Relative equilibrium points in a variant of the restricted averaged four-body problem

Details Relative equilibrium points in a variant of the restricted averaged four-body problem Relative equilibrium points in a variant of the restricted averaged four-body problem

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976sva....19..784z&link_type=abstract

(Astronomicheskii Zhurnal, vol. 52, Nov.-Dec. 1975, p. 1314-1323.) Soviet Astronomy, vol. 19, no. 6, 1976, p. 784-788. Translat

Astronomy and Astrophysics

Astronomy

Four Body Problem, Lagrangian Equilibrium Points, Stationary Orbits, Euler-Lagrange Equation, Gravitational Fields, Long Term Effects, Oblate Spheroids, Orbit Perturbation, Satellite Perturbation, Synchronous Satellites

Scientific paper

Equilibrium points of a problem of motion of a mass-point in the
gravitational field of an oblate (at least triaxial) planet and two
perturbating bodies moving along eccentrical orbits with any inclination
are found. The perturbations due to an influence of two perturbating
bodies have the same order as those provided by the planet oblateness.

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