Thermal evolution of Venus - A preliminary study based on tectonic feature spacing

Details Thermal evolution of Venus - A preliminary study based on tectonic feature spacing Thermal evolution of Venus - A preliminary study based on tectonic feature spacing

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..883m&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 883.

Physics

Tectonics, Venus Surface, Temperature Gradients, Brittleness, Lithosphere

Scientific paper

The surface of Venus consists predominantly of structures formed since
the 300-500 ma resurfacing event. Subsequent to this event, the
lithosphere underwent a period of rapid cooling. This cooling resulted
in a decrease in the global thermal gradient over time.

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