檔案:PIA07712 - F ring animation.gif

PIA07712_-_F_ring_animation.gif(微格四五〇矩四五〇,度:三點四三 MB,多用網際網路副檔名之型:image/gif、循、六五幀、二六秒)

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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.
http://ciclops.org/view.php?id=1361
作者 NASA/JPL/Space Science Institute
其他版本
本圖像或影音收錄於美國國家航空暨太空總署 (NASA)噴射推進實驗室(Jet Propulsion Laboratory),其照片編號為: PIA07712

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描繪內容 繁體中文

成立或建立時間 繁體中文

一三 四 2005

多媒體型式 繁體中文

image/gif

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揀日尋檔。

日時用戶
二〇〇七年一一月二四日 (六) 一九時五一分於二〇〇七年一一月二四日 (六) 一九時五一分之縮四五〇矩四五〇(三點四三 MB)WolfmanSFReduce file size by deleting alternate frames. Double delay setting to maintain speed of animation.
二〇〇七年一一月二三日 (五) 〇九時四八分於二〇〇七年一一月二三日 (五) 〇九時四八分之縮四五〇矩四五〇(六點四四 MB)WolfmanSFtruncate down to 122 frames
二〇〇七年一一月二三日 (五) 〇二時〇〇分於二〇〇七年一一月二三日 (五) 〇二時〇〇分之縮四五〇矩四五〇(六點九一 MB)WolfmanSFfurther truncation down to 131 frames
二〇〇七年一一月二二日 (四) 〇九時〇二分於二〇〇七年一一月二二日 (四) 〇九時〇二分之縮四五〇矩四五〇(七點一二 MB)WolfmanSF
二〇〇七年一一月二一日 (三) 一〇時〇一分於二〇〇七年一一月二一日 (三) 一〇時〇一分之縮四五〇矩四五〇(九點〇一 MB)WolfmanSF{{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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