One resonance case of the perturbed motion of the satellite of a spheroidal planet

Details One resonance case of the perturbed motion of the satellite of a spheroidal planet One resonance case of the perturbed motion of the satellite of a spheroidal planet

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981kosis..19..133m&link_type=abstract

Kosmicheskie Issledovaniia, vol. 19, Jan.-Feb. 1981, p. 133-136. In Russian.

Physics

Celestial Mechanics, Natural Satellites, Orbit Perturbation, Perturbation Theory, Equations Of Motion, Hamiltonian Functions, Quadratures, Resonance, Spheroids

Scientific paper

Doubly averaged (in the sense of Delaunay-Hill) Hamiltonians of equations of the perturbed motion of the satellite of a spheroidal planet in action-angle variables are reduced to quadratures. It is assumed that nonperturbed motion is determined by the generalized problem of two fixed centers; the influence of the perturbing body is taken into account.

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