Lunar Meteorite Source Crater Size: Constraints from Impact Simulations

Details Lunar Meteorite Source Crater Size: Constraints from Impact Simulations Lunar Meteorite Source Crater Size: Constraints from Impact Simulations

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1768h&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1768

Physics

2

Scientific paper

Hydrocode simulations show that craters 450 m across are viable sources
of the lunar meteorites. The number of such craters expected to form in
the last 0.1 Ma agrees with the CRE data. Samples from older events are
underrepresented.

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