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Titan's global map combining VIMS and ISS mosaicsTitan, Saturn’s largest moon, is the only ocean world, besides Earth, with a dense atmosphere. This outstanding feature is also a challenge since it was believed before the launch of the Cassini mission that optical cameras (visible and infrared) could not see the surface and that only radar instruments could map Titan’s surface. However, the Visual and Infrared
Mapping Spectrometer (VIMS) and the Imaging Science Subsystem (ISS) onboard the Cassini spacecraft demonstrated that Titan’s surface can be observed in several infrared atmospheric windows.
Document ID
20210012227
Acquisition Source
Jet Propulsion Laboratory
Document Type
Preprint (Draft being sent to journal)
External Source(s)
Authors
Turtle, Elizabeth P.
Sotin, Christophe
Pasek, Virginia
Karkoschka, Erick
Joseph, Emily C.S.
Brown, Robert H.
Le Mouelic, Stephan
Seignovert, Benoit
Date Acquired
September 15, 2019
Publication Date
September 15, 2019
Publication Information
Publisher: Pasadena, CA: Jet Propulsion Laboratory, National Aeronautics and Space Administration, 2019
Distribution Limits
Public
Copyright
Other
Technical Review

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