A NUMERICAL STUDY OF THE INFLUENCE OF THE POYNTING-ROBERTSON EFFECT ON THE EQUILIBRIUM POINTS OF THE PHOTOGRAVITATIONAL RESTRICTED 3-BODY PROBLEM .2. OUT-OF-PLANE CASE
O. Ragos et al., A NUMERICAL STUDY OF THE INFLUENCE OF THE POYNTING-ROBERTSON EFFECT ON THE EQUILIBRIUM POINTS OF THE PHOTOGRAVITATIONAL RESTRICTED 3-BODY PROBLEM .2. OUT-OF-PLANE CASE, Astronomy and astrophysics, 300(2), 1995, pp. 579-590
The photogravitational circular restricted three-body model including
the Poynting-Robertson effect is employed to describe the motion of a
particle in the vicinity of two massive radiating bodies. The equilibr
ium points lying out of the orbital plane of the primaries are studied
numerically. The exact number of these points is determined by means
of the topological degree theory. Subsequently, a modified bisection m
ethod is used to compute the positions of the equilibrium. Finally the
ir stability is studied.