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Thermal Inertia, Albedo, and MOLA-derived Roughness for Terrains in the Terra Meridiani Area, MarsSurface 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. Additional information is contained in the original extended abstract.
Document ID
20020046275
Acquisition Source
Goddard Space Flight Center
Document Type
Abstract
Authors
Arvidson, R. E. (Washington Univ. Saint Louis, MO United States)
Deal, K. (Washington Univ. Saint Louis, MO United States)
Hynek, B. M. (Washington Univ. Saint Louis, MO United States)
Seelos, F. P., IV (Washington Univ. Saint Louis, MO United States)
Snider, N. O. (Washington Univ. Saint Louis, MO United States)
Mellon, M. T. (Colorado Univ. Boulder, CO United States)
Garvin, J. B. (NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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