The Main Belt and NEA Size Distributions: Linked Collisionaland Dynamical Evolution

Details The Main Belt and NEA Size Distributions: Linked Collisionaland Dynamical Evolution The Main Belt and NEA Size Distributions: Linked Collisionaland Dynamical Evolution

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.2018o&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.2018

Other

Scientific paper

We model the combined collisional and dynamical evolution of the main
belt and NEA populations, and obtain results that are consistent with
observations and other constraints. We discuss the implications for the
cratering records on asteroids.

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