Crustal Thickening Above a Convecting Mantle with Application to Venus and Mars

Details Crustal Thickening Above a Convecting Mantle with Application to Venus and Mars Crustal Thickening Above a Convecting Mantle with Application to Venus and Mars

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1652c&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1652

Physics

Scientific paper

It has been suggested that highlands on Venus have formed via crustal
thickening over mantle downwellings. To evaluate the physical
plausibility of this hypothesis, we explore a simplified system of
chemical layer thickening above a convecting mantle.

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