Physics
Scientific paper
May 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..371z&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, May-June 1985, p. 371-381. In Russian.
Physics
Natural Satellites, Planetary Orbits, Satellite Perturbation, Satellite Rotation, Stationary Orbits, Three Body Problem, Angular Velocity, Axisymmetric Bodies, Canonical Forms, Celestial Mechanics, Earth-Moon System, Mass Ratios, Resonance, Translational Motion
Scientific paper
The translational-rotational motion of a resonant satellite in the gravitational field of a triaxial planet is investigated with allowance for perturbations from a third body moving in a Keplerian orbit. The method used involves the finding of stationary and conditional-periodic solutions of the canonical systems of differential equations for sharp frequency resonance. Families of stationary solutions defining the translational-rotational motion of an axisymmetric satellite are obtained in the case of the variation of parameters characterizing the figure of the planet and the relative mass of the perturbing body. Values of parameters close to those which characterize the earth-moon system are taken as the input quantities.
Tagaev A. T.
Zhuravlev S. G.
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