Using Surface Thermal Inertia to Estimate the Thickness of the Iapetian Dark Material

Details Using Surface Thermal Inertia to Estimate the Thickness of the Iapetian Dark Material Using Surface Thermal Inertia to Estimate the Thickness of the Iapetian Dark Material

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1073r&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1073

Physics

Scientific paper

Using CIRS surface temperature readings of Iapetus, the new global
Iapetian bolometric Bond albedo map, and our thermal model, we provide
thermal constraints on the thickness of the dark material overburden.

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