Evolution of Small Near-Earth Asteroid Binaries

Details Evolution of Small Near-Earth Asteroid Binaries Evolution of Small Near-Earth Asteroid Binaries

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..647j&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.647

Physics

Scientific paper

Stable small, binary asteroid systems will evolve according to three
processes: the YORP effect, mutual body tides, and the binary YORP
(BYORP) effect. The interplay of these effects on the dynamics of the
system must result in the observed binary asteroid systems: asynchronous
binaries, synchronous binaries, and doubly synchronous binaries.

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