Bruce Murray Space Image Library

Color view of Titan from VIMS

Color view of Titan from VIMS
Color view of Titan from VIMS Combining three images taken at wavelengths of 2.0, 2.8, and 5.0 microns gives VIMS a colorful map of Titan's surface, indicating plenty of surface diversity, not a global ocean of methane, and no specular reflections. (The bright spot, near the south pole, is because of clouds there.) NASA / JPL-Caltech / University of Arizona

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