The photogravitational restricted three-body problem: Comments on the 'out-of-plane' equilibrium points

Details The photogravitational restricted three-body problem: Comments on the 'out-of-plane' equilibrium points The photogravitational restricted three-body problem: Comments on the 'out-of-plane' equilibrium points

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.215..237t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 215, no. 2, p. 237-243

Astronomy and Astrophysics

Astrophysics

3

Celestial Mechanics, Equilibrium, Gravitation, Gravitational Effects, Lagrangian Equilibrium Points, Orbital Mechanics, Three Body Problem, Binary Stars, Dynamic Stability, Radiation Pressure, Stellar Gravitation, Stellar Motions, Stellar Systems

Scientific paper

The photogravitational restricted three-body problem is reviewed and the
case of the 'out-of-plane' equilibrium points is analysed. It is found
that, when the motion of an infinitesimal body is determined only by the
gravitational forces and effects of the radiation pressure, there are no
'out-of-plane' stable equilibrium points.

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