Long-Wavelength Topography and Gravity Anomalies of Mars and Their Implications to the Formation of Tharsis Rise

Details Long-Wavelength Topography and Gravity Anomalies of Mars and Their Implications to the Formation of Tharsis Rise Long-Wavelength Topography and Gravity Anomalies of Mars and Their Implications to the Formation of Tharsis Rise

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.2124z&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.2124

Physics

1

Scientific paper

We study internal and surface loading for Mars with viscous and
viscoelastic rheology. We show that convection models with a viscous
rheology greatly overestimate the geoid and that the low degree geoid
may be largely induced by surface loading of the Tharsis.

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