Thermal Inertia, Albedo, and MOLA-derived Roughness for Terrains in the Terra Meridiani Area, Mars

Details Thermal Inertia, Albedo, and MOLA-derived Roughness for Terrains in the Terra Meridiani Area, Mars Thermal Inertia, Albedo, and MOLA-derived Roughness for Terrains in the Terra Meridiani Area, Mars

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1748a&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1748

Physics

1

Scientific paper

Surface properties of layered deposits draped on dissected, cratered
terrain in the Terra Meridiani area are analyzed using remote sensing
data. The etched plains are cemented and differentially eroded, and the
hematite plains are loose and drifting.

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