The theory of the rotational motion of Mercury and of synchronous satellites of planets

Details The theory of the rotational motion of Mercury and of synchronous satellites of planets The theory of the rotational motion of Mercury and of synchronous satellites of planets

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..235b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, May 1978, p. 235-239.) Soviet Astronomy Letters, vol. 4, May-June 1978, p. 128-131.

Astronomy and Astrophysics

Astronomy

Artificial Satellites, Mercury (Planet), Natural Satellites, Planetary Rotation, Solar Orbits, Synchronous Satellites, Celestial Bodies, Jupiter (Planet), Kepler Laws, Mars (Planet), Saturn (Planet)

Scientific paper

Intermediate resonance rotational motions are studied on the basis of integrable Delaunay-Hill averaging of the problem concerning the rotational motion of a triaxial rigid body that is traveling along a Keplerian elliptical orbit. Intermediate motions of this type are determined for resonance motions similar to those of the moon and Mercury. The basic properties of these intermediate motions are summarized.

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