Equilibrium points in the generalised photogravitational non-planar restricted three body problem

Abstract

We generalised the photogravitational non-planar restricted three body problem by considering the smaller primary as an oblate spheroid. With both the primaries radiating, we located the equilibrium points which lie outside the orbital plane, contrary to the classical case. Besides finding the equations of motion of the problem, two equilibrium points lie outside the plane, different from five such points in the classical case.