Bolometric Bond Albedos For Saturnian Satellites From Cassini VIMS: Leading and Trailing Hemispheres

Details Bolometric Bond Albedos For Saturnian Satellites From Cassini VIMS: Leading and Trailing Hemispheres Bolometric Bond Albedos For Saturnian Satellites From Cassini VIMS: Leading and Trailing Hemispheres

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2035p&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2035

Physics

Scientific paper

We present values of disk-integrated bolometric Bond albedo, phase
integrals, and geometric albedos, derived using Cassini VIMS solar phase
curves at 7-15 wavelengths, for the saturnian satellites Rhea, Dione,
Tethys, Mimas, and Enceladus.

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