Periodic motions with respect to the center of mass of an axisymmetric satellite in elliptic orbit

Details Periodic motions with respect to the center of mass of an axisymmetric satellite in elliptic orbit Periodic motions with respect to the center of mass of an axisymmetric satellite in elliptic orbit

Jul 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977kosis..15..526b&link_type=abstract

Kosmicheskie Issledovaniia, vol. 15, July-Aug. 1977, p. 526-532. In Russian.

Astronomy and Astrophysics

Astronomy

Center Of Gravity, Elliptical Orbits, Orbit Perturbation, Satellite Rotation, Astrodynamics, Periodic Functions, Perturbation Theory, Poincare Problem

Scientific paper

In the present paper, Poincare's small parameter method is used to
analyze the existence of periodic rotational motions of an axisymmetric
satellite moving along an elliptic orbit. The conditions for the
existence of periodic solutions are derived in analytical form, and are
studied qualitatively and quantitatively.

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