Stationary motions of an axisymmetric satellite in circular orbit

Details Stationary motions of an axisymmetric satellite in circular orbit Stationary motions of an axisymmetric satellite in circular orbit

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..176a&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, Mar.-Apr. 1989, p. 176-179. In Russian.

Physics

3

Celestial Mechanics, Circular Orbits, Satellite Orientation, Spacecraft Motion, Axisymmetric Bodies, Hamiltonian Functions, Harmonic Analysis, Kepler Laws

Scientific paper

Stationary solutions are obtained to the problem of the rotation of a rigid axisymmetric satellite whose mass center moves in circular Keplerian orbit. The second and third harmonics are conserved in the force-function expansion. In particular, solutions are obtained which generalize the conical and hyperbolic precession of a satellite described by Sarychev (1978).

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