Geoid to Topography Ratios on Venus and Implications for Crustal Thickness

Details Geoid to Topography Ratios on Venus and Implications for Crustal Thickness Geoid to Topography Ratios on Venus and Implications for Crustal Thickness

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2663j&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2663

Physics

1

Scientific paper

Using gravity and topography data from the Magellan mission, we develop
a crustal thickness map of Venus. We also calculate geoid to topography
ratios in order to identify regions of dynamic support.

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