Constraints on the NEO Impact Frequency from Analysis and Modeling of Apollo Impact Events

Details Constraints on the NEO Impact Frequency from Analysis and Modeling of Apollo Impact Events Constraints on the NEO Impact Frequency from Analysis and Modeling of Apollo Impact Events

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1416l&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

The lunar impact frequency is analysed from events recorded by the
Apollo seismometers. Models of Ivanov et al. [2003] or Ortiz et al.
[2006] provide a better match with the lunar seismic observations than
those of Brown et al. [2002].

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