CAOSP abstracts, Volume: 32, No.: 2, year: 2002

Abstract: The differential equations of the perturbed motion for the particular case of the nonrestricted three-bodies problem are received, using the classical method of variation of constants. As the perturbing function the terms of the third order in the Hamiltonian were used. The equations of the perturbed motion of the periastrons of the inner and outer orbits and the node were integrated by the iteration method. As the example the stellar system ξ UMa was used.

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Last update: February 12, 2003