Early Martian Dynamo Generation due to Giant Impacts

Details Early Martian Dynamo Generation due to Giant Impacts Early Martian Dynamo Generation due to Giant Impacts

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1948r&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1948

Physics

Scientific paper

Giant impacts produce localized melt regions facilitating rapid
iron-silicate segregation. Impactor iron heated by the collision can
carry thermal energy to the core and establish conditions favorable for
core cooling and dynamo generation.

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