpertranfuerfum,per quem contingatlibratio deuiatio= nis.Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circu« lus a b corbis eccetri Veneris uel Mercuri), fintep a c nodi hui9 latitudinis motus, b lineg maximae deuiationis, quo fa*
<?io centro circulus paruus de= feribatur d f g,cuius dimeties dbf (itpertranfuerfum,per quem contingatlibratio deuiatio= nis.Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam politum e fi:,quod exiftete terra in apogsco uel perigaeo orbis eccentri ftella:,ipfa ftella maxima faciat deuiatio nem,nempe in f ligno,& circulus ipiam deferens tunccirculu paruu tangebat in F.Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
31utgmrtf251e8jav7q2gpi4blh26b4
183997
183996
2022-07-19T13:43:12Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcucp remota ab apogaeo uel perigaeo eccetri ftella:,fecudu que motu capiatur limiliscir cumfcretia parui circuli.qua: fit f g,& deferiptus a g c circulus,q ftellam defert paruu circulu,fecabit Si eius diametru in b. Sitcp ftella in x,eritq? e k circumferetia ipfi o f fimilis iuxta hypothe fim,aga t etia k l ppcndicularis ad a b c circulu.Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
01i14cl6duooijye4v3lang00uu3eqv
183999
183997
2022-07-19T13:58:07Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propofitu eft ex f g,e k,8C b E.inuenire magnitudine k L,id eft diftatia ftellg ab abc circulo.Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
2vzim8f3verp1nym7w8i95qoe7huysa
184000
183999
2022-07-19T14:02:28Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quonia em p f gn'rcufefentia,erit s a data, tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
foo3rpti2ribj4y2u65aomby91f6fec
184001
184000
2022-07-19T14:02:50Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quonia em p f gn'rcufefentia,erit s a data , tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
oi5na30aw7vm8ru48l70mb1yb0co1wx
184002
184001
2022-07-19T14:03:08Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em p f gn'rcufefentia,erit s a data , tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
nwsyqb1rtgf1bvjeq2tfyovh5b8n322
184003
184002
2022-07-19T14:04:25Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p f gn'rcufefentia,erit s a data , tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
bc2135y37ijynzw3vqjdhounn64wsne
184004
184003
2022-07-19T14:04:59Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> n'rcufefentia,erit s a data , tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
4yscwknnr9wzj5mi9fbxnwhm0rthxpo
184005
184004
2022-07-19T14:06:09Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit s a data , tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
hfo4rcisbxyghaesbxmzil08feflkds
184006
184005
2022-07-19T14:06:34Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tancjj re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
78r5pk12hvr62r4dx4whrzu4t8xzbzc
184007
184006
2022-07-19T14:06:51Z
Autonomous agent 5
23837
proofread-page
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq re<fia minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
t9pcdw55u05ugij87vj82uf3y0iabe4
184008
184007
2022-07-19T14:07:09Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differes a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
b0a4ztdwif8m0tflofph2cw368665hu
184009
184008
2022-07-19T14:07:36Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs a circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
h5py4w5ggmgpcwjz5bk3omzu4t00ms8
184010
184009
2022-07-19T14:07:59Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulat i,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
g654quot5i8iv8m6a6g4vwgzap1xuxp
184011
184010
2022-07-19T14:08:17Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,Si e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
kh35tm51888lifkrdn2qlavpzceqrer
184012
184011
2022-07-19T14:08:32Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& e f fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
0hyujoceppks9uqpyde2q6btrkhe51i
184013
184012
2022-07-19T14:08:57Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> fimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
083jlabt9zkadv82q589vfyj8f3m85s
184014
184013
2022-07-19T14:09:21Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus b f tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
nl8codnuwkokn6ooqvf31s0jrsxav87
184015
184014
2022-07-19T14:09:54Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq b s.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
1zzlom99wbbd86buctcyj02x1m2gdp5
184016
184015
2022-07-19T14:10:37Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eft autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
6msshhj2bwg5p9x0d8okx60u9d8b01z
184017
184016
2022-07-19T14:11:13Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt autB f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
koz18szswfidmeuap3qp43remgybwgl
184019
184017
2022-07-19T14:11:41Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt B f ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
k5s2np3a845qie7r1v1lr3eimmsldz2
184020
184019
2022-07-19T14:12:22Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad b E,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
b6ldtbmpc9ohcz58pfuqttba06co89l
184021
184020
2022-07-19T14:12:48Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ficut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
9p21p0jkafjvuo84iy6j9hn8a7sf3be
184022
184021
2022-07-19T14:13:17Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut fubtefa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
mrftlyn62v0hybrwzwlcz9yddinhnqs
184023
184022
2022-07-19T14:13:54Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli c b quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
7xprofp3mshva3h28bs9w3he2ucz929
184024
184023
2022-07-19T14:14:22Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quas drangulu ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
7brvtkat2mje1m91cy0f4eny0us2cvz
184025
184024
2022-07-19T14:14:58Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad fubtefam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
cqxo6nkuqjdgolbk3gezck5majnc5zq
184026
184025
2022-07-19T14:15:50Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli c K,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
omrz776pgiw4ruf9p7ykf7sxogf8g6l
184027
184026
2022-07-19T14:16:30Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atqj b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
nsx2932sd18pfq1bhmiysspwdmihl9k
184028
184027
2022-07-19T14:16:46Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq b b ad k L.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
4fpccshpfpo0g8ro3epo0s9i3qf8pqn
184029
184028
2022-07-19T14:17:41Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
ks4bpxknljmo01j75uayy3jj67twvrb
184030
184029
2022-07-19T14:18:34Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad nume 7u6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
osiebspof4vf8cjmp9tdvows9slhlxo
184031
184030
2022-07-19T14:19:10Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ 6o.pofuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
kiokm7ozab3s17zksgr5q2lnqa3inmq
184032
184031
2022-07-19T14:19:31Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ 6o.poſuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
0jbzbkt7k84m5naqfejhx45rsw0x888
184033
184032
2022-07-19T14:20:05Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& b f,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
ilg9jxq4gcdygwuun0bt0zknqtn2bli
184034
184033
2022-07-19T14:20:32Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etia qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
gkdx2yeo4ibvqlzwqgo8fionp284gi8
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2022-07-19T14:20:56Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã qug ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
m4ev74p82effnxrzl8vsvnhmlhjnsdd
184036
184035
2022-07-19T14:21:25Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cetro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
h2w47z3dlonhohqb21msn9eumirlwn5
184037
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2022-07-19T14:21:54Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro c b,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
3tq5jsi3dj93be7yixwt1wmhoqbqhy0
184038
184037
2022-07-19T14:22:29Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etia b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
qs6h8rheoyh5oveq0z5bjuw36ktw9mw
184039
184038
2022-07-19T14:23:11Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā b b in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
dztazzdhxrwendgx5bqng6lfv5fumox
184040
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2022-07-19T14:23:37Z
Autonomous agent 5
23837
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text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eifde,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
f8b76yyt7c3aeuz3j99vuxu0lm9jww2
184042
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2022-07-19T14:24:19Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,qux cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
nb0vo1gc26jn9hmfgiyq8k3owda8eb7
184043
184042
2022-07-19T14:24:42Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cu in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
86cyk2rzw6b699mehdufrc005qxye17
184044
184043
2022-07-19T14:25:03Z
Autonomous agent 5
23837
proofread-page
text/x-wiki
<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in fe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
l0dso1u07j79hv0673jt7lps388gk1t
184045
184044
2022-07-19T14:25:19Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,Si procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
d51fqq24gum3w4lf8vtioc9z11jko8y
184046
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2022-07-19T14:25:38Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatu p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
i8ppfqnepmuoedke7pfofqrcxzlzp6m
184047
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2022-07-19T14:26:06Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p 6 di-uifum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
lkng6rjny5kiyo2penmb1nlpk46eah5
184048
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2022-07-19T14:26:38Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus k d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
6jj8sfsjjhmoxtqanufoks2m1jnl5lt
184050
184048
2022-07-19T14:27:12Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K</small></small> d fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
50jumha52l4b7a763ifk3szritin9dr
184051
184050
2022-07-19T14:27:27Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> fcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
quqf4goukdj8mis9kl8behk9aaeqagj
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2022-07-19T14:27:54Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionu b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
owgm8gvst64wk0ergmtlit9avqf3zk9
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2022-07-19T14:28:22Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ b k circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
gfr3l2jzcu3z284fk319v09x78p5ilw
184054
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2022-07-19T14:28:48Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circuferetia: qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
bye5fokqicy1eiml967buh9gc0fjze7
184055
184054
2022-07-19T14:29:50Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ qua: lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
ifg7lmux9dls63kawogdeajlqsrnpqk
184056
184055
2022-07-19T14:30:09Z
Autonomous agent 5
23837
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ lita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
nz17dk3s12phrrzpa7snmhhddp6n5n1
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2022-07-19T14:30:32Z
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita. Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
ph2do4jqt5w0asnzp43v9m2s618uwzu
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Qua: etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
c806dupz4dshu2or1hu5f4xlw6q3vaq
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quæ etiJ adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
st5qe3om2wgb0avrl7yp2xylxljir6d
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quæ etiã adfignauimusCanoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quæ etiã adſignauimus Canoniquinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
ccnu212d1sw4u3x89s4dd869zodww11
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quæ etiã adſignauimus Canoni quinto,# ultimo loco,ut fequitur.<noinclude><references/></noinclude>
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<noinclude><pagequality level="2" user="Autonomous agent 5" /></noinclude>triangulo <small><small>A K E</small></small>,duobus lateribus <small><small>A K</small></small>,<small><small>K E</small></small> datis,<small><small>K</small></small> rectũ cõprehendentibus,datur angulus <small><small>K A E</small></small> reſpondens deuiationi ad <small><small>E F</small></small> circumferentiam,quam quærebamus,quæ etiã parum diſcernitur ab obſeruatis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Similiter in alἤs & circa Venerẽ faciemus, cõſignabimusq
<div style="text-align:right;">[[File:CLXXXXIII.png|300px|]]</div>
in Canone ſubſcribendo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quibus ſic expoſitis, pro eis quæ inter hos ſunt limites deuiationibus tam Veneri quàm Mercurio Sexageſimas ſiue ſrup<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>proportionũ adaptabimus<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sit enim circulus <small><small>A B C</small></small> orbis eccẽtri Veneris uel Mercurἤ, ſintq <small><small>A C</small></small> nodihui<sup><small>9</small></sup> latitudinis motus, <small><small>B</small></small> lineę maximæ deuiationis, quo facto centro circulus paruus deſcribatur <small><small>D F G</small></small>,cuius dimetiẽs <small><small>D B F</small></small> ſit pertranſuerſum,per quem contingat libratio deuiationis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Et quoniam poſitum eſt,quod exiſtẽte terra in apogæo uel perigæo orbis eccentri ſtellæ,ipſa ſtella maximã faciat deuiationem,nempe in <small><small>F</small></small> ſigno,& circulus ipſam deferens tunc circulũ paruũ tangebat in <small><small>F</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Sit modo terra utcũq remota ab apogæo uel perigæo eccẽtri ſtellæ,ſecudu quẽ motũ capiatur ſimilis circumferẽtia parui circuli,quæ ſit <small><small>F G</small></small>,& deſcriptus <small><small>A G C</small></small> circulus,q ſtellam defert paruū circulũ,ſecabit & eius diametrũ in <small><small>E</small></small><sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Sitq ſtella in <small><small>K</small></small>,eritq <small><small>E K</small></small> circumferētia ipſi <small><small>G F</small></small> ſimilis iuxta hypotheſim,agat̆ etiã <small><small>K L</small></small> ppendicularis ad <small><small>A B C</small></small> circulũ<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Propoſitũ eſt ex <small><small>F G</small></small>,<small><small>E K</small></small>,& <small><small>B E</small></small>,inuenire magnitudinẽ <small><small>K L</small></small>,id eſt diſtãtiã ſtellę ab <small><small>A B C</small></small> circulo<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>Quoniã em̃ p <small><small>F G</small></small> circũferentiã,erit <small><small>E G</small></small> data , tanq recta minime differẽs à circulari,& <small><small>E F</small></small> ſimiliter in ptibus, qbus <small><small>B F</small></small> tota,& reliq <small><small>B E</small></small>.Eſt aũt <small><small>B F</small></small> ad <small><small>B E</small></small>,ſicut ſubtẽſa dupli <small><small>C E</small></small> quadrangulũ ad ſubtēſam dupli <small><small>C K</small></small>,atq <small><small>B B</small></small> ad <small><small>K L</small></small>.Si igit̆ ad numerũ <small>6</small>o.poſuerimus,& <small><small>B F</small></small>,etiã quę ex cẽtro <small><small>C E</small></small>,habebimus etiā <small><small>B E</small></small> in eiſdē,quæ cũ in ſe multiplicata fuerit,& procreatũ p <small>6</small> diuiſum,habebimus <small><small>K L</small></small> ſcrup.proportionũ <small><small>B K</small></small> circūferẽtiæ quæ ſita<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub> Quæ etiã adſignauimus Canoni quinto,# ultimo loco,ut ſequitur.<noinclude><references/></noinclude>
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Pagina:Nicolai Copernici torinensis De revolutionibus orbium coelestium.djvu/400
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<noinclude><pagequality level="2" user="Ratte" /></noinclude>{|style="text-align:right;border-collapse:collapse" border=1
!colspan=13 style=text-align:center|Latitudines Saturni,Iouis, & Martis<sub><sup><sub><sup><sub>'''♦'''</sub></sup></sub></sup></sub>
|-
!colspan=2 style=text-align:center|Circũferentiæ.
!style=width:1.5em|
!style=text-align:center|Semiſſ. ſubtend dup. cir.
!style=width:1.5em|
!style=text-align:left|Differentiæ.
!rowspan=14 style=width:5em|
!colspan=2 style=text-align:center|Circũferentiæ.
!style=width:1.5em|
!style=text-align:center|Semiſſes ſubtend. dup. cir.
!style=width:1.5em|
!style=text-align:left|Differentiæ.
|-
!ꝑt.<!-- = partes circumferentiæ = gradus -->!!ſec.!!!!!!!!
!ꝑt.!!ſec.!!!!!!!!
|-
|||10<br>20<br>30||||74<span style=color:red>7</span><br>892<br>87036||||<span style=color:red>4</span><br>4<br>3
|||10<br>20<br>30||||472<br>590<br>706||||118<br>7<br>6
|-
|<br><br>61||40<br>50<br>0||||178<br>32<span style=color:red>0</span><br>462||||<span style=color:red>2</span><br>2<br>1
|<br><br>67||40<br>50<br>0||||822<br>936<br>92050||||5<br>4<br><span style=color:red>3</span>
|-
|||10<br>20<br>30||||603<br>743<br>882||||140<br>13<span style=color:red>9</span><br>9
|||10<br>20<br>30||||164<br>276<br>388||||3<br>2<br>1
|-
|<br><br>62||40<br>50<br>0||||88020<br>158<br>295||||8<br>7<br>7
|<br><br>68||40<br>50<br>0||||499<br>609<br>718||||11<span style=color:red>0</span><br>10<span style=color:red>9</span><br>9
|-
|||10<br>20<br>30||||431<br>566<br>701||||6<br>5<br>4
|||10<br>20<br>30||||827<br>935<br>93042||||8<br>7<br><span style=color:red>6</span>
|-
|<br><br>63||40<br>50<br>0||||835<br>968<br>89101||||4<br>3<br>2
|<br><br>69||40<br>50<br>0||||148<br>253<br>358||||<span style=color:red>5</span><br>5<br>4
|-
|||10<br>20<br>30||||232<br>363<br>493||||1<br>1<br>130
|||10<br>20<br>30||||462<br>565<br>667||||3<br><span style=color:red>2</span><br>2
|-
|<br><br>64||40<br>50<br>0||||62<span style=color:red>2</span><br>75<span style=color:red>1</span><br>879||||129<br>8<br>8
|<br><br>70||40<br>50<br>0||||769<br>87<span style=color:red>0</span><br>969||||1<br>100<br>99
|-
|||10<br>20<br>30||||9000<span style=color:red>6</span><br>133<br>25<span style=color:red>8</span>||||7<br>6<br><span style=color:red>6</span>
|||10<br>20<br>30||||94068<br>167<br>264||||<span style=color:red>8</span><br>8<br>7
|-
|<br><br>65||40<br>50<br>0||||383<br>507<br>631||||<span style=color:red>5</span><br>4<br>3
|<br><br>71||40<br>50<br>0||||361<br>457<br><span style=color:red>4</span>52||||6<br><span style=color:red>5</span><br><span style=color:red>4</span>
|-
|||10<br>20<br>30||||753<br>875<br>996||||2<br>1<br>1
|||10<br>20<br>30||||646<br>73<span style=color:red>9</span><br>832||||<span style=color:red>3</span><br>3<br>2
|-
|<br><br>66||40<br>50<br>0||||91116<br>23<span style=color:red>5</span><br>35<span style=color:red>4</span>||||120<br>119<br>8
|<br><br>72||40<br>50<br>0||||924<br>95015<br>10<span style=color:red>5</span>||||1<br><span style=color:red>0</span><br>90
|}<noinclude><references/></noinclude>
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Liber:Olim Ludi Scaenici.pdf
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|Author=Effie Ryle
|Title=[[Ólim]]
|Year=1914
|Publisher=G. Bell & Sons
|Source=British Library / Wikimedia Commons
|Image=[[File:Olim_Ludi_Scaenici.pdf|page=4|225px]]
|Pages=<pagelist
1=cover
2=1
/>
|Remarks=<h2>Summāria</h2>
*[[Ólim/Preface|{{sc|Preface}}]]
*[[Ólim/Prooemium|{{sc|Prooemium}}]]
*[[Ólim/Colloquium: “Passer Mortuus”|{{sc|Colloquium: “Passer Mortuus”}}]]
*[[Ólim/Virgínia|{{sc|Virgīnia}}]]
*[[Ólim/Vestis sanguine tíncta|{{sc|Vestis sanguine tīncta}}]]
*[[Ólim/Léx Oppia|{{sc|Lēx Oppia}}]]
*[[Ólim/Lúdi Magister|{{sc|Lūdi Magister}}]]
*[[Ólim/Imber Impendet|{{sc|Imber Impendet}}]]
}}
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<noinclude><pagequality level="4" user="PWidergren" /></noinclude>{{center|{{xxx-larger|ŌLIM}}}}
{{center|{{x-larger|LŪDĪ SCAENICĪ}}}}
{{center|{{sc|by}}}}
{{center|{{larger|E. RYLE}}}}
{{center|{{x-smaller|CLASSICAL MISTRESS<br/>AIGBURTH VALE HIGH SCHOOL, LIVERPOOL}}}}
{{center|{{larger|LONDON<br/>G. BELL AND SONS, {{sc|Ltd}}.<br/>1914}}}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="4" user="PWidergren" />{{rh|viii|ŌLIM|}}</noinclude>except in “Vestis Sanguine Tīncta,” but even here Ovid has already Romanized for us a tale of Babylon. Livy has provided the sources of “Virgīnia” and “Lēx Oppia”; Catullus, Martial, and Virgil the poems on which the shorter dialogues are based, and to which they form an introduction.
It has sometimes been felt that many Latin school books are better adapted for boys than for girls; perhaps ''Ōlim'' may claim to be primarily for girls. “Virgīnia,” “Passer Mortuus,” and “Vestis Sanguine Tīncta” have already been acted in the class-room; “Lēx Oppia” was performed at Cambridge in September 1913 by some of the members of the Association for the Reform of Latin Teaching.
I wish to acknowledge my gratitude to Mr. Appleton, Perse School, Cambridge, for various helpful suggestions; to Dr. Rouse for some advice on a few points of language and “quantity”; and to Mr. C. L. Mainwaring, Whitgift School, Croydon, for his reading of the proofs and assistance in “hidden quantities.”
{{dextra|{{larger|E. RYLE.}}{{gap|5em}}}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="4" user="PWidergren" /></noinclude>{{center|{{x-larger|PROOEMIUM}}}}
{{center|SCRĪPTOR FĀBULĀRUM LĒCTŌRIBUS S.D.}}
{{sc|Ut}} linguās Gallicam et Germānicam, sīc linguam Latīnam, illī optimē intellegunt quī nōn modō legunt {{nowrap|scrībunt-ve}}, sed etiam dīcunt. Nōnne enim lingua est membrum quō hominēs dīcunt?
Forsitan respondeās: Gallicē quidem vel Germānicē loquī volumus, quia Gallī {{nowrap|Germānī-que}} adhuc vīvunt, {{nowrap|nōbīs-que}} respondēre possunt. Cūr autem Latīnē loquī oportet, cum Rōmānī iamdiū mortuī sint? At negō Rōmānōs mortuōs esse, sīquidem verba et facta eōrum repetās, dum Catullum vel Virgīniam vel ipsum Catōnem tē esse simulēs. Hāc dē causā fabulās paucās brevēs-que composuī, quās dum agitis, Rōmānī Rōmānae-que esse vidēbiminī. Nē fortē negētis tālēs fabulās ā puellīs {{nowrap|puerīs-ve}} agī posse, āiō ferē omnēs aut ab amīcīs meīs adultīs, aut ā discipulīs, iam anteā aetās esse.
{{center|{{sc|Valēte.}}}}<noinclude><references/>
{{c|9}}</noinclude>
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<noinclude><pagequality level="4" user="PWidergren" /></noinclude>{{center|{{x-larger|PROOEMIUM}}}}
{{center|SCRĪPTOR FĀBULĀRUM LĒCTŌRIBUS S.D.}}
{{sc|Ut}} linguās Gallicam et Germānicam, sīc linguam Latīnam, illī optimē intellegunt quī nōn modō legunt {{nowrap|scrībunt-ve}}, sed etiam dīcunt. Nōnne enim lingua est membrum quō hominēs dīcunt?
Forsitan respondeās: Gallicē quidem vel Germānicē loquī volumus, quia Gallī {{nowrap|Germānī-que}} adhuc vīvunt, {{nowrap|nōbīs-que}} respondēre possunt. Cūr autem Latīnē loquī oportet, cum Rōmānī iamdiū mortuī sint? At negō Rōmānōs mortuōs esse, sīquidem verba et facta eōrum repetās, dum Catullum vel Virgīniam vel ipsum Catōnem tē esse simulēs. Hāc dē causā fabulās paucās {{nowrap|brevēs-que}} composuī, quās dum agitis, Rōmānī {{nowrap|Rōmānae-que}} esse vidēbiminī. Nē fortē negētis tālēs fabulās ā puellīs {{nowrap|puerīs-ve}} agī posse, āiō ferē omnēs aut ab amīcīs meīs adultīs, aut ā discipulīs, iam anteā aetās esse.
{{center|{{sc|Valēte.}}}}<noinclude><references/>
{{c|9}}</noinclude>
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<noinclude><pagequality level="4" user="PWidergren" /></noinclude>{{center|{{x-larger|Colloquium “Passer Mortuus”}}}}
{|style="margin-left: auto; margin-right: auto;
|-
| {{sc|Catullus}} || {{***|4|char=.|1em}} || Poēta
|-
| {{sc|Lesbia}} || {{***|4|char=.|1em}} || Mulier Romāna
|}
{{Center|''(Catullus Lesbiam salūtātum venit, quam flentem cōnspicit.))''}}
''Catullus.'' Salvē, Lesbia mea cārissima. Ēheu! Quid factum est? Nam oculī tuī flendō rubent.
''Lesbia.'' Ō mī Catulle! amīce cārissime. Ecce! passer meus mortuus est. Ō mē miseram!
''Catullus.'' Væ factum male! Morbō-ne dēcēssit, an fēlis eum necāvit?
''Lesbia.'' Nesciō equidem quōmodo mortuus sit. Illud sōlum prō certō habeō: herī passer misellus in gremiō meō circumsiliēbat, ad mē pipilābat, sīcut solēbat; hodiē ancilla mea eum humī iacentem invēnit. Vae miselle passer!
''Catullus.'' Nōnne cum māgnopere amābās, puella mea?
''Lesbia.'' Ita vērō: plūs quam oculōs meōs eam amābam.
{{nop}}<noinclude><references/>
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<div class=text>
{{titulus
|Scriptor= Euphemia Ryle
|OperaeTitulus=Ōlim
|OperaeWikiPagina=
|Annus= 1914
|SubTitulus=
|Liber=Olim Ludi Scaenici.pdf
|Genera=Theatrum, Textus ad discendam linguam latinam
}}
{{Liber
|Ante=
|AnteNomen=
|Post= Preface
|PostNomen= Ólim/Preface
}}
<pages index="Olim Ludi Scaenici.pdf" from=4 to=7 />
<br/>
{|style="margin-left: auto; margin-right: auto;
|-
| [[/Preface|{{sc|Preface}}]]
|-
| [[/Prooemium|{{sc|Prooemium}}]]
|-
| [[/Colloquium: “Passer Mortuus”|{{sc|Colloquium: “Passer Mortuus”}}]]
|-
| [[/Virgínia|{{sc|Virgīnia}}]]
|-
| [[/Vestis sanguine tíncta|{{sc|Vestis sanguine tīncta}}]]
|-
| [[/Léx Oppia|{{sc|Lēx Oppia}}]]
|-
| [[/Lúdi Magister|{{sc|Lūdi Magister}}]]
|-
| [[/Imber Impendet|{{sc|Imber Impendet}}]]
|}
{{Liber
|Ante=
|AnteNomen=
|Post= Preface
|PostNomen= Ólim/Preface
}}
</div>
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<noinclude><pagequality level="4" user="PWidergren" /></noinclude>{{center|{{x-larger|“VESTIS SANGUINE TĪNCTA”}}}}
{{center|''Drāmatis Personae.''}}
{|style="margin-left: auto; margin-right: auto;
|-
|| || {{sc|Pȳramus}} || {{***|3|char=.|2em}} || iuvenis Balylōnius.
|-
|| || {{sc|Thisbē}} || {{***|3|char=.|2em}} || virgō Babylōnia.
|-
|rowspan="2"|[[Imago:Bracket left 4.png|4px]]||colspan="2"| Pater Pȳramī. ||
|-
|colspan="2"| Māter Pȳamī. ||
|-
|rowspan="2"|[[Imago:Bracket left 4.png|4px]]||colspan="2"| Pater Thisbēs. ||
|-
|colspan="2"| Māter Thisbēs. ||
|-
|||colspan="2"|II. Puellae Babylōniae. ||
|}
{{center|''(Domūs Pȳramí et Thisbēs contiguae sunt.)''}}
{{center|{{larger|{{sc|Scaena Prīma.}}}}}}
{{center|''(Extrā casīs contiguās.)''}}
{{center|''(Intrat Thisbē cum duābus puellīs.)''}}
''Thisbē'' ''(suspírat)''. Hei mihi!
''Puella I''. Dīc nōbīs, Thisbē, quamobrem suspīrēs.
''Puella II''. Cūr numquam nōbīscum lūdis, ut anteā solēbās?
''Thisbē''. Nesciō quae sit mihi causa trīstitiae.
''Puella I''. Pȳramum equidem crēdō causam esse.
''Puella II''. Gaudēre tē oportet, nam haud dubium est quīn ille tē cēterīs puellīs praeferat.
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<noinclude><pagequality level="4" user="PWidergren" />{{rh|34|ŌLIM|}}</noinclude>''Catō''. Quid? Mulierēs etiam in pūblicō convenīre, et magistrātūs adīre et appellāre audent? Prō pudor! Statim discēdant, domum redeant! Dīc mē cum eīs loquī omnīnō nōlle. ''(Dāvus exit.)'' Minus cum fēminīs negōtiī habērēmus, sī iūs suum et māiestātem retinērent virī. Nunc autem{{bar|1}}''(Dāvus redit.)''
''Dāvus''. Sī tēcum loquī nōn liceat, ōrant ut hoc volūmen ēvolvās, perlegās. Inde intellegēs quid petant. In līmine tuō manēre cōnstituērunt, dōnec respōnsum ā tē accēperint.
''Catō''. Dī tantam impudentiam pūniant! Dā mihi volūmen. Quid in eō scrīptum est? ''(Recitat.)''
“Consulī Mārcō Porciō Catōní mātrōnae {{nowrap|cēterae-que}} mulierēs Rōmānae salūtem dīcunt. Vīgintī iam annōs mulierēs Rōmānae iniūriās lēgis Oppiae tulimus. Nec plūs sēmūnciam aurī habēre, nec vestīmentō versicolōrī ūtī, nec iūnctō vehiculō in urbe {{nowrap|oppidō-ve,}} nisi sacrōrum pūblicōrum causā, vehī licet. Cūr sit lāta lēx, bene scīmus: Hannibal in Ītaliā erat, victor ad Cannās; Tarentum, Arpōs, Capuam iam habēbat; ad urbem ipsam admōtūrus exercitum vidēbātur; Rōmānī omnibus subsidiīs egēbant. Nōn ad coercendam lūxuriam mulierum lēx lāta est, sed quia omnium prīvātōrum pecūniae in ūsum pūblicum vertendae erant. Nunc autem cum flōret rēs pūblica, crēscit in diēs prīvāta omnium fortūna,<noinclude><references/></noinclude>
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<noinclude><pagequality level="4" user="PWidergren" /></noinclude>ōrāmus ut prīstinus ōrnātus nōbīs reddátur. Illud quoque animadvertendum: mulierēs eīs prīvantur quae virīs {{nowrap|puerīs-que}} permīttuntur. Virī enim purpurā, ūtuntur, praetextāti in magistrātibus, in sacerdōtiīs; līberī nostrī praetextātīs purpurā togīs ūtuntur; etiam equī speciōsius instrātī sunt quam uxōrēs vestītae.
Immō vērō, sociōrum Latīnī nōminis uxōribus vidēmus ea concēssa ōrnāmenta quae nōbīs sunt adempta: illae vehuntur per urbem, nōs pedibus sequimur. Haec nōn ferenda sunt, neque ā nōbīs diūtius ferentur. Prōmītte, igitur, fore ut lēx Oppia quam prīmum abrogētur.”
{{bar|1}}Ēdepol! Quis iūris cōnsultus haec scrīpsit?
''Dāvus''. Vīs-ne mulieribus illīs respondeam? Metuō nē totam noctem tē manēre cōnstituerint.
''Catō''. Imperā eīs ut statim discēdant; nam prius lupī āgnōs fugient quam ego fēminīs cēdam. ''(Exit Dāvus.)'' Dī immortālēs! Ubinam gentium sumus? Quam rempūblicam habēmus, sī domī meae ā mulieribus cōnsul ego obsideor?
''(Dāvus redit.)''
''Dāvus''. Abscēssērunt, ut iussistī, sed vereor nē quās insidiās parent; minimē amīcē dē tē locūtae sunt.
''Catō'', Nīl timeó. Sed nox adest, et lucernīs parcere soleō: eāmus igitur dormītum.
{{dextra|[''Exeunt.''}}
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<noinclude><pagequality level="4" user="PWidergren" />{{rh||LĒX OPPIA|41}}</noinclude>''M. I. B''. Tacē tū. Cōnsulem audī.
''Catō''. Nostram ob culpam, dīcō, Quirītēs, tantum cum ūniversīs fēminīs negōtiī habēmus; domī enim ab eīs victa est lībertās nostra.
''Aurēlia''. At fēminae lībertātem nōn habent.{{bar|1}}
''T. I. B''. Tacē tū.
''Catō''. Haec cōnsternātiō muliebris, sīve suā sponte, sīve auctōribus vōbīs, Mārce Fundānī et Lūcī Valerī, facta est, haud dubiē ad culpam magistrātuum pertinet.
''Claudia''. Haud dubiē, cum{{bar|1}}
''Catō''. Dēdecorī sit nōbīs, sī, ut plēbis quondam, sīc nunc mulierum sēcēssiōne, lēgēs accipīendae vel abrogandae sint.
''Fundānia''. Dēdecorī sit vōbīs nisi lēx Oppia abrogētur.
''M. I. B''. Tacē, mulier.
''Catō''. Sed quī hic mōs est in pūblicum procurrendī et obsidendī viās, et virōs aliēnōs appellandī? Illud ipsum suōs quaeque domī rogāre nōn potuērunt? Quamquam nē domī quidem lēgēs rogandās {{nowrap|abrogandās-ve}} cūrāre decuit. Māiōrēs nostrī fēminās nē privātam quidem rem per sē agere voluērunt, sed in manū esse parentum, frātrum, virōrum. Nōs iam etiam rem pūblicam capessere patimur.
''Omnēs mulierēs''. Sānē. Iūs suffrāgiī mulieribus permittendum est!
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<noinclude><pagequality level="4" user="PWidergren" />{{rh|42|ŌLIM|}}</noinclude>''T. I. B''. Tacēte, vōs.
''Catō''. Sed nunc ipsam ad lēgem Oppiam veniō. Cūr fēminae hanc lēgem abrogārī cupiunt? Porrō, ut aurō et purpurā fulgeant, ut carpentīs per urbem vehantur, ut nūllus sit modus sūmptibus {{nowrap|lūxuriæ-ve}}. Saepe mē audīvistis dē fēminārum sūmptibus querentem, saepe dē virōrum{{bar|1}}
''Iūlia''. Vēra dīxistí. Saepius audīvimus.
''M. I. B''. Tacē, fēmina.
''Catō''. Dīcō nimiam lūxuriam iamnunc cīvitātī inesse: sīn autem retinācula hūius lēgis remōta erunt, nec modus nec fīnis erit sūmptibus. Ego nūllō modō abrogandam lēgem cēnseō.
''Mulierēs''. Prō pudor!
''Valerius''. Pauca respondēre mē oportet. Questus es, Mārce Catō, in pūblicum vēnisse mulierēs. Nōn dēbuistī eās reprehendere, sī in causā propriē ad ipsās pertinentī id fēcērunt. Quid tamen fēcērunt, nisi quod supplicēs nōs adiērunt? Superbās, medius fidius, aurēs habēmus, sī, cum dominī servōrum nōn fāstīdiant precēs, nōs rogārī ab honestīs fēminīs indīgnāmur. Fēminās audiendās cēnseō.
''Fundānius''. Mihi etiam quaedam dīcenda sunt. Utrum sit cīvitātī nimia lūxuria necne, nesciō. Sed sīve ita est, sīve nōn est, cūr sōlae fēminae lēge coercendae? Aut virīs quoque modum impōne, aut fēminīs adime. Egomet lēgem abrogandam cēnseō.
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<noinclude><pagequality level="4" user="PWidergren" />{{rh||LĒX OPPIA|43}}</noinclude>''Mulierēs''. Euge Fundāní! Optimē dīxistī.
''Catō''. Nōn in forō, sed in cūriā, dē hāc rē disputandum est nōbīs. Hīc maneant fēminae. Nōs ad cūriam eāmus.
{{dextra|[''Exeunt virī.''}}
''Flāvia''. Dī rem prosperē gerant!
{{center|{{sc|Scaena Quārta.}} ''(Extrā Brūtōrum aedēs.)''}}
{{center|''(Intrant Mārcus Brūtus et Titus Brūtus.)''}}
''M. I. B''. Rogātiōnī collēgārum nostrōrum intercēssimus, ego et tū.
''T. I. B''. Ita vērō. Potēns vōx est “Vetō” …
''M. I. B''. Ecquid audīs? Turba hominum appropinquēre vidētur.
''T. I. B''. Intrō eāmus{{bar|1}}festīnemus{{bar|1}}mulierēs illae nōs persequuntur!
{{dextra|[''Domum citō intrant.''}}
{{center|''(Mulierēs ad aedēs perveniunt.)''}}
''Flāvia''. Haec est domus Brūtōrum.
''Iūlia''. Forēs pulsā, Aurēlia.
{{dextra|[''Aurēlia pulsat.''}}
''Claudia''. Iānuam aperīre eōs iubē.
''Aurēlia''. Mārce Brūte! Tite Brūte! Aperīte iānuam!
''Fundānia''. Abscēdere nōlumus, dōnec ad nōs veniētis.
{{center|''(M. et T. Brūtī ad fenestram appārent.)''}}
''M. I. B''. Quid est, dominae?
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<noinclude><pagequality level="4" user="PWidergren" />{{rh|44|ŌLIM|}}</noinclude>''T. I. B''. Ecquid vultis, dominae?
''Flāvia''. Iānuās vestrās obsidēre nōn ante dēsinēmus quam intercēssiō ā vōbīs remōta erit.
''M. I. B''. Nōs minīs movērī crēditis?
''T. I. B''. In vincula dūcēminī, nisi statim abībitis.
''Iūlia''. Vincula nōn timēmus.
''Fundānia''. Immō vērō, vinculīs nōs ipsās ad postēs vestrōs ligābimus, nē quis nōs abdūcere possit.
''Claudia''. Lapidēs per fenestrās vestrās cōniciēmus.
''Aurēlia''. Facēs parātās habeō. Quīn aedēs ipsās incendimus?
''Flāvia''. Omnēs tabellāriōs opperiēmur, quī lītterās vōbīs adferunt; epistulās ātrō aliquō venēnō ita corrumpēmus ut legī nōn possint.
''M. I. B''. Tite, quid fierī oportet?
''T. I. B''. Mārce, quid tū faciendum esse putās?
''M. I. B''. Illīs mōrem gerere mālō quam domī meae obsidērī.
''T. I. B''. Vīs-ne remīttārus intercēssiōnem nostram?
''M. I. B''. Ita. Remittere cam praestat.
''Ambō''. Remīttimus intercēssiōnem.
''Mulierēs''. Intercēssiōnem remittunt! Iam abrogābitur lēx Oppia. Iō triumphe!
''Flāvia''. Domum redeāmus ut purpuram aurum-<noinclude><references/></noinclude>
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<noinclude><pagequality level="4" user="PWidergren" />{{rh||LĒX OPPIA|45}}</noinclude>que statim induāmus. Catōnem superāvimus mulierēs.
''Claudia''. Fortasse aliquandō etiam suffrāgiī iūs nōbīs permīttētur.
''Omnēs''. Intereā, nōniam lēge Oppiā continēbimur.
{{dextra|[''Exeunt.''}}
{{center|FĪNIS}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="4" user="PWidergren" />{{rh||LŪDI MAGISTER|49}}</noinclude>''Mārtiālis''.
<div style="margin-left:3em"><poem>“Quid tibi nōbīscum est, lūdī scelerāte magister,
:invīsum puerīs virginibus-que caput?
Nōndum cristātī rūpēre silentia gallī:
:murmure iam saevō verberibus-que tonās.
Tam grave percussīs incūdibus aera resultant,
:causidicum mediō cum faber aptat equō:
Mītior in māgnō clāmor furit amphitheātrō,
:vincentī parmae cum sua turba favet.
Vīcīnī somnum{{bar|1}}nōn tōtā nocte{{bar|1}}rogāmus,
:nam vigilāre leve est, pervigilāre grave est.
Discipulōs dīmītte tuōs. Vīs, garrule, quantum
:accipis ut clāmēs, accipere ut taceās?”
</poem></div>
''Iuvenālis''. Euge! Scrībe nunciam, et ad vīcīnum illum molestum mītte.
''Mārtiālis''. Hoc faciam.
''Iuvenālis'' Valē, mī amīce. Ut tandem quiēscās!
''Mārtiālis''. Valē, Ō Iuvenālis.
{{center|FĪNIS.}}<noinclude><references/></noinclude>
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Liber:Campanella, Tommaso – Poesie, 1915 – BEIC 1777758.djvu
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{{:MediaWiki:Proofreadpage_index_template
|Author=[[Scriptor:Thomas Campanella|Tommaso Campanella]]
|Title=Poesie (1915)
|Year=1915
|Publisher=Laterza
|Source={{IA|070CampanellaPoesieSi065}}
|Image=[[File:Campanella, Tommaso – Poesie, 1915 – BEIC 1777758.djvu|200px|page=5]]
|Pages=<pagelist
1to6=-
7=1
326to328=-
/>
|Remarks=[[Ecloga in principis Galliarum Delphini admirandam nativitatem]] (pag. [[Pagina:Campanella, Tommaso – Poesie, 1915 – BEIC 1777758.djvu/199|193]] - [[Pagina:Campanella, Tommaso – Poesie, 1915 – BEIC 1777758.djvu/214|208]])
See also [[:it:Index:{{PAGENAME}}]][[Category:La-it index pages]]
[[it:Index:{{PAGENAME}}]]
}}
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<noinclude><pagequality level="3" user="PWidergren" />{{rh|52|LUDI CIRCENSES|}}</noinclude>''B.'' In Britannia quoque pueros mittere solēmus qui tāli mūnere fungantur quōtiēs in theātrō locos vīli emere volumus.
{{***}}
''R.'' Ēn Circum Maximum.<ref>'''Circum Maximum.''' The Circus Maximus was a recreation ground laid out by Tarquintus Priscus in the valley between the Palatine and Aventine hills, south of the Capitol. It was enlarged by Caesar.</ref>
''B.'' Rēs vērē immānis. Apud nōs nihil simile est. Quot cīvibus licet lūdos simul spectāre?
''R.'' Ducenta quīnquāgintā millia.
''B.'' Nos vīginti millia, ad hūiusmodi lūdum congregāta, numerum aestimāmus ūnicum.
''R.'' Circus est sescentos passūs longus et ducentos lātus. Sed in eo est ut prīmum ineant curriculum.
''B.'' Quārē prō equīs claustra illa ōbiciuntur?
''R.'' Carceres appellantur, quibus sublātis, equi in curriculum prōruunt. Hīc missus est septem spatiōrum, id est circā trium millium passuum. Hōc ūnum velim tibi dīcere, priusquam ē carceribus mittentur. Ille humilis mūrus, in medio situs et statuis ornātus, spīna appellātur, cūius ad utrumque finēm est mēta, tribus columnis insignis. Sed, ēn, consul<ref>'''consul.''' The giver of the games entered the Circus at the head of a triumphal procession, and presided. He started the races.</ref> mappam albam dīmīsit.
{{nop}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="PWidergren" />{{rh||LUDI CIRCENSES|53}}</noinclude>B. Ēvax, mittuntur quattuor quadrīgae! Quam parvi vīdentur et leves currūs, duōbus rotis sublīmes lāti! Sed cūr quadrīgārius cultrum in balteo habet?
R. Ut, si quid infēlīciter accidat, habēnas secet quae post tergum sunt.
{{c|{{Hic est imago}}}}
{{c|{{sc|Chariot Race in a Roman Circus.}}}}
B. Quā ratiōne currūs et agitātōrum vestīmenta varios ostendunt colōres?
R. Quattuor societātes, quae et equos ct currus possident, quattuor colōribus distinguuntur. Factiōnes eōrum qui societāti ūnīcuīque favent nōmine vocantur albāta, russāta, prasina, veneta.
{{nop}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="PWidergren" />{{rh||LUDI CIRCENSES|53}}</noinclude>''B.'' Ēvax, mittuntur quattuor quadrīgae! Quam parvi vīdentur et leves currūs, duōbus rotis sublīmes lāti! Sed cūr quadrīgārius cultrum in balteo habet?
''R.'' Ut, si quid infēlīciter accidat, habēnas secet quae post tergum sunt.
{{c|{{Hic est imago}}}}
{{c|{{sc|Chariot Race in a Roman Circus.}}}}
''B.'' Quā ratiōne currūs et agitātōrum vestīmenta varios ostendunt colōres?
''R.'' Quattuor societātes, quae et equos et currus possident, quattuor colōribus distinguuntur. Factiōnes eōrum qui societāti ūnīcuīque favent nōmine vocantur albāta, russāta, prasina, veneta.
{{nop}}<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="PWidergren" />{{rh|54|LUDI CIRCENSES}}</noinclude>''B.'' Mihi quidem vidētur veneta numero māior, et quadrīga veneta currit proxima spīnae.
''R.'' Prasina autem, mēhercle, interiōrem adfectābit locum ad prīmam mētam.
''B.'' Iam iam mētae propinquat. O rem perīculōsam!
''R.'' Ita, Profecto venetā propius spīnam rādit. Heu, rota icta est, currus perculsus … sed ipse incolumis.
''B.'' Prasina iam prior, albāta prope sequitur.
''R.'' Vidēn ut servus ille ē septem sextam pilam<ref>'''pilam.''' These were seven egg-shaped objects on a pedestal. To keep the spectators informed how many heats had been run, one was taken down after each lap.</ref> dēmat: spatium ineunt ultimum.
''B.'' Vehementer commoventur omnes! Quadrīgārii in ultimum certāmen equos verberant!
''R.'' Actum est, Russata tamen albam līneam<ref>'''lineam.''' A chalk line drawn across the ground near the entrance.</ref> prīma transiit.
''B.'' Quid sibi reportat victor?
''R.'' Īlicet vidēbis. Iam prōcēdit, ad consulem dēductus. Magnam pecūniam aufert. … Iam equos agitat per portam vīctōribus reservātam.
''B.'' Hōc certāmine animus mihi valdē commovēbātur.
{{nop}}<noinclude><references/></noinclude>
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Patrologia Latina/Scriptores
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{{titulus2
|Scriptor=Iacobus Paulus Migne
|OperaeTitulus=Patrologia Latina
|OperaeWikiPagina=Patrologia Latina/Scriptores
|Annus= 1844
|SubTitulus=Scriptores
|Genera=
|Editio=Migne 1844
|Fons=[http://www.documentacatholicaomnia.eu/30_10_De_Latinis_Scriptoribus.html Documenta Catholica Omnia]
}}
* 0050-0150- [[Scriptor:Pseudo Clemens|Pseudo Clemens]]
* 0100-0200- [[Scriptor:Minucius Felix|Minucius Felix]]
* 0129-0216- [[Scriptor:Claudius Galenus|Galenus Claudius]]
* 0150-0250- [[Scriptor:Alexander Aphrodisiensis|Alexander Aphrodisiensis]]
* 0160-0220- [[Scriptor:Tertullianus|Tertullianus]]
* 0180-0254- [[Scriptor:Hippolytus Romanus|Hippolytus Romanus]]
* 0200-0300- [[Scriptor:Antonius|Antonius]]
* 0200-0300- [[Scriptor:Arnobius|Arnobius Afrus]]
* 0200-0300- [[Scriptor:Commodianus Gazaeus|Commodianus]]
* 0200-0300- [[Scriptor:Magnetes|Magnetes]]
* 0200-0300- [[Scriptor:Minucius Felix|Minucius Felix]]
* 0201-0300- Auctores Incerti
* 0240-0300- [[Scriptor:Victorinus Petavionensis|Victorinus]]
* 0240-0320- [[Lucius Caelius Firmianus Lactantius|Lactantius]]
* 0243-0243- [[Scriptor:Morcellus|Morcellus]]
* 0250-0350- [[Scriptor:Celsus|Celsus]]
* 0250-0350- [[Scriptor:Macarius Nitriensis|Macarius Nitriensis]]
* 0251-0251- [[Scriptor:Maximus|Maximus]], [[Scriptor:Sidonius|Sidonius]] , Macharius
* 0251-0258- [[Scriptor:Novatianus|Novatianus]]
* 0258-0258- [[Scriptor:Victorius Aquitanus|Victorius Aquitanus]]
* 0280-0330- [[Scriptor:Eumenius Augustodunensis|Eumenius]]
* 0280-0380- [[Scriptor:Publilius Optatianus Porfirius|Optatianus Porphyrius]]
* 0283-0371- [[Scriptor:Eusebius Vercellensis|Eusebius Vercellenses]]
* 0292-0348- [[Scriptor:Pachomius Tabennisiensis|Pachomius Abbas Tabennense]]
* 0300-0400- [[Scriptor:Drepanius Florus|Drepanius Florus]]
* 0300-0400- [[Scriptor:Grimlaicus presbyter|Grimlaicus Presbyter]]
* 0300-0400- [[Scriptor:Severus Minoricensis|Severus Minoricensis]]
* 0301-0400- Auctores Incerti
* 0307-0307- [[Scriptor:Sigonius|Sigonius]]
* 0308-0346- [[Scriptor:Orsiesius|Orsiesius Abbas Tabennense]]
* 0310-0370- [[Scriptor:Osius Cordubensis|Osius Cordubensi Episcopus]]
* 0310-0380- [[Scriptor:Orsiesius|Orsiesius]]
* 0310-0380- [[Scriptor:Zeno Veronensis|Zeno]]
* 0310-0383- [[Scriptor:Ulfilas|Ulfila]]
* 0312-0337- [[Scriptor:Constantinus I|Constantinus Imperator]]
* 0314-0360- [[Scriptor:Iulius Firmicus Maternus|Firmicius Maternus]]
* 0317-0397- [[Scriptor:Martinus Turonensis|Martinus Episcopus Turonensis]]
* 0321-0321- [[Scriptor:Nazarius|Nazarius]]
* 0323-0387- [[Scriptor:Optatus Milevitanus|Optatus Afrus]]
* 0328-0391- [[Scriptor:Phoebaudius Aginensis|Phoebaudius Aginensis Episcopus]]
* 0330-0340- [[Isaia Abbas|Isaia Abbas]]
* 0335-0414- [[Scriptor:Nicetas Aquileiensis|Nicetas Aquileiensis Episcopus]]
* 0336-0399- [[Scriptor:Aurelius Carthaginensis|Aurelius Carthaginenses]]
* 0340-0402- [[Scriptor:Quintus Aurelius Symmachus|Aurelius Symmachus]]
* 0341-0397- [[Scriptor:Philastrius Brixiensis|Philastrius Episcopus]]
* 0342-0342- [[Scriptor:Coelius Sedulius|Coelius Sedulius]]
* 0347-0354- [[Scriptor:Lucifer Calaritanus|Lucifer Episcopus]]
* 0348-0413- [[Scriptor:Aurelius Prudentius Clemens|Aurelius Prudentius]]
* 0350-0450- [[Scriptor:Anastasius III (antipapa)|Anastasius Bibliothecarius]]
* 0350-0450- [[Scriptor:Decimus Magnus Ausonius|Ausonius Decimus]]
* 0350-0450- [[Scriptor:Avitus presbyter|Avitus Presbyter]]
* 0350-0450- [[Scriptor:Eucherius Lugdunensis|Eucherius Arelatus]]
* 0350-0450- [[Scriptor:Fastidius Britanniae|Fastidius Episcopus]]
* 0350-0450- [[Scriptor:Maximus Grammaticus]]
* 0350-0450- [[Scriptor:Novatus Catholicus|Novantius Catholicus]]
* 0350-0450- [[Scriptor:Publius Victor|Publius Victor]]
* 0350-0450- [[Scriptor:Quodvultdeus|Quodvultdeus]]
* 0350-0450- [[Scriptor:Secundinus Manichaeus|Secundinus Manichaeus]]
* 0350-0450- [[Scriptor:Severus Rhetor|Severus Rhetor]]
* 0350-0450- [[Scriptor:Tichonius Afer|Tichonius Afer]]
* 0350-0450- [[Scriptor:Valentinus|Valentinus]]
* 0350-0450- [[Scriptor:Valeria Faltonia Proba|Valeria Faltonia Proba]]
* 0350-0450- [[Scriptor:Vettius Aquilinus Juvencus|Vettius Aquilius Juvencus]]
* 0353-0431- [[Scriptor:Paulinus Nolanus|Paulinus Nolanus Episcopus]]
* 0354-0354- [[Scriptor:Dionysius Filocalus|Furius Dionysius Filocalus]]
* 0354-0430- [[Scriptor:Lucianus presbyter|Lucianus Presbyter Caphamargalae]]
* 0360-0406- [[Scriptor:Cromatius Aquileiensis|Cromatius Episcopus Aquileiensis]]
* 0360-0420- [[Scriptor:Sulpicius Severus|Sulpicius Severus]]
* 0360-0430- [[Scriptor:Bachiarius Hispaniae|Bacharius Monachus]]
* 0360-0430- [[Scriptor:Evagrius monachus|Evagrius Monachus]]
* 0360-0430- [[Scriptor:Pelagius Britannicus|Pelagius Britannicus]]
* 0360-0430- [[Scriptor:Zacchaeus Christianus|Zacchaeus Christianus]]
* 0360-0435- [[Scriptor:Iohannes Cassianus|Cassianus Ioannes]]
* 0362-0362- [[Scriptor:Mamertinus|Mamertinus Claudius]]
* 0362-0372- [[Scriptor:Victorinus Petavionensis|Victorinus Afrus]]
* 0366-0366- [[Scriptor:Potamius Ulyssiponensis|Potamius Episcopus]]
* 0368-0384- [[Scriptor:Faustinus|Faustinus]]
* 0368-0384- [[Scriptor:Vigilius Tridentinus|Vigilius Episcopus]]
* 0370-0418- [[Scriptor:Paulinus Mediolanensis|Paulinus Mediolanensis]]
* 0370-0430- [[Scriptor:Aurelius Carthaginensis|Aurelius Episcopus Carthaginensis]]
* 0370-0430- [[Scriptor:Gaudentius Brixiensis|Gaudentius]] Brixiae Episcopus
* 0370-0450- [[Scriptor:Vincentius Lirinensis|Vincentius Lirinensis]]
* 0370-0470- [[Scriptor:Maximus Taurinensis|Maximus Taurinensis]] Episcopus
* 0371-0444- [[Scriptor:Flavius Lucius Dexter|Flavius Lucius Dexter]]
* 0380-0394- [[Scriptor:Theodosius|Theodosius]]
* 0380-0450- [[Scriptor:Eucherius Lugdunensis|Eucherius Lugdonensis]] Episcopus
* 0380-0450- [[Scriptor:Petrus Chrysologus|Petrus Chrysologus]]
* 0380-0450- [[Scriptor:Vincentius Lirinensis|Vincentius Lerinus]]
* 0381-0398- [[Scriptor:Vigilius Tridentinus|Vigilius Episcopus]]
* 0385-0420- [[Scriptor:Orosius]]
* 0385-0445- [[Scriptor:Claudius Marius Victor|Claudius Marius Victor]] (Victorinus)
* 0387-0493- [[Scriptor:Patricius]], Sanctus
* 0388-0468- [[Scriptor:Idatius Aquae Flaviensis|Idatius Aquaeflaviensis]] Episcopus
* 0390-0420- [[Scriptor:Paulus Orosius|Paulus Orosius]]
* 0390-0451- [[Scriptor:Marius Mercator|Marius Mercator]]
* 0390-0463- [[Scriptor:Prosper Tiro Aquitanus|Prosperus Aquitanus]]
* 0397-0397- [[Scriptor:Pacianus Barcilonensis|Pacianus]]
* 0397-0435- [[Scriptor:Possidius Calamensis|Possidus Calamensis]] Episcopus
* 0400-0469- [[Scriptor:Idatius Aquae Flaviensis|Hydatius]]
* 0400-0470- [[Scriptor:Salvianus Massiliensis|Salvianus Massiliensis]] Episcopus
* 0400-0473- [[Scriptor:Mamertus Claudianus|Mamertus Claudianus]]
* 0400-0500- [[Scriptor:Arnobius|Arnobius]]
* 0400-0500- [[Scriptor:Dracontius Blossius|Dracontius Blossius]]s Aemilius
* 0400-0500- [[Scriptor:Julius Hilarianus]]
* 0400-0500- [[Scriptor:Merobaudes Scholasticus|Merobaudus Flavius]]
* 0400-0500- [[Scriptor:Valerianus Cemeliensis]] Episcopus
* 0401-0449- [[Scriptor:Hilarius Arelatensis|Hilarius Arelatensis]] Episcopus
* 0401-0500- Auctores Incerti
* 0408-0450- Scriptor:Thedosius Imperator II
* 0410-0470- Scriptor:Annaeus Sylvius Episcopus Octodurensis
* 0410-0470- [[Scriptor:Paschasinus Lillybaetanus|Paschasinus Lillybaetanus]] Episcopus
* 0410-0470- [[Scriptor:Turribius Austricensis|Turribius Austricensis]] Episcopus
* 0419-0479- [[Scriptor:Lupus Trecensis|Lupus Trecensis]] Episcopus
* 0425-0490- [[Scriptor:Faustus Rhegiensis|Faustus Rhegiensis]] Episcopus
* 0426-0426- [[Scriptor:Leporius monachus|Leporius monachus]]
* 0426-0432- [[Scriptor:Capreolus Carthaginensis|Capreolus Carthaginensis]]
* 0428-0428- [[Scriptor:Merobaudes Scholasticus|Merobaudes]] Scholasticus
* 0428-0530- [[Scriptor:Theodosius II|Scriptor:Theodosius]] Imperator
* 0430-0430- [[Scriptor:Possidius Calamensis|Scriptor:Possidius]] Episcopus
* 0430-0484- [[Scriptor:Victor Vitensis|Victor Vitensis]]
* 0430-0489- [[Scriptor:Sidonius Apollinaris|Sidonius Apollinaris]] Episcopus
* 0430-0490- [[Scriptor:Iulianus Pomerius|Julianus Pomerius]]
* 0432-0432- [[Scriptor:Uranius presbyter|Scriptor:Uranius Presbyter]]
* 0438-0438- [[Scriptor:Antoninus Honoratus|Antoninus Honoratus]] Episcopus
* 0439-0521- [[Scriptor:Brigida|Brigida]]
* 0447-0507- [[Scriptor:Ruricius|Ruricius Lemovicensis]] Episcopus
* 0448-0448- [[Scriptor:Polemeus Sylvius|Polemeus]] Silvius
* 0450-0450- [[Scriptor:Eustathius|Eustathius]]
* 0450-0450- [[Scriptor:Orientius |Orientius Ausciensis]] Episcopus
* 0450-0525- Scriptor:Dionigi lo pseudo-Areopagita
* 0450-0550- [[Scriptor:Albericus Diaconus|Albericus Diaconus]]
* 0450-0550- [[Scriptor:Eugyppius|Eugyppius]]. Abbas Africanus
* 0450-0550- [[Scriptor:Faustinus|Faustinus]]
* 0450-0550- [[Scriptor:Ferreolus Ucetienses|Ferreolus Ucetienses]] Episcopus
* 0450-0550- [[Scriptor:Gennadius Massiliensis|Gennadius Massiliensis]]
* 0450-0550- Scriptor:Sancti Paulus Et Stefanus Abbati
* 0451-0457- [[Scriptor:Proterius Alexandrinus|Proterius Alexandrinus]] Episcopus
* 0453-0453- [[Scriptor:Salonius Viennensis|Salonius Viennensis]] Episcopus
* 0454-0526- [[Scriptor:Theodoricus Rex Gothorum|Theodoricus Rex Gothorum]]
* 0456-0531- [[Scriptor:Eleutherius |Eleutherius Tornacensis]]
* 0460-0518- [[Scriptor:Avitus Viennensis|Avitus Viennensis]] Episcopus
* 0460-0538- [[Scriptor:Eugippius|Eugippus]]
* 0466-0511- [[Scriptor:Clodoveus I Rex Francorum|Clodoveus I]] Rex Francorum
* 0467-0532- [[Scriptor:Fulgentius Ruspensis|Fulgentius Ruspensis]] Episcopus
* 0468-0542- [[Scriptor:Caesarius Arelatensis]] Episcopus
* 0470-0470- [[Scriptor:Auspicius Tullensis]] Episcopus
* 0470-0523- [[Scriptor:Eugenius Carthaginensis]] Episcopus
* 0470-0544- [[Scriptor:Dionysius Exiguus|Dionysius Exiguus]]
* 0474-0521- [[Scriptor:Ennodius Ticinensis|Magnus Felix Ennodius]]
* 0474-0534- [[Scriptor:Marcellinus comes|Marcellinus Comes]]
* 0479-0516- [[Scriptor:Gundebaldus Rex Francorum|Gundebaldus Rex Francorum]]
* 0480-0524- [[Scriptor:Anicius Manlius Torquatus Severinus Boethius|Boethius]], Severinus
* 0480-0524- [[Scriptor:Elpis Uxor Boethii|Elpis Uxor Boethii]]
* 0482-0482- [[Scriptor:Perpetuus Turonensis]] Episcopus
* 0482-0565- [[Scriptor:Justinianus|Justinianus]] Imperator
* 0485-0485- [[Scriptor:Cerealis Castellinensis|Cerealis Castellinensis]] Episcopus
* 0485-0585- [[Cassiodorus Vivariensis|Cassiodorus Vivariensi]]s Abbas
* 0489-0533- [[Scriptor:Remigius Rhemensis|Remigius Archiepiscopus]] Remenensis
* 0490-0490- [[Scriptor:Amoenus|Perpetuus Turonensis]]
* 0490-0490- [[Scriptor:Paulinus Petricordiensis|Paulinus Petricordiensis]]
* 0490-0518- [[Scriptor:Avitus Viennensis|Scriptor:Aviturs Viennensis]] Episcopus
* 0490-0583- [[Scriptor:Cassiodorus Flavius]]
* 0491-0512- [[Scriptor:Paschasius Diaconus]]
* 0494-0570- [[Scriptor:Gildas Sapiens]]
* 0496-0496- [[Scriptor:Ioannes Diaconus|Joannis Diaconus]]
* 0497-0561- [[Scriptor:Clotarius I Francorum|Clotarius I]] Rex Francorum
* 0500-0555- [[Scriptor:Ioannes subdiaconus|Vigilius Diachonus]]
* 0500-0585- [[Scriptor:Vigilius Diaconus|Vigilius Diaconus]]
* 0500-0600- [[Scriptor:Alulfus Tornacensis|Alulfus Tornacensis]]
* 0500-0600- [[Scriptor:Amphilocus|Amphilocus]]
* 0500-0600- [[Scriptor:Antonius discipulus Simeonis Stylitae|Scriptor:Antonius Discipulus]]
* 0500-0600- [[Scriptor:Antonius Placentinus|Antonius Placentinus]]
* 0500-0600- [[Scriptor:Ephraem Syrus|Scriptor:Ephraem Archidiaconus]]
* 0500-0600- [[Erchembertus Cassinensis|Erchambertus]]
* 0500-0600- [[Scriptor:Flavius Cresconius Corippus]]
* 0500-0600- [[Scriptor:Florianus|Florianus Abbas]] Romani Monasterii
* 0500-0600- Graecus Incertus
* 0500-0600- [[Scriptor:Heraclides Alexandrinus|Heraclides Alexandrinus]]
* 0500-0600- Scriptor:Jacobus Diaconus
* 0500-0600- [[Scriptor:Joannes Arelatensis|Joannes Arelatensi]]s Episcopus
* 0500-0600- [[Scriptor:Leontius Neapoleos|Leontio Neapoleos]] Cyprorum Episcopus
* 0500-0600- [[Scriptor:Luculentus|Luculentus]]
* 0500-0600- [[Scriptor:Palladius Helenopolitanus|Palladius Helenopolis]] Episcopus
* 0500-0600- [[Scriptor:Paphnutius Aegyptius|Paphnutius Abbas]]
* 0500-0600- [[Scriptor:Severius Sulpicius]] Et Scriptor:Joannes Cassianus
* 0500-0600- [[Scriptor:Sophronius Ierosolymitanus|Scriptor:Sophronius Jerosolymitanus]] Episcopus
* 0500-0600- [[Scriptor:Theophilus|Theophilus]]
* 0501-0600- Auctores Incerti
* 0508-0573- [[Scriptor:Nicetius Trevirensis|Nicetius Trevirensis]] Episcopus
* 0510-0573- [[Scriptor:Martinus Bracarensis|Martinus Dumiensis]] Episcopus Bracarensis
* 0511-0558- [[Scriptor:Chidelbertus II|Chidelbertus]] Rex Francorum
* 0513-0519- [[Scriptor:Petrus Diaconus]]
* 0515-0523- [[Scriptor:Viventulus Lugdunensis]] Episcopus
* 0515-0580- [[Scriptor:Martinus Bracarensis]]
* 0518-0518- [[Scriptor:Vigilius Tapsensis|Vigilius Tapsensis]]
* 0520-0520- [[Scriptor:Rusticus Helpidius]]
* 0520-0587- [[Scriptor:Radegundis regina Francorum|Scriptor:Radegundis]] Regina Franciae
* 0522-0531- [[Scriptor:Montanus Toletanus|Montanus]] Episcopus Toletanus
* 0523-0526- [[Scriptor:Trifolius presbyter|Trifolius Prebyter]]
* 0526-0530- [[Scriptor:Prosper Tiro Aquitanus|Scriptor:Prosperus Conversus]]
* 0530-0594- [[Scriptor:Marius Aventicensis|Marius Aventicensis]] Episcopus
* 0530-0609- [[Scriptor:Venantius Fortunatus|Venantius Fortunatus]]
* 0530-0609- [[Scriptor:Venantius Fortunatus|Venantius Fortunatus]] Episcopus
* 0533-0547- Scriptor:Theodebertus Rex Francorum
* 0534-0601- [[Scriptor:Leandrus Hispalensis]] Episcopus
* 0538-0594- [[Scriptor:Gregorius Turonensis]] Episcopus
* 0540-0540- Scriptor:Junilius Africanus Episcopus
* 0540-0540- Scriptor:Justus Urgellensis Episcopus
* 0540-0540- [[Scriptor:Laurentius Novariensis|Laurentius Novariensis]]
* 0540-0540- [[Scriptor:Pontianus|Pontianus]] Africanus Episcopus
* 0540-0540- [[Scriptor:Troianus Santonensis|Trojanus Santonensis]] Episcopus
* 0546-0551- [[Scriptor:Aurelianus Arelatensis]] Episcopus
* 0547-0547- [[Scriptor:Facondus Hermianensis]] Episcopus
* 0547-0547- [[Scriptor:Fulgentius Ferrandus|Fulgentius Ferrandus]]
* 0547-0555- [[Scriptor:Theobaldus Rex Francorum|Theobaldus Rex Francorum]]
* 0548-0548- [[Scriptor:Leo Senonensis|Leo Senonensis]] Episcopus
* 0549-0549- [[Scriptor:Mapinius Rhemensis|Mapinius Rhemensis]] Episcopus
* 0549-0549- [[Scriptor:Rusticus diaconus|Rusticus Diaconus]]
* 0550-0550- [[Scriptor:Mappinus Rhemensis]] Episcopus
* 0550-0550- [[Scriptor:Primasius Adrumetanus]] Episcopus
* 0550-0550- [[Scriptor:Victor Capuanus]] Episcopus
* 0550-0619- [[Scriptor:Ioannes Moschus]]
* 0550-0650- [[Scriptor:Joannes Biclarensis]] Abbas
* 0551-0551- [[Scriptor:Arator|Arator]] Subdiaconus
* 0551-0551- [[Scriptor:Nicetius Trevirensis|Nicetus Trevirensis Episcopus]]
* 0552-0552- [[Scriptor:Agnellus Ravennatis|Agnellus Ravennas]] Episcopus
* 0555-0555- [[Scriptor:Victor Tununensis|Victor Tununensis Episcopus
* 0555-0576- [[Scriptor:Germanus Parisiensis|Germanus Parisiensis]] Episcopus
* 0556-0556- [[Scriptor:Liberatus Carthaginensis]] Diaconus
* 0560-0616- [[Scriptor:Ethelbertus Anglorum Rex|Scriptor:Ethelbertus]] Anglorum Rex
* 0573-0603- [[Scriptor:Aunarius Autissiodorensis]] Episcopus
* 0575-0595- [[Scriptor:Chidelbertus II|Scriptor:Chidelbertus II Rex Francorum]]
* 0575-0596- [[Scriptor:Chidelbertus II]] Rex Francorum
* 0576-0576- [[Scriptor:Domnolus Cenomatensis]] Episcopus
* 0584-0584- [[Scriptor:Licinianus Carthaginensis]] Episcopus
* 0584-0629- [[Scriptor:Chlotarius II|Chlotarius II]] Francorum Rex
* 0584-0629- Scriptor:Chlotarius II Rex Francorum
* 0586-0586- [[Scriptor:Veranus episcopus|Scriptor:Veranus]]
* 0586-0601- [[Scriptor:Recaredus |Scriptor:Recaredus Rex Visigotorum]]
* 0589-0589- [[Scriptor:Sedatus Biterrensis]] Episcopus
* 0590-0604- [[Scriptor:Paterius Notarius Gregorii I]]
* 0595-0604- [[Scriptor:Augustinus Apostolus Anglorum]]
* 0595-0660- [[Scriptor:Fredegarius Scholasticus Burgundiae|Scriptor:Fredegarius Scholasticus]]
* 0600-0600- [[Scriptor:Dinothus Abbas]]
* 0600-0600- [[Scriptor:Eutropius Episcopus]]
* 0600-0600- [[Scriptor:Tarra monachus|Scriptor:Tarra Monachus]]
* 0601-0601- [[Scriptor:Dynamus Patricius|Dynamus Patricius]]
* 0601-0667- [[Scriptor:Hildefonsus Toletanus|Hildefonsus Toletanus]] Episcopus
* 0601-0700- Auctores Incerti
* 0603-0639- [[Scriptor:Dagobertus Francorum Rex]]
* 0604-0690- [[Scriptor:Theodorus Cantuariensis|Theodorus Cantuariensis]] Archiepiscopus
* 0610-0610- [[Scriptor:Bulgaranus comes|Bulgaranus Comes]]
* 0610-0610- [[Scriptor:Paulus Emeritanus|Paulus Emeritanus Diaconus]]
* 0610-0610- [[Scriptor:Tamaius De Vargas|Tamaius De Vargas]]. Thomas
* 0610-0612- [[Scriptor:Gondemarus|Gondemarus]] Rex Gothorum
* 0612-0612- [[Scriptor:Marcus Cassinensis|Marcus Cassinensis]]
* 0615-0615- [[Scriptor:Aileranus Scoto-Hibernus|Aileranus Scoto Hibernus Abbas]]
* 0615-0615- [[Scriptor:Alphanus Beneventanus|Alphanus Beneventianus]] Episcopus
* 0615-0615- [[Scriptor:Warnaharius Lingonensis|Warnaharius Lingonensis]] Episcopus
* 0616-0679- [[Scriptor:Leodegarius Augustodunensis|Leodegarius Augustodunensis]] Episcupus
* 0621-0621- [[Scriptor:Sisebutus Gothorum Rex]]
* 0623-0623- [[Scriptor:Bertichramnus Cenomanensis]] Episcopus
* 0624-0624- [[Scriptor:Protandius Vesuntinus|Protandius Vesuntinus]] Archiepiscopus
* 0625-0625- [[Scriptor:Sonniatus Rhemensis|Sonniatus Rhemensis]] Archiepiscopus
* 0625-0625- [[Scriptor:Verus Ruthenensis|Verus Ruthenensis]] Episcopus
* 0634-0656- [[Sigebertus|Sigebertus III Rex Francorum]]
* 0638-0638- [[Scriptor:Hadoinudus Cenomanensis|Hadoinudus Cenomanensis]] Episcopus
* 0639-0658- [[Scriptor:Clodoveus II|Clodoveus II]] Francorum Rex
* 0640-0640- [[Scriptor:Autbertus Cameracensis|Autbertus Cameracensis]] Episcopus
* 0640-0640- [[Scriptor:Sulpicius Bituricensis|Sulpicius Bituricensis]] Episcopus
* 0645-0645- [[Scriptor:Eutrandus Ticinensis|Eutrandus Ticinensis]] Diaconus
* 0645-0645- [[Scriptor:Maximus Caesaraugustanus|Maximus Caesaraugustanus]] Episcopus
* 0646-0646- [[Scriptor:Braulio Caesaraugustiani|Braulio Caesaraugustiani]] Episcopus
* 0646-0646- [[Scriptor:Gallus Abbas|Gallus Abbas]]
* 0646-0646- [[Scriptor:Taio Caesaraugustianus|Taio Caesaraugustianus]] Episcopus
* 0646-0646- [[Scriptor:Victor Carthaginensis|Victor Carthaginensis]] Episcopus
* 0648-0648- [[Scriptor:Maurus Ravennatensis|Maurus Ravennatensis]] Episcopus
* 0650-0650- [[Scriptor:Paulus Virodunensis|Paulus Virodunensis]] Episcopus
* 0651-0651- [[Scriptor:Desiderius Cadurcensis|Desiderius Cadurcensis]] Episcopus
* 0651-0651- [[Scriptor:Donatus Vesontionensis|Donatus Vesontionensis]] Episcopus
* 0651-0651- [[Scriptor:Landericus Parisiensis|Landericus Parisiensis]] Episcopus
* 0654-0654- [[Scriptor:Livinus Metensis|Livinus]] Episcopus
* 0656-0656- [[Scriptor:Annemundus Lugdunensis|Annemundus Lugdunensis]] Episcopus
* 0656-0656- [[Scriptor:Valerius S. Petri de Montibus|Valerius Abbas]]
* 0657-0657- [[Scriptor:Eugenius III Toletanus|Eugenius III Toletanus]] Episcopus
* 0659-0659- [[Scriptor:Eligius Noviomensis|Eligius Noviomensis]] Episcopus
* 0660-0660- [[Scriptor:Marculfus Monachus|Marculfus Monachus]]
* 0660-0660- [[Scriptor Sirmondus Jacobus|Sirmondus Jacobus]]
* 0660-0660- [[Scriptor:Valerius De Montibus]]
* 0661-0661- [[Scriptor:Cummianus Hibernus|Cummianus Hibernus]]
* 0661-0662- [[Scriptor:Clotarius III|Clotarius III]] Francorum Rex
* 0662-0675- [[ Childericus II|Childericus II]] Francorum Rex
* 0665-0665- [[Scriptor:Fructuosus Bracarensis|Fructuosus Brancarensis]] Episcopus
* 0670-0670- [[Scriptor:Faro Meldinensis|Faro Meldinensis]] Episcopus
* 0670-0670- [[Scriptor:Ionas Elnonensis|Jonas Elnonensis]] Abbas
* 0672-0754- [[Scriptor:Bonifacius Moguntinus|Bonifacius Moguntinus]] Episcopus
* 0676-0679- [[Scriptor:Dagobertus II Francorum|Dagobertus II]] Francorum Rex
* 0679-0679- [[Scriptor:Amandus Trajectensis|Amandus Trajectensis]] Episcopus
* 0679-0679- [[Scriptor:Damianus Ticinensis|Damianus Ticinensis]] Episcopus
* 0679-0691- [[Scriptor:Theodoricus III Francorum|Theodoricus III]] Francorum Rex
* 0680-0690- [[Scriptor:Iulianus Toletanus|Julianus Toletanus]] Episcopus
* 0700-0800- [[Scriptor:Adamanus Benedectinus|Adamanus Benedectinus]]
* 0700-0800- [[Scriptor:Catulfus|Catulfus]]
* 0700-0800- [[Scriptor:Constans Sacerdos|Constans Sacerdos]]
* 0700-0800- [[Scriptor:Crisconius Africanus|Crisconius Africanus]] Episcopus
* 0700-0800- [[Scriptor:Defensor Locociagensis|Defensor Locociagensis]] Monachus
* 0700-0800- [[Scriptor:Evatius Troclariensis|Evatius Troclariensis]] Abbas
* 0700-0800- [[Scriptor:Fulgentius Ferrandus|Fulgentius Ferrandus]]
* 0700-0800- [[Scriptor:Isidorus Pacensis|Isidorus Pacensis]]
* 0700-0800- [[Scriptor:Landulfus Sagax|Landulfus Sagax]]
* 0700-0800- [[Scriptor:Petrus archidiaconus|Petrus Archidiaconus]]
* 0701-0800- Auctores Incerti
* 0709-0709- [[Scriptor:Aldhelmus Schireburgenensis|Aldhelmus Schireburgenensis]] Episcopus
* 0709-0709- [[Scriptor:Ceolfridus Wiremutensis|Ceolfridus Wiremutensis]] Presbyter
* 0715-0766- [[Scriptor:Chrodeganus Metensis|Chrodeganus Metensis]] Episcopus
* 0717-0717- [[Scriptor:Felix Ravennatensis|Felix Ravennatensis]] Episcopus
* 0720-0799- [[Scriptor:Paulus Diaconus|Paulus Winfridus Diaconus]]
* 0725-0725- [[Scriptor:Benedictus Crispus|Benedictus Crispus]] Mediolanensis Archiepiscopus
* 0726-0804- [[Scriptor:Paulinus Aquileiensis|Paulinus Aquileiensis]] Patriacha
* 0729-0729- [[Scriptor:Egbertus Eboracensis|Egbertus Eboracensis]] Archiepiscopus
* 0730-0784- [[Scriptor:Ambrosius Autpertus|Ambrosius Autpertus]] Beneventianus Abbas
* 0735-0804- Alcuinus, [[Scriptor:Flaccus Albinus|Flaccus Albinus]]
* 0739-0739- [[Scriptor:Wilibrordus Ultrajectinus|Wilibrordus Ultrajectinus]] Episcopus
* 0742-0778- Reges Francorum
* 0745-0814- [[Scriptor:Angilbertus Centulensis|Angilbertus Centulensis]]
* 0745-0814- Angilbertus Centulensis Abbas
* 0747-0814- Karolus Magnus
* 0747-0821- [[Scriptor:Benedictus Anianensis|Benedictus Anianensis]] Abbas
* 0750-0821- [[Scriptor:Theodulfus Aurelianensis|Theodulfus Aurelianensis]]
* 0750-0850- [[Scriptor:Aimonius Sangermanensis|Aimonius Sangermanensis]]
* 0750-0850- [[Scriptor:Ascarius|Ascarius]] Tusaredo
* 0750-0850- [[Scriptor:Candidus Fuldensis|Candidus Fuldensis]]
* 0750-0850- [[Scriptor:Hildemarus|Hildemarus]]
* 0750-0850- [[Scriptor:Ioannes De Deo|Joannes De Deo]]
* 0750-0850- [[Scriptor:Lambertus Pultariensis|Lambertus Pultariensis]]
* 0750-0850- [[Scriptor:Paulinus Aquileiensis|Paulinus Aquileiensis]]
* 0750-0850- [[Scriptor:Speraindeo Abba|Speraindeo Abba]]s
* 0751-0818- [[Scriptor:Magnus Senonensis|Magnus Senonensis]] Archiepiscopus
* 0753-0876- [[Scriptor:Lullus Moguntium|Lullus Moguntium]] Episcopus
* 0754-0783- [[Scriptor:Elipandus Toletanus|Elipandus Toletanus]] Episcopus
* 0758-0758- [[Scriptor:Priminus Abbas|Priminus Abbas]]
* 0760-0760- [[Scriptor:Cyprianus Cassinensis|Cyprianus Cassinensis]] Monachus
* 0760-0830- [[Scriptor:Remigius Curiensis|Remigius Curiensis]] Episcopus
* 0760-0860- [[Scriptor:Bernowinus Claromontensis|Bernowinus Claromontensis]]
* 0760-0860- Dungalus Reclusus
* 0761-0822- Eigil Fuldensis
* 0763-0836- Hetto (Ahyto) Basileensis
* 0767-0767- Auctor Incertus
* 0770-0770- Angelramnus Metensisi
* 0770-0827- Jeremias Senonensis Archiepiscopus
* 0770-0834- Ansegius Fontanellensis Abbas
* 0770-0840- Eginhardus (Einhardus)
* 0770-0840- Smaradgus Abbas
* 0770-0870- Adalhardus Corbeiensis Abbas
* 0775-0836- Aldricus Senonensis Archiepiscopus
* 0775-0842- Hilduinus Sandionysianus Abbas
* 0776-0766- Sturmius Fuldensis Abbas
* 0776-0852- Symphosius Amalarius
* 0778-0840- Ludovicus Pius Francorum Imperator
* 0779-0841- Agobardus Lugdunensis
* 0780-0849- Walafridus Strabo Fuldensis
* 0780-0850- Jonas Aurelianus Episcopus
* 0780-0853- Freculphus Lexoviensis Episcopus
* 0780-0870- Aldricus Cenomanensis Episcopus
* 0780-0880- Audradus Senonensis Chorepiscopus
* 0781-0826- Ermoldus Nigellus
* 0785-0785- Heterius Uxamensis
* 0788-0788- Rachio Argentinensis Episcopus
* 0790-0790- Wicbodus
* 0790-0840- Dodana Sive Duodena (Dhuoda)
* 0790-0860- Florus Lugdunensis Diaconus
* 0790-0865- Paschasius Radbertus Corbeiensis Abbas
* 0791-0791- Angelramus Metensis Episcopus
* 0794-0794- Felix Urgellensis Episcopus
* 0795-0855- Lotharius I Germaniae
* 0799-0859- Eulogius Toletanus Episcopus
* 0800-0845- Nithardus S Richarii Abbas
* 0800-0868- Ratramnus Corbeiensis
* 0800-0900- Cyprianus Cordubensis
* 0800-0900- Dulcidius Salmaticenses
* 0800-0900- Grimlaicus Presbyter (Grimlaiec)
* 0800-0900- Isidorus Mercator
* 0800-0900- Leuvigildus Cordubensis
* 0800-0900- Pseudo Luitprandus
* 0801-0900- Auctores Incerti
* 0802-0923- Francorum Regum Imperatorum
* 0805-0846- Agnellus (Andreas) Ravennatensis
* 0806-0882- Hincmarus Rhemensis Episcopus
* 0807-0861- Paulus Alvarus Cordubensis
* 0807-0866- Gotteschalcus Orbacensis
* 0809-0809- Dagulfus Sandionysianus
* 0809-0809- Farnulfus Sandionysianus
* 0809-0809- Ludgerus Mimigardenfordensis Episcopus
* 0809-0809- Simpertus Abbas Murbacensis
* 0809-0814- Amalarius Fortunatus Trevirensis
* 0810-0861- Servatus Lupus Ferrariensis Abbas
* 0810-0865- Rodulphus Bituricensis Episcopus
* 0810-0875- Usuardus Sangermanensis Monachus
* 0811-0842- Maxentius Aquileiensis Patriarcha
* 0813-0870- Wandalbertus Prumiensis Monachus
* 0814-0878- Adrevaldus Floriacensis Monachus
* 0815-0815- Amalarius Fortunatus Trevirensis Archiepiscopus
* 0815-0877- Joannes Scotus Erigena
* 0816-0816- Leidradus Lugdonensis Episcopus
* 0816-0826- Reges Francorum
* 0816-0845- Ebbo (Ebo) Rheminensis Episcopus
* 0817-0827- Claudius Taurinensis Episcopus
* 0817-0831- Halitgarius Cameracensis Episcopus
* 0817-0871- Iso Sangallensis
* 0818-0871- Aenea Parisiensis Episcopus
* 0820-0820- Sedulius Scotus
* 0822-0853- Rothadus II Suessionensis Episcopus
* 0823-0877- Carolus Calvus Francorum Rex
* 0827-0875- Angilbertus Mediolanensis Archiepiscopus
* 0830-0830- Benedictus Diaconus
* 0830-0830- Monachus Sancti Galli
* 0830-0888- Rembertus Hamburgensis Episcopus
* 0834-0834- Fredegisus Abbas
* 0834-0834- Haiminius Sancti Vedasti Atrebatensis
* 0834-0834- Jesse Ambianensis Episcopus
* 0834-0876- Hildericus. Cassinensis Abbas
* 0840-0853- Haymo Halberstatensis Episcopus
* 0840-0871- Milo Monachus Sancti Amandi
* 0840-0900- Ratpertus Sangallensis Monachus
* 0840-0912- Notkerus Balbulus
* 0840-0930- Hucbaldus Sancti Amandi
* 0841-0852- Amulo Lugdunensis Episcopus
* 0841-0876- Hericus Antissiodorensis Monachus
* 0843-0843- Theganus Trevirensis Chorepiscopus
* 0844-0844- Frotharius Tullensis Episcopus
* 0844-0861- Prudentius Trecensis Episcopus
* 0845-0845- Eldefonsus Hispalensis Episcopus
* 0846-0846- Josephus Sacerdos
* 0848-0859- Sedulius Scotus
* 0848-0875- Vulfadus Bituricensis Episcopus
* 0850-0850- Christianus Druthmarus
* 0850-0850- Columbanus Trudonis Abbas
* 0850-0850- Ermanricus Augiensis
* 0850-0869- Guntharius Coloniensis Episcopus
* 0850-0874- Ado Viennensis Archiepiscopus
* 0851-0851- Aurelianus Recomensis
* 0852-0875- Remigius Lugdonensis Episcopus
* 0853-0853- Erchambertus Frisingensis Episcopus
* 0855-0874- Adventius Metinensis Episcopus
* 0855-0878- Anastasius Bibliothecarius Abbas
* 0856-0856- Angelomus Luxovensis
* 0856-0871- Herardus Turonensis Archiepiscopus
* 0856-0872- Grimaldus Sangallensis Abbas
* 0860-0860- Walterius Aurelianensis Episcopus
* 0860-0943- Cappidus Stavriensis
* 0861-0880- Odo Bellovacensis Episcopus
* 0862-0864- Engelmodus Suessionensis Episcopus
* 0865-0865- Anscharius Hamburgensis Episcopus
* 0868-0868- Lotharius
* 0868-0868- Theudoinus Catalaunensis
* 0871-0871- Bernardus Monachus Francus
* 0872-0900- Alfredus Magnus Anglorum Rex
* 0876-0876- Andreas Bergomas Presbyter
* 0876-0936- Henricus I Imperator
* 0878-0878- Hincmarus Laudunensis Episcopus
* 0880-0880- Isaacus Lingonensis Episcopus
* 0880-0890- Angilbertus Corbeiensis Abbas
* 0881-0923- Dado Virdunensis Episcopus
* 0882-0900- Fulco Rheimensis Archiepiscopus
* 0882-0908- Remigius Antissiodorensis
* 0882-0915- Regino Prumiensis Abbas
* 0883-0883- Bertarius Cassinensis Abbas
* 0883-0916- Robertus Metensis Episcopus
* 0884-0884- Harmotus Sangallensis Abbas
* 0884-0902- Riculfus Suessonensis Episcopus
* 0885-0960- Atto Vercellensis Episcopus
* 0887-0887- Aimonius Sangermanensis Monachus
* 0888-0888- Franciscus Blanchinus Veronensis
* 0888-0906- Waldrammus Argentinensis Episcopus
* 0890-0890- Erchembertus Cassinensis Monachus
* 0890-0916- Salomon Constantiensis Episcopus
* 0890-0974- Ratherius Veronensis Episcopus
* 0892-0892- Petrus Bibliothecarius
* 0893-0893- Wolfhardus Hasenrietanus Presbyter
* 0893-0911- Ludovicus IIII Franciae Rex
* 0894-0966- Flodoardus Remensis Canonicus
* 0895-0968- Mathildis (Mechthild) Regina Francorum
* 0899-0899- Anamodus Ratisbonensis Subdiaconus
* 0899-0916- Radbodus Trajectensis Ad Rhenum (Utrech) Episcopus
* 0900-0900- Eutropius Longobardus
* 0900-0922- Hervaeus Rhemensis Episcopus
* 0900-1000- Adso Dervensis
* 0900-1000- Albuinus Eremita
* 0900-1000- Amblalardus Sollemniacensis Abbas
* 0900-1000- Gerardus Suessonensis
* 0900-1000- Richerus Remenses
* 0900-1000- Teraldus
* 0900-1027- Romualdus Camaldulensis Abbas
* 0901-0920- Stephanus Leodiensis Episcopus
* 0901-0961- Odo Cantuariensis Archiepiscopus
* 0901-1000- Auctores Incerti
* 0902-0902- Mantio Catalaunensis Episcopus
* 0905-0905- Christophorus (Antipapa)
* 0905-0906- Edwardus Senior Anglorum Rex
* 0906-0906- Martianus Monachus
* 0909-0988- Dunstanus Cantauriensis Archiepiscopus
* 0910-0910- Willelmus Arvernorum
* 0912-0973- Otto I Imperator
* 0912-0973- Otto Magnus Imperator I
* 0915-0915- Bertarius Virdunensis
* 0915-0927- Agio Narbonensis Episcopus
* 0920-0926- Odilo Sancti Medardi Suessonensis
* 0922-0925- Seulfus Rhemensis Archiepiscopus
* 0922-0972- Liutprandus Cremonensis Episcopus
* 0923-0923- Abbo Sangermanensis
* 0923-0923- Radbdus Dolentis
* 0923-0923- Walterius Senoensis Episcopus
* 0924-0939- Aethelstanus Anglorum Rex
* 0924-0973- Udalricus Augustianus Episcopus
* 0926-0926- Berno Abbas
* 0928-0928- Cyprianus Cordubensis
* 0928-0975- Folquinus Sanbertinianus Monachus
* 0930-1002- Hrorshitha Gandersheimensis
* 0932-0954- Joannes Italus Cluniacensis
* 0936-0950- Leotaldus Matisconensis
* 0939-0946- Edmundus Anglorum Rex
* 0940-0948- Hoelus Dha (Howell The Good)
* 0942-1007- Herigerus Lobiensis Abbas
* 0945-1004- Abbo Floriacensis Abbas
* 0946-0961- Arthaldus Rhemensis Archiepiscopus
* 0947-1030- Adalbero Laudunensis Episcopus
* 0950-0950- Cosmas Japygus Materiensis
* 0950-0950- Laurentius Cassinensis
* 0950-0984- Gezo Dertonensis Abbas
* 0950-1008- Aimoinus Floriacensis
* 0953-0965- Bruno Coloniensis Episcopus I
* 0955-0983- Otto Imperator II
* 0956-0996- Adalbertus Pragensis Episcopus
* 0959-0971- Eralius (Eraclus) Leodiensis Episcopus
* 0959-0975- Edgarus Anglorum Rex (Eadgar)
* 0960-1012- Bridfertus Ramensis Monachus
* 0960-1029- Dudo Viromandensis Decanus
* 0960-1038- Godehardus Hildesheimensis Episcopus
* 0961-0983- Ethelwoldus Wintoniensis Episcopus
* 0962-0969- Odalricus Rhemenseis Archiepiscopus
* 0963-0963- Fridegodus Benedectinus
* 0963-0963- Sigehardus Trevirensis
* 0964-0964- Adalgerus Episcopus
* 0964-0979- Richardus Floriacensis Abbas
* 0964-0982- Bernerus Humolariensis Abbas
* 0964-0984- Theodericus Metensis Episcopus
* 0964-0994- Maiolus Cluniacensis Abbas IV
* 0965-0965- Utho Argentinensis Episcopus
* 0965-0966- Wiboldus Cameracensis Episcopus
* 0965-0990- Folcuinus Laubiensis Abbas
* 0965-0991- Erkembaldus Argentinensis Episcopus
* 0965-0994- Aymardus Cluniacensis Abbas
* 0966-0966- Guillelmus Cabillonensis
* 0967-0985- Gumpoldus Mantuanus Episcopus
* 0968-0970- Hatto Moguntinus II Archiepiscopus
* 0968-1027- Mathildis Regina
* 0969-0988- Adalbero Remensis Archiepiscopus
* 0970-0983- Windukindus (Witikundus) Corbeiensis
* 0972-1024- Henricus Imperator II
* 0974-1008- Notgerius Leodiensis Episcopus
* 0975-1039- Cunegonda Imperatrix Henrici II Uxor
* 0976-0996- Guido Podiensis Episcopus II
* 0976-1018- Thietmarus Merseburgensis Episcopus
* 0977-0983- Joannes Metensis Abbas
* 0979-0979- Adalbertus Metensis
* 0979-1016- Aethelredus Anglorum Rex II
* 0980-0980- Helpericus Monachus S Galli
* 0980-0980- Wigo Phyuhtwangesis Decanus
* 0980-1002- Otto Imperator III
* 0983-0983- Odo Ausciensis
* 0985-1047- Rodulfus Glaber Cluniacensis
* 0985-1048- Odorannus Monachus
* 0986-0986- Poeta Saxo
* 0988-1034- Ademarus Engolismensis
* 0990-0990- Joannes Smera Polovecius
* 0994-1032- Radulphus Burgundiorum Rex
* 0994-1049- Odilo Cluniacensis Abbas
* 0995-1030- Guillelmus Aquitaniae Dux V
* 0995-1048- Wippo Presbyter
* 0995-1073- Gualbertus Vallumbrosanus
* 0996-0996- Letaldus Micianensis
* 0996-1031- Robertus II Francorum Rex
* 0997-0997- Gunzo Grammaticus (Novariensis)
* 0999-0999- Conradus Celtus
*
* 1000-1000- Wido Monachus
8rh81ggt3qt182wj7k8lgnrxu9jshi0
Scriptor:Paschasius Radbertus
102
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{{Scriptor
|Munera=
|Natio=
|PostNationem=
|IndicisNomen=
}}
==Opera==
* [[De partu Virginis (Ratbertus Corbeiensis)|De partu Virginis]]
* [[Fragmentum de partu Virginis]]
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<noinclude><pagequality level="3" user="Aschroet" /></noinclude>''worden'' / Lectus sum vel sui. Interdum
particula ''worden'' omittitur, Vt:
''Ich bin gelesen'' / Lectus sum, vel, ''Ich bin gelesen worden'' /
Lectus sui.
Neutrum est, cui praeponitur in praesenti
Indicatiuo, ''Ich'' / ''du'' / ''der'' / ''Wir'' / ''jr'' /
''sie'' / vt in Actiuo: Et in praeterito Persecto,
''Ich bin'' / ''du bist'' / ''der ist'' / ''Wir sind'' / ''ir seid'' /
''sie sind'' / vt in Passiuo, sed particula
''worden'' non additur, vt: ''Ich sterbe'' / Morior.
''Ich bin gestorben'' / Mortuus sum.
Quaedam etiam coniugantur vt Actiua,
sed Passiuum ex se non formant, vt:
''Ich lebe'' / Viuo. ''Ich habe gelebet'' / Vixi.
Sed non, ''Ich werde gelebet.'' Quaedam
etiam vtroque modo formant praeteritum,
vt: ''Ich stehe'' / Sto. ''Ich bin gestanden'' / &,
''Ich habe gestanden'' / Steti. ''Ich gehe'' /
Eo. ''Ich bin gegangen'' / &, ''Ich habe gegangen'' /
lui. ''Ich sitze'' / Sedeo. ''Ich bin gesessen'' / &
''Ich habe gesessen'' / Sedi.
Sub Neutro comprehenditur Subastantiuum
''Ich bin'' / Sum, & Neutroapassiuum,
''Ich werde'' / Fio, & ex hoc
composita , quae Latinis inchoatiua
sunt, vt: ''Ich werde innen'' / ''Ich werde gewar'' /<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="Aschroet" /></noinclude>Praesentisco. ''Ich werde warm'' / monde
Calesco, &c.
{{center|TEMPVS.}}
Tempora in Verbis sunt quinque:
Praesens, Imperfectum, Perfectum,
Plusquamperfectum, & Futurum.
Praesens est ipsum verbi thema, cui,
praeponītur nominatiui personae, ''Ich'' /
''du'' / ''er'' / ''sie'' / ''das'' / ''es'' / ''Wir'' / ''jr'' / ''sie'' / vt: ''Ich liebe'' /
Amo. ''Du liebest'' / Amas. ''Er liebet'' /
Amat. ''Wir lieben'' / Amamus. ''Ihr liebet'' /
Amatis. ''Sie lieben'' / Amant. Sed in secunda
& tertia persona singulari mutantur
quaedam vocales & diphthongi
in disyllabis, ve: ''Ich ziehe'' / Traho, Prosicifcor,
''Du zeuchst'' / ''Er zeucht''. ''Wir ziehen'' /
''Ihr ziehet'' / ''Sie ziehen''. ''Ich gebe'' /
Do, ''Du gibst'' / ''Er gibt''. ''Wir geben'' / ''Ihr gebet'' /
''Sie geben''. ''Ich liege'' / Mentior,
''Du leugest'' / ''Er leuget''. ''Wir liegen'', ''Ihr lieget'' /
''Sie liegen.'' Cum vero verbum
est monosyllabum in prima persona singulari
Indicatiui praesentis , tres personae
singulares habent easdem vocales
& diphthongos, quae in plurali mutantur<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="Aschroet" /></noinclude>in alias, & tertia primae similis
est, vt: ''Ich kan'' / Possum. ''Du kanst'' / Potes.
''Er kan'' / Potest. ''Wir koennen'' / Possumus.
''Ihr koennet'' / Potestis. ''Sie koennen'' /
Possunt. ''Ich mag'' / Licet mihi. ''Du magst'' /
Licet cibi. ''Er mag'' / Licet illi.
''Wir moegen'' vel ''muegen ''(Saepe enim inter
se permutantur ''o'' & ''u'' / ''oe'' & ''ue'' ) Licet
nobis. ''Ihr moeget'' vel'' mueget'' / Licet vobis.
''Sie moegen'' vel ''muegen'' / Licet illis.
''Ich will'' / Volo. ''Wir woellen'' / Volumus.
''Ich soll'' / Debeo. ''Wir sollen'' / Debemus.
''Ich weiss'' / Scio. ''Wir wissen'' / Scimus.
''Ich taug'' / Aptus sum, Frugi sum. ''Wir tuegen'' /
Apti sumus. ''Ich thar'' / Ausim.
''Wir thueren'' / Audemus. ''Ich darff'' / Fas
mihi. ''Wir duerffen'' / Fas nobis. ''Ich muss'' /
Oportet me. ''Wir muessen'' / Oportet nos.
Sed de hac mutatione dicetur infra
post coniugationes.
Imperfectum murat vocales & diphthongos
sui thematis in alias , vt: ''Ich zihe'' /
''Ich zoch'' & ''zog''. Ich schiesse'' / laculor,
''Ich schoss''. ''Ich keuffe'' / Emo, ''Ich kauffte''.
Definit vero in aliquibus in
consonantem verbi , vt: ''Ich schreibe'' /<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="Aschroet" /></noinclude>Scribo. ''Ich schreib'' / Scribebam. ''Ich lese'' /
Lego. ''Ich las'' / Legebam. In aliquibus
verò in ''te'' syllabam ad thema verbi
assumtam, vt: ''Ich liebe'' / Amo. ''Ich liebete'' /
Amabam. ''Ich lere'' / Doceo. ''Ich lerete'' /
Docebam. Et in talibus aliquando
''e'' penultimum per syncopen , aliquando
vltimum per apocopen, ali ils
quando vtrumque abijcitur breuitatis
caussa, vt: ''Ich liebete'' / vel ''liebte'' / vel
''liebt'' / Amabam. Prima & tertia singulares
sunt similes, & prima ac tertia plurales
itidem similes , vt: ''Ich liebete'' /
Amabam. ''Er liebete'' / Amabat. ''Wir liebeten'' /
Amabamus. ''Sie liebeten'' / Amabant.
''Ich gab'' / Dabam. ''Er gab'' / Dabat.
''Wir gaben'' / Dabamus. ''Sie gaben'' /
Dabant. Secunda singularis in quibusdam
mutat vocales primae personae in
alias , quam sequuntur tres persona
plurales, vt: ''Ich sang'' / Canebam. ''Du sungest'' /
Canebas. ''Wir sungen'' / Canebamus.
''Ihr sunget'' / Canebatis, &c. Cum
thema verbi est monosyllabum , omnes
Imperfecti personae habent eadem vocales,
vt: ''Ich mag'' / Licet mihi. ''Ich''<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="Aschroet" /></noinclude>''mochte'' / Licebat mihi. ''Du mochtest'' / Licebat
tibi. ''Er mochte'' / Licebat illi. ''Wir mochten'' /
Licebat nobis. ''Ihr mochtet''/
Licebat vobis. ''Sie mochten'' / Licebar illis.
''Ich will'' / ''Ich wolte''. ''Ich soll'' / ''Ich solte.''
''Ich weis'' / ''Ich wuste''. ''Ich taug'' / ''Ich tochte''.
''Ich thar'' / ''Ich thurste''. ''Ich darff'' /
''Ich durffte''. ''Ich muss'' / ''Ich muste''. ''Ich kan'' /
''Ich kundte.'' Sed de hac quoque mutatione
vocalium & diphthongorum
in Imperfecto, dicetur infra post Coniugaciones.
Perfectum praeponit themati in Actiuis,
''Ich habe.'' In Passiuis, ''Ich bin worden.''
In Neutris, ''Ich bin'' / & in aliquibus,
''Ich habe'' / in aliquibus vtrumque, &
in initio assumit augmentum ''ge'' / cum
mutatione vocalium & diphthongorum
in penultima, vt: ''Ich habe gelesen'' /
Legi. ''Ich bin gelesen worden'' / Lectus
sum vel sui. ''Ich bin gestorben'' / Mortuus
sum. ''Ich habe gelebet'' / Vixi. ''Ich bin oder habe gestanden'' /
''gegangen'' / Steti,
lui. Quae in imperfecto in consonantem
verbi definunt, eorum praeteritum
Perfectum exit in ''en'' / vt: ''Ich schreib'' /<noinclude><references/></noinclude>
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<noinclude><pagequality level="3" user="Aschroet" /></noinclude>Scribebam. ''Ich habe geschrieben'' / Scripsi.
''Ich las'' / Legebam. ''Ich habe gelesen'' /
Legi. Quae vero in Imperfecto assumunt
''te'' / eorum praeteritum Perfectum
definit in ''et'' / vt: ''Ich liebete'' / Amabam.
''Ich habe geliebet'' / Amaui. ''Ich lerete'' /
Docebam. ''Ich habe geleret'' / Docui.
Et in talibus ''e'' in vltima ante ''t'' non
rarò abijcitur, vt: ''Geliebt'' / ''Gelert''.
Composita augmentum recipiunt
in medio, id est, inter veram partem
compositionis, vt : ''Ich habe ausgelesen'' /
Elegi.'' Ausgeschrieben'' / Descripsi.
''Umbgestoffen'' / Euerti. ''Zugemacht'' / Clau
si. Quaedam etiam à principio recipiunt
augmentum, vt: ''Ich habe geweissaget'' /
Prophetaui, Matth. 7. Quaedam etiam
augmento carent, vt composita cum
''be'' / ''ver'' / ''zer'' / & quae composita accentum
habent in posteriore parte compositionis, vt: ''Bekuemmern'' /
Molestia afficere, ''Bekuemmert''. ''Befehlen'' / Mandare,
''Befohlen''. ''Verachten'' / Contemnere,
''Verachtet''. ''Zerstoeren'' / Destruere, ''Zerstoeret''.
''Ich habe uberlesen'' / Perlego. ''Ich habe uberlesen'' /
Perlegi. ''Ich ubergebe'' / Trado.<noinclude><references/></noinclude>
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<noinclude><pagequality level="1" user="Aschroet" /></noinclude>''Zwelff jar alt /'' Annos natus duodecim
&c. Vsurpatur & genitiuus, vt: ''Einer''
''hand breit /'' Latitudine palmi. ''Eines fusses''
''breit /'' Latitudine pedis. ''Eins jars alt /''
Anniculus.
XI.
Ablatiuus instrumentum, causam,
materiam , aut partem significans, subijcitur
adiectiuis & participijs cum
præpofitione: Inſtrumentum quidem ad
cum praepositione ''mit /'' vt: ''mit ruten gesteupt /''
Virgis caesus. ''Mit der fauft geschlagen /''
Pugno percuſfus. ''Mit dem''
''Schwerdte getoedtet'' : Cauffa uerò cum
praepositione von uel ''an /'' vt: ''Er ist muede''
''von arbeit /'' Feſſus labore. ''Truncken''
''vom wein /'' Ebrius uino. ''Kranck am fiber /''
''Gestorben an der Schwindsucht /''
Laborans febri, mortuus phthiſi: Materia
autem cum praepositione ''aus'' uel
''von /'' vt: ''Von gold gemacht /'' Ex auro
factus. ''Aus Holze geschnitzt /'' Exculptus
è ligno: Pars denique cum praepositione
''an /'' vt: ''Er ist lahm an henden vnd fuessen /''
Pedibus manibus que claudus. ''Zart /''<noinclude><references/></noinclude>
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<noinclude><pagequality level="1" user="Aschroet" /></noinclude>''rein am leibe /'' Corpore tenero, Mundus
corpore.
XII.
Adiectiua voluntatem aut facultatem
significantia requirunt praepositionem
''zu'' cum suo casu uel infinitiuo,
vt: ''Er ist geschickt zu dem dinge /'' Aptus
seu idoneus ad hoc. ''Bereit vnd willig''
''zu thun /'' Paratus & promtus ad faciendum.
XIII.
Formulae laudandi & vituperandi
efferuntur trifariam : 1. Vel per geminum
genitiuum adiectiui & substantiui,
vt: ''Ein Weib schoener gestalt /'' Foemina
vultus speciosi. ''Ein Man grosses''
''verstandes /'' Vir magni iudicij. ''Boeser''
''art /'' Prauae naturae: 2. Vel per geminum
ablatiuum adiectiui & substantiui ,
cum praepositione von / vt: ''Ein''
''Weib von schoener gestalt /'' Forma speciosa.
''Von guter art / ''Bona natura.
''Von grosser kunst /'' Praestans arte: 3. Vel
per praepositionem ''an'' uel ''von'' cum suo<noinclude><references/></noinclude>
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A First Latin Reader/1
0
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{{titulus
|Scriptor=H.C. NUTTING. Ph.D.
|OperaeTitulus=A First Latin Reader
|OperaeWikiPagina=A First Latin Reader
|Annus= 1912
|SubTitulus=Lesson 1<br/ >
''Christopher Columbus''
|Liber=A_First_Latin_Reader.pdf
}}
<div class=text>
{{Liber
|Ante= Preface
|AnteNomen=A_First_Latin_Reader/Preface
|Post=2. Christopher Columbus (Continued)
|PostNomen=A_First_Latin_Reader/2
}}
<pages index="A_First_Latin_Reader.pdf" from=11 to=12 fromsection=1 tosection=1 />
{{c|{{bar|8}}}}
<references/>
</div>
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Scriptor:Aldhelmus Schireburgenensis
102
56841
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Demetrius Talpa
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#REDIRECT [[Scriptor:Aldhelmus Schireburnensis]]
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Scriptor:Theodulfus Aurelianensis
102
56842
184089
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Demetrius Talpa
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Redirigens ad [[Scriptor:Theodulfus]]
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#REDIRECT [[Scriptor:Theodulfus]]
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