The rotational motion of an axisymmetric satellite in the case of resonance

Details The rotational motion of an axisymmetric satellite in the case of resonance The rotational motion of an axisymmetric satellite in the case of resonance

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980sval....6..343m&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Sept.-Oct. 1980, p. 654-658.) Soviet Astronomy Letters, vol. 6, Sept.-Oct. 1980, p.

Astronomy and Astrophysics

Astronomy

Axisymmetric Bodies, Orbital Mechanics, Resonance, Satellite Perturbation, Satellite Rotation, Libration, Perturbation Theory, Three Body Problem

Scientific paper

A first approximation to the rotational motion of an axisymmetric
satellite in the resonance case is obtained by means of perturbation
theory on the basis of intermediate motion. The satellite is taken at
the triangular libration point L sub 4 of the circular restricted
three-body problem.

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