Numerical Simulation of Heating of Target at Crater-Field-forming Impact Events

Details Numerical Simulation of Heating of Target at Crater-Field-forming Impact Events Numerical Simulation of Heating of Target at Crater-Field-forming Impact Events

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1351o&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1351

Physics

1

Scientific paper

We show that small (10-100 m) meteorite craters may have significant
amount of target material heated to several hundred degrees. Some
meteoritic and heated material are spread as ejecta, but the majority
remains within the crater, most likely at great depth near the center.

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