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Periodic Orbits of Arbitrary Inclinations and Eccentricities in the General 3-Body Problem
Published online by Cambridge University Press: 14 August 2015
Abstract
Usual periodic orbits have periods of the order of magnitude of a few revolutions. However if we consider much longer periods it is possible to find, for three given masses, periodic orbits in any neighbourhood of arbitrary given initial eccentricities and inclinations provided that the distance of the outer body is sufficiently large with respect to the mutual distance of the two inner bodies.
- Type
- Part I: Stability, N- and 3-Body Problems, Variable Mass
- Information
- Symposium - International Astronomical Union , Volume 81: Dynamics of the Solar System , 1979 , pp. 29 - 32
- Copyright
- Copyright © Reidel 1979