First High Solar Phase Angle Observations of Rhea Using Cassini VIMS: Upper Limits on Geologic Activity

Details First High Solar Phase Angle Observations of Rhea Using Cassini VIMS: Upper Limits on Geologic Activity First High Solar Phase Angle Observations of Rhea Using Cassini VIMS: Upper Limits on Geologic Activity

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1387p&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

In this work, we use Cassini's Visual and Infrared Mapping Spectrometer
(VIMS) solar phase angle data for Rhea (extended to phase angles up to
160°) to yield information on whether or not Rhea shows any evidence
for plume activity.

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