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The Dynamics of NEO Binary Asteroids

Published online by Cambridge University Press:  01 August 2006

D.J. Scheeres*
Affiliation:
Dept. of Aerospace Engineering, The University of Michigan, Ann Arbor, MI 48109-2140, USA, email: scheeres@umich.edu
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Abstract

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The dynamics of binary Near-Earth objects (NEO) are discussed and a simple model for the study of their dynamics is introduced. Main results on the motion and stability of binary asteroids are reviewed. The effect of perturbations external to the binary system, including solar gravity, solar radiation pressure, and planetary gravity, are considered.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

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