The stability of periodic motions of a satellite relative to its own center of mass

Details The stability of periodic motions of a satellite relative to its own center of mass The stability of periodic motions of a satellite relative to its own center of mass

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..631b&link_type=abstract

Kosmicheskie Issledovaniia, vol. 20, July-Aug. 1982, p. 631-634. In Russian.

Computer Science

Numerical Analysis

Center Of Mass, Orbit Perturbation, Satellite Rotation, Spacecraft Stability, Axes Of Rotation, Elliptical Orbits, Motion Stability, Periodic Functions

Scientific paper

The paper examines the periodic rotational motions of a rigid satellite
with a dynamic-symmetry axis, under the assumption that its center of
mass moves in a Keplerian elliptical orbit in a central Newtonian field.
A numerical analysis of the stability of the appropriate periodic
solutions is presented.

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