The Effects of Dynamic Topography and Thermal Isostasy on the Topography and Geoid of Venus

Details The Effects of Dynamic Topography and Thermal Isostasy on the Topography and Geoid of Venus The Effects of Dynamic Topography and Thermal Isostasy on the Topography and Geoid of Venus

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1811o&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

1

Scientific paper

The magnitude of the dynamic topography on Venus is small. Long
wavelength global geoid and topography anomalies can be explained by
thermal thinning of a thick lithosphere with only a limited contribution
from crustal thickness variations.

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