File:F Ring and Atlas PIA10448.jpg

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A train of diagonal channels in Saturn's F ring follows behind the moon Prometheus. Each of these features was created during a previous close approach of Prometheus to the ring.

When the moon is at the farthest point in its orbit of the planet, it strays close to (and often into) the F ring. The resulting gravitational disturbance leaves behind the channels seen here.

Atlas (30 kilometers, or 19 miles across at its widest point) appears at lower right.

This view looks toward the unilluminated side of the rings from about 27 degrees above the ringplane. The image was taken in visible light with the Cassini spacecraft narrow-angle camera on July 5, 2008. The view was acquired at a distance of approximately 1.1 million kilometers (675,000 miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 34 degrees. Image scale is 6 kilometers (4 miles) per pixel.
Date
Source http://photojournal.jpl.nasa.gov/catalog/PIA10448
Author NASA
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(Reusing this file)
Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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Transferred from en.wikipedia to Commons using For the Common Good.

The original description page was here. All following user names refer to en.wikipedia.
Date/Time Dimensions User Comment
09:43, 19 August 2008 930 × 1,017 (20,543 bytes) w:en:Kwamikagami (talk | contribs) {{Information |Description=A train of diagonal channels in Saturn's F ring follows behind the moon Prometheus. Each of these features was created during a previous close approach of Prometheus to the ring.<br><br>When the moon is at the farthest point in

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5 July 2008

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current10:30, 14 February 2015Thumbnail for version as of 10:30, 14 February 2015930 × 1,017 (20 KB)Jcpag2012Transferred from en.wikipedia: see original upload log above
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