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tectonics of the tharsis region of mars: insights from mgs topography and gravityWe have investigated the Tharsis region using gravity, topography, and geology to constrain a spherical thin shell model. We find that Tharsis likely formed primarily by volcanic construction, and has been largely unchanged since the Noachian.
Document ID
20000080643
Document Type
Conference Paper
Authors
Banerdt, W. Bruce
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Golombek, Matthew P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA 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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