Asymptotic orbits at the triangular equilibria in the photogravitational restricted three-body problem (Q863217)

In the present paper the asymptotic homoclinic and heteroclinic orbits associated with the triangular equilibrium points in the gravitational and the photogravitational restricted plane circular three-body problem were studied numerically. Many of asymptotic orbits for equal masses of the primaries and various values of the radiation pressure are computed and some interesting of them are illustrated. It is found that the mass parameter has stronger influence on the structure of the orbits than the radiation factor.