Abstract
In the first part of the paper, the notion of evolution is introduced, as opposed to that of stability and instability. A definition is proposed that involves the variations of the energy and angular momentum integrals of a subgroup of an isolated N body system.
When there are only gravitational interactions between the bodies, the conditions for evolution are outlined and some examples are given. This is in particular applied to the case when there exists a massive central body.
Several examples of evolution when non-conservative forces are also acting are proposed. It is shown that evolution takes place because generally there exists a non-vanishing component of the disturbing force perpendicular to the radius vector in the orbital plane. This is the case of the atmospheric drag, of the Poynting-Robertson effect and of tidal effects. Some details are presented for the latter and the results are applied to the evolution of the Earth-Moon system.
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© 1988 Kluwer Academic Publishers
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Kovalevsky, J. (1988). Orbital Evolution. In: Roy, A.E. (eds) Long-Term Dynamical Behaviour of Natural and Artificial N-Body Systems. NATO ASI Series, vol 246. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3053-7_4
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DOI: https://doi.org/10.1007/978-94-009-3053-7_4
Publisher Name: Springer, Dordrecht
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