File:PIA07712 - F ring animation.gif

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PIA07712_-_F_ring_animation.gif (450 × 450 pixels, file size: 3.43 MB, MIME type: image/gif, looped, 65 frames, 26 s)

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This movie sequence from Cassini shows dark drapes in the inner strands of the F ring caused by the gravitational influence of the shepherd moon Prometheus (102 kilometers, 63 miles across).

Prometheus appears first in the sequence, interior to the F ring, and Pandora (84 kilometers, 52 miles across) follows along outside of the ring. Radial structure in the bright core of the ring is visible throughout the movie.

Prometheus orbits closer to Saturn, and thus faster, than the icy particles that make up the F ring. The moon passes comes closest to the ring at “apoapse”, when it is farthest from Saturn. It is during these apoapse passages that Prometheus has its greatest influence on the fine ring material. With time, the ring material previously affected falls behind so that on the next apoapse passage of Prometheus, a new gore in the inner ring material is made. The material closer to Prometheus orbits the planet faster than the material closer to the bright F ring core. The gores, together with the sheared-out material due to differential orbital motion, create the dark, diagonal drapes.

Several background stars are seen moving across the field during the movie.

The visible light images in this sequence were acquired using the narrow angle camera on April 13, 2005 from a distance of approximately 1.2 million kilometers (700,000 miles) from Saturn.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.

For more information about the Cassini-Huygens mission, visit http://saturn.jpl.nasa.gov and the Cassini imaging team home page, http://ciclops.org.

This is a truncation of NASA's half-size animated gif version of the sequence.

The full size image sequence is also available at http://photojournal.jpl.nasa.gov/animation/PIA07712.
Date
Source http://ciclops.org/view.php?id=1361
Author NASA/JPL/Space Science Institute
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This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA07712.

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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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Date/TimeThumbnailDimensionsUserComment
current19:51, 24 November 2007Thumbnail for version as of 19:51, 24 November 2007450 × 450 (3.43 MB)WolfmanSF (talk | contribs)Reduce file size by deleting alternate frames. Double delay setting to maintain speed of animation.
09:48, 23 November 2007Thumbnail for version as of 09:48, 23 November 2007450 × 450 (6.44 MB)WolfmanSF (talk | contribs)truncate down to 122 frames
02:00, 23 November 2007Thumbnail for version as of 02:00, 23 November 2007450 × 450 (6.91 MB)WolfmanSF (talk | contribs)further truncation down to 131 frames
09:02, 22 November 2007Thumbnail for version as of 09:02, 22 November 2007450 × 450 (7.12 MB)WolfmanSF (talk | contribs)
10:01, 21 November 2007Thumbnail for version as of 10:01, 21 November 2007450 × 450 (9.01 MB)WolfmanSF (talk | contribs){{Information |Description=This movie sequence from Cassini shows dark drapes in the inner strands of the F ring caused by the gravitational influence of the shepherd moon Prometheus (102 kilometers, 63 miles across). Prometheus appears first in the sequ

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