CICLOPS: Cassini Imaging Central Laboratory for OPerationS
Pandora's Color Close-up

Pandora's Color Close-up
PIA 07632

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  Cassini's best close-up view of the F ring shepherd moon, Pandora, shows that this small ring moon is mantled in fine dust-sized icy material.

Craters formed on this object by impacts appear to be covered by debris, a process that probably happens rapidly in a geologic sense. The crisp craters on Saturn's moon Hyperion provide a contrasting example of craters on a small object (see PIA07740).

The grooves and small ridges on Pandora (81 kilometers, 50 miles across) suggest that fractures affect the overlying smooth material.

Cassini acquired infrared, green and ultraviolet images on Sept. 5, 2005 which were combined to create this false color view. The image was taken with the Cassini narrow-angle camera at a distance of approximately 52,000 kilometers (32,000 miles) from Pandora and at a Sun-Pandora-spacecraft, or phase, angle of 54 degrees. Resolution in the original image was about 300 meters (1,000 feet) per pixel. The image has been magnified by a factor of two to aid visibility.

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 and the Cassini imaging team home page,

Credit: NASA/JPL/Space Science Institute
Released: November 16, 2005 (PIA 07632)
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