On the rapid rotations of a satellite at a triangular libration point

Details On the rapid rotations of a satellite at a triangular libration point On the rapid rotations of a satellite at a triangular libration point

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983kosis..21..794m&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 21, Sept.-Oct. 1983, p. 794-797. In Russian.

Physics

2

Equations Of Motion, Libration, Orbital Mechanics, Satellite Rotation, Angular Velocity, Center Of Mass, Motion Stability, Three Body Problem

Scientific paper

An analysis is made of the rotational motion of a three-axis satellite with respect to its mass center under the assumption that this center is located at the L4 triangular libration point in the restricted circular three-body problem. The basic parameters of intermediate motion of the rapidly rotating satellite are determined, and it is noted that the rapid-rotation regime can be considered as a source of possible steady motions.

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