Plume-induced Topography and Geoid Anomalies and Their Implications for the Tharsis Rise on Mars

Details Plume-induced Topography and Geoid Anomalies and Their Implications for the Tharsis Rise on Mars Plume-induced Topography and Geoid Anomalies and Their Implications for the Tharsis Rise on Mars

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1125r&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1125

Physics

1

Scientific paper

Elastic stresses in the Martain lithosphere reduce the dynamic
topography created by plume buoyancy. The associated geoid becomes very
small, inconsistent with that observed for Tharsis, suggesting that
Tharsis is not dynamically supported.

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