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Titan’s Surface What we might see. Torrence V. Johnson Cassini Imaging Science Team. Titan: The Ultimate Icy Satellite?. Subsurface-Oceans? Craters? Surface liquid hydrocarbons – YES Atmospheric interactions? And what else??. Cassini ISS Approach Map 0.95 m continuum.
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Titan’s SurfaceWhat we might see Torrence V. Johnson Cassini Imaging Science Team
Titan: The Ultimate Icy Satellite? • Subsurface-Oceans? • Craters? • Surface liquid hydrocarbons – YES • Atmospheric interactions? • And what else??
Cassini ISS Approach Map 0.95 m continuum Keck 2 / NIRC2, Nov-Dec. 2004 K' surface albedo map Titan Surface Albedo Maps
Cassini ISS Cassini VIMS