VIMS Observations of Titan's Surface

Details VIMS Observations of Titan's Surface VIMS Observations of Titan's Surface

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006agufm.p11a..02b&link_type=abstract

American Geophysical Union, Fall Meeting 2006, abstract #P11A-02

Physics

5400 Planetary Sciences: Solid Surface Planets, 5422 Ices, 5464 Remote Sensing, 6281 Titan

Scientific paper

By the time this talk is presented Cassini will have conducted over 20 flybys of Saturn's largest moon Titan. As a result of such intensive study, many questions regarding Titan's surface properties have been answered, but many more have emerged. The Visual and Infrared Mapping Spectrometer (VIMS) on Cassini provides unique data for the study of Titan's surface that addresses questions ranging from the surface composition of Titan to the nature of its geology and the processes that shape and modify it. This paper will focus on a discussion of the results of the last 5 flybys of Titan up to flyby T20.

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