Stability of the coplanar libration points in the photogravitational three-body problem. II

Details Stability of the coplanar libration points in the photogravitational three-body problem. II Stability of the coplanar libration points in the photogravitational three-body problem. II

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..722t&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Sept. 1986, p. 722-725) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Sept.-O

Astronomy and Astrophysics

Astronomy

1

Coplanarity, Librational Motion, Motion Stability, Particle Motion, Stellar Gravitation, Three Body Problem, Astronomical Models, Binary Stars, Liapunov Functions, Radiation Pressure

Scientific paper

The Liapunov stability of the relative equilibrium positions (coplanar libration points) is investigated for a particle in a gas-dust cloud subject to the gravitational field and radiation pressure of a binary star whose components have an arbitrary mass ratio. The dynamical model adopted is the restricted circular photogravitational three-body problem. Some earlier results for the libration points are extended and refined.

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