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Orientation of a Satellite Located at the Libration Point in the Restricted Three-Body Problem

Published online by Cambridge University Press:  12 April 2016

Grzegorz Duliński
Affiliation:
Institute of Astronomy, Nicolaus Copernicus University, Chopina 12/18, 87-100 Toruń, Poland
Andrej J. Maciejewski
Affiliation:
Institute of Astronomy, Nicolaus Copernicus University, Chopina 12/18, 87-100 Toruń, Poland

Extract

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In this paper the initial results of an investigation of the motion of a rigid body located at the libration point in the planar, restricted three-body problem are given. This problem was analyzed in part by Kane and Marsh (1971), Markeev (1967a,b). However the present investigation is formulated in terms of hamiltonian mechanics. The final results will by used to study nonlinear effects connected with the gravitational influence of the “second” central body.

Type
Part I - Satellites and Planets
Copyright
Copyright © Reidel 1983

References

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Diliński, G. and Maciejewski, A.: 1983, in preparationGoogle Scholar
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Markeev, A.P.: 1967b, Kosm. Issled. 5, pp. 530540 Google Scholar
Markeev, A.P.: 1978, Libration Points in Celestial Mechanics and Astrodynamics, Nauka, Moscow (in Russian)Google Scholar
Markley, F.L.: 1978, in Wertz, J.R. (ed.), D. Reidel Publ. Company, ASSL Vol. 73 Google Scholar