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On The Stability of Stationary Solutions of the Twice-Averaged Hill’s Problem Taking Into Account The Planet Oblateness

Published online by Cambridge University Press:  12 April 2016

M.A. Vashkovyak
M.A. Vashkovyak*
Affiliation:
Keldysh Institute of Applied Mathematics, Russian Academy of Sciences, Miusskaya pl., 4, Moscow, 125047RussiaE-mail:vashkov@applmat.msk.su

Extract

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The problem of satellite orbital evolution with the combined influence of a distant perturbing body and the planet oblateness is well known (Laplace, 1805; Lidov, 1962, 1973; Kozai, 1963; Kudielka, 1994, 1997). The case of near-circular orbits is investigated in more details in (Sekiguchi, 1961; Allan and Cook, 1964; Vashkovyak, 1974).

Type
Extended Abstracts
Information
International Astronomical Union Colloquium , Volume 172: Impact of Modern Dynamics in Astronomy , 1999 , pp. 457
Copyright
Copyright © Kluwer 1999

References

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