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This stunning false-color view of Hyperion reveals crisp details and differences in color across the strange, tumbling moonís surface that represent differences in the composition of surface materials. The view was obtained during Cassiniís very close flyby on September 26, 2005.
Hyperion has a notably reddish tint when viewed in natural color. The red color was toned down in this false-color view, and the other hues were enhanced, in order to make more subtle color variations across Hyperionís surface more apparent.
Cassini scientists think that Hyperionís unusual appearance can be attributed to the fact that it has an unusually low density for such a large object, giving it weak surface gravity and high porosity. These characteristics help preserve the original shapes of Hyperionís craters by limiting the amount of impact ejecta coating the moonís surface. Impactors tend to make craters by compressing the surface material, rather than blasting it out. Further, Hyperionís weak gravity, and correspondingly low escape velocity, means that what little ejecta is produced has a good chance of escaping the moon altogether.
Images taken using infrared, green and ultraviolet spectral filters were combined to create this view. The images were taken with the narrow angle camera from a distance of approximately 62,000 kilometers (38,500 miles) from Hyperion and at a Sun-Hyperion-spacecraft, or phase, angle of 52 degrees. The image scale is 362 meters (1,200 feet) per pixel.
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.