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Stationary Solutions of the Averaged Three-Body Problem and Some Problems of Planet Motion Stability

Published online by Cambridge University Press:  14 August 2015

G. A. Krasinsky
G. A. Krasinsky*
Affiliation:
Institute of Theoretical Astronomy, Leningrad, U.S.S.R.

Abstract

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A general theory of stationary solutions of the averaged N-body problem is briefly described. Numerical results in some particular cases (general three-body problem in the nonresonant case and restricted circular problem both in the nonresonant and resonant ones) are presented. Some applications into the problem of planetary stability are developed.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 62: The Stability of the Solar System , 1974 , pp. 95 - 116
Copyright
Copyright © Reidel 1974 

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