Stability of Binary Asteroids Formed Through Fission

Details Stability of Binary Asteroids Formed Through Fission Stability of Binary Asteroids Formed Through Fission

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1632s&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1632

Physics

1

Scientific paper

The evolution of NEA contact binaries to orbital binaries due to spin-up
effects (such as YORP) is discussed. The stability of the resulting
systems indicate a strong preference for the formation of binary systems
with non-elongate primaries.

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