Plane periodic motions of a satellite with respect to the center of mass near the triangular libration point.

Details Plane periodic motions of a satellite with respect to the center of mass near the triangular libration point. Plane periodic motions of a satellite with respect to the center of mass near the triangular libration point.

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989cosre..27..290d&link_type=abstract

Cosmic Res., Vol. 27, No. 3, p. 290 - 295

Physics

Three-Body Problem: Restricted, Three-Body Problem: Periodic Orbits

Scientific paper

The periodic motions of a satellite about the center of mass on periodic orbits near L4 of the restricted circular three-body problem are investigated. It is assumed that the satellite is a rigid body with a triaxial central ellipsoid of inertia. The problem of the existence of (2πn)-periodic motions produced by plane rotations and oscillations of arbitrary amplitude and their stability are examined.

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