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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
Abstract
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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