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lithospheric structure from mars global surveyor topography and gravity and implications for the early thermal evolution of marsRegional variations in the thickness of the elastic lithosphere on Mars derived from a combined analysis of topography and gravity anomalies determined by Mars Global Surveyor provide new insight into the planet's thermal history.
Document ID
20000080639
Document Type
Conference Paper
Authors
Solomon, Sean C.
(Carnegie Institution of Washington Washington, DC United States)
Zuber, Maria T.
(Massachusetts Inst. of Tech. Cambridge, MA United States)
Phillips, Roger J.
(Washington Univ. Saint Louis, MO United States)
Smith, David E.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Tyler, G. Leonard
(Stanford Univ. Stanford, CA United States)
Aharonson, Oded
(Massachusetts Inst. of Tech. Cambridge, MA United States)
Balmino, Georges
(Groupe de Recherches de Geodesie Spatiale Toulouse, France)
Banerdt, W. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Head, James W.
(Brown Univ. Providence, RI United States)
Johnson, Catherine L.
(Carnegie Institution of Washington Washington, DC United States)
Date Acquired
August 19, 2013
Publication Date
March 1, 2000
Publication Information
Publication: Lunar and Planetary Science XXXI
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle20000080557Analytic PrimaryLunar and Planetary Science XXXI