The Collisional Evolution of the Main Belt Population

Details The Collisional Evolution of the Main Belt Population The Collisional Evolution of the Main Belt Population

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1696k&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1696

Computer Science

Scientific paper

Within our model of disruptive cascade populations we adjust the best
size-strength scaling relations for asteroidal strength. To compare with
the lunar size-frequency crater distribution we smooth the obtained
populations with a sliding time window of 2 Ma.

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