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A Note as to a Perturbation of Hill's Curves

Published online by Cambridge University Press:  14 August 2015

V. R. Matas
V. R. Matas*
Affiliation:
Astronomical Institute, Czechoslovak Academy of Sciences, Praha, Czechoslovakia

Abstract

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Let us consider motion of an infinitesimal body in the gravitational field of two homogeneous spheroids with coinoident equatorial planes. Let mass of the infinitesimal body M - a material point - be negligible if compared with masses of the spheroids S1, S2 respectively. We will study the motion of M in the common equatorial plane provided that the spheroids move along circular orbits (in an inertial frame of reference) - see Kondurar', 1952.

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. 33 - 36
Copyright
Copyright © Reidel 1979 

References

Kondurar', V.T.: 1952, “Trudy Gos. Astron. Inst. Shternberga” 21, pp. 135–158.Google Scholar
Matas, V.: 1978, Coles. Mech. (in press).Google Scholar