Existence of Equilibrium Points in the Generalised Photogravitational Restricted Three Body Problem Space

We have found the position of equilibrium points in the generalised photogravitational restricted three body problem. The problem is generalised in the sense that both primaries are oblate spheroid. The position of equilibrium points depends on radiation and oblateness of both primaries. They are different from classical case. The oblateness affects the motion of the primaries. Further studies on this topic will be very useful in research areas in future research work.