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Retrograde Satellites in the Circular Plane Restricted Three-Body Problem

Published online by Cambridge University Press:  14 August 2015

D. Benest
D. Benest*
Affiliation:
Observatoire, Universitè de Nice, Le Mont-Gros, 06 Nice, France

Extract

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Characteristics and stability of simple-periodic retrograde satellites of the lighter body are presented for Hill's case and for all values of the mass ratio m2/(m1+m2) between 0 and 0.5.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 62: The Stability of the Solar System , 1974 , pp. 129
Copyright
Copyright © Reidel 1974