Heating of the Martian Interior Due to Giant Impacts: Revisited

Details Heating of the Martian Interior Due to Giant Impacts: Revisited Heating of the Martian Interior Due to Giant Impacts: Revisited

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2049r&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2049

Physics

Scientific paper

Heating from giant impacts has been suggested as a possible cause for
the cessation of the martian dynamo. Core heat flow heterogeneity and
shock heating models are revisited to better understand how impacts can
affect the thermal evolution of Mars.

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