Regolith Generation, Retention, and Movement on Asteroid Surfaces: Early Modeling Results

Details Regolith Generation, Retention, and Movement on Asteroid Surfaces: Early Modeling Results Regolith Generation, Retention, and Movement on Asteroid Surfaces: Early Modeling Results

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1084r&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1084

Physics

Scientific paper

A three-dimensional model of cratered surface evolution is used to
investigate the development of regolith layers on initially rocky,
S-type asteroid bodies as a function of time and accumulated impacts.

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