Titan: Surface Composition from Cassini VIMS

Details Titan: Surface Composition from Cassini VIMS Titan: Surface Composition from Cassini VIMS

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1398m&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1398

Computer Science

1

Scientific paper

The surface composition of Titan was explored using Cassini VIMS data.
Surface compositional units appear. Dirty water ice is consistent with
the visually dark units but no compositional match for the visually
bright units was found.

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