Beeld:Saturnus F-RingPIA02272.jpg

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Original Caption Released with Image: The three separate components of Saturn's F-ring are seen in this image taken by NASA's Voyager l on Nov. 12, 1980, from a range of 750,000 kilometers (466,000) miles. Two prominent bright strands appear twisted and kinked, while the fainter, innermost third strand largely lacks such non-uniformities. The kinking appearance of the ring may be caused by the gravitational perturbations of two nearby satellites -- S-13 on the outside and S-14 on the inside -- or the effect may be caused by electromagnetic forces upon small F-ring particles. The Voyager project is managed for NASA by the Jet Propulsion Laboratory, Pasadena, Calif.

Public domain: This file is in the public domain because it was created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (NASA copyright policy page or JPL Image Use Policy).

Source:http://photojournal.jpl.nasa.gov/catalog/PIA02272

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  • (skrap) (huidige) 16:11, 10 Maart 2007 . . Anrie (Besprekings | bydraes) . . 469×443 (6 656 grepe) ('''Original Caption Released with Image:''' The three separate components of Saturn's F-ring are seen in this image taken by NASA's Voyager l on Nov. 12, 1980, from a range of 750,000 kilometers (466,000) miles. Two prominent bright strands appear twisted)

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