Titan’s Surface What we might see
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Titan’s Surface What we might see Torrence V. Johnson Cassini Imaging Science Team
description
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. - PowerPoint PPT Presentation
Transcript of Titan’s Surface What we might see
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Titan’s SurfaceWhat we might see
Torrence V. JohnsonCassini Imaging Science Team
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Titan: The Ultimate Icy Satellite?
• Subsurface-Oceans?• Craters?• Surface liquid hydrocarbons
– YES• Atmospheric interactions?• And what else??
![Page 3: Titan’s Surface What we might see](https://reader036.fdocuments.in/reader036/viewer/2022062814/5681680a550346895ddd8e70/html5/thumbnails/3.jpg)
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Keck 2 / NIRC2, Nov-Dec. 2004K' surface albedo map
Titan Surface Albedo Maps
Cassini ISS Approach Map 0.95 m continuum
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CassiniISS
CassiniVIMS