Asteroid Collisional Evolution: Implications for Internal Structure

Details Asteroid Collisional Evolution: Implications for Internal Structure Asteroid Collisional Evolution: Implications for Internal Structure

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1506c&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1506

Physics

Scientific paper

A new model of asteroid collisional evolution is constrained by a size
distribution inferred from crater size distributions on the Moon,
Mercury and Mars. The asteroid size distribution is constrained to
evolve over 3.9 Gy to the present day state.

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