The possible motions of a satellite about an oblate planet

Details The possible motions of a satellite about an oblate planet The possible motions of a satellite about an oblate planet

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983cemec..30...49z&link_type=abstract

Celestial Mechanics (ISSN 0008-8714), vol. 30, May 1983, p. 49-58.

Astronomy and Astrophysics

Astronomy

3

Angular Momentum, Astrodynamics, Natural Satellites, Oblate Spheroids, Planetary Orbits, Circular Orbits, Equations Of Motion, Equatorial Orbits, Hamiltonian Functions, Hill Method

Scientific paper

The regions of motions of a satellite for given values of energy and
angular momentum about polar axes are shown. Special attention is paid
to the circular equatorial orbits which have been shown to bee Hill
stable. The anomalistic and the nodal period for the motions near to the
circular equatorial orbits have been found.

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