Quasi-Static Evolution of Self-gravitating Aggregates

Details Quasi-Static Evolution of Self-gravitating Aggregates Quasi-Static Evolution of Self-gravitating Aggregates

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..584s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.584

Physics

1

Scientific paper

Analytical and numerical approaches to understanding the evolution of rubble pile asteroids under increasing angular momentum (due to YORP) are studied. Exact analytical results can be found for few particle systems and provide stringent tests for numerical simulations for rubble piles with large numbers of self-gravitating grains. We test the limits of acceleration rate needed to reproduce quasi-static behavior and how aggregates will change with increasing numbers of grains.

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