Exploring Methods to Rule Out Surface Compositional Types on Titan Using Cassini VIMS T20 Data

Details Exploring Methods to Rule Out Surface Compositional Types on Titan Using Cassini VIMS T20 Data Exploring Methods to Rule Out Surface Compositional Types on Titan Using Cassini VIMS T20 Data

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1165b&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

1

Scientific paper

During the Oct. 25, 2006, Cassini T20 Titan flyby, VIMS observed Bohai
Sinus, a dune-free area exhibiting apparent color differences between
materials. Our goal is to develop methods to exclude possible non-H2O
endmember candidates for this region.

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