CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Color Variation Across Rhea and Dione
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Color Variation Across Rhea and Dione
PIA 07769

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  The cratered ice moons Rhea and Dione come alive with vibrant color that reveals new information about their surface properties.

To create these false-color views, ultraviolet, green and infrared images were combined into a single black and white picture that isolates and maps regional color differences. This "color map" was then superposed over a clear-filter image of each moon.

The combination of color map and brightness image shows how the colors vary across the moon's surface in relation to geologic features. The origin of the color differences is not yet understood, but may be caused by subtle differences in the surface composition or the sizes of grains making up the icy soil.

The Rhea view is a 2x1 mosaic. Images in the mosaic were acquired on August 1, 2005 at a mean distance of 214,700 kilometers (133,400 miles) from Rhea and at a Sun-Rhea-spacecraft, or phase, angle of 88 degrees. Image scale is 1.3 kilometers (0.8 miles) per pixel.

The mosaic shows terrain on the trailing hemisphere of Rhea (1,528 kilometers, 949 miles across) and is centered on 42 degrees south latitude. North is up and rotated 28 degrees to the left.

Images in the Dione false-color view were acquired on August 1, 2005 at a mean distance of 267,600 kilometers (166,300 miles) from Dione. Image scale is 1.6 kilometers (1 mile) per pixel.

The image shows terrain on the trailing hemisphere of Dione (1,123 kilometers, 698 miles cross) and is centered on 41 degrees south latitude. North is up.

The images have not been scaled to show the moons' proper relative sizes.

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.

Credit: NASA/JPL/Space Science Institute
Released: December 6, 2005 (PIA 07769)
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