The restricted photogravitational three-body problem: A modern state

Details The restricted photogravitational three-body problem: A modern state The restricted photogravitational three-body problem: A modern state

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26at....6..283k&link_type=abstract

Astronomical and Astrophysical Transactions (ISSN 1055-6796), vol. 6, no. 4, p. 283-293

Mathematics

Logic

10

Celestial Mechanics, Libration, Mass Ratios, Particle Mass, Radiation Pressure, Three Body Problem, Dynamic Stability, Gravitational Effects, Linear Equations, Nonlinear Equations, Pressure Effects, Surface Properties

Scientific paper

We discuss a modern state of the three-body problem when an infinitesimal mass is effected not only by gravitation but also by light pressure from one (or both) of the primaries. This problem, called the photogravitational one, attracted much attention during the last ten years. Many aspects of the libration point locations and their stability for all values of radiation pressure and mass ratios are shown and discussed. A retrospective chronological review of the results is given.

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