The photogravitational restricted three bodies within the framework of the post-Newtonian
approximation is carried out. The mass of the primaries are assumed changed under the …

This paper examines the motion of a test particle in the vicinity of the triangular points L 4, 5
by considering the more massive primary as a source of radiation in the framework of the …

The photogravitational restricted three body within the framework of the post-Newtonian
approximation is carried out. The mass of the primaries are assumed changed under the …

The problem of restricted three bodies is considered. The treatment is carried out within the
framework of the post‐Newtonian approximation. The primaries also are assumed to be …

The centrifugal and Coriolis forces do not appear as a result of physically imposed forces,
but are due to a special property of a rotation. Thus, these forces are called pseudo-forces or …

The restricted three-body problem is studied in the post-Newtonian framework. The
primaries are assumed oblate radiant sources. The perturbed location of the L 1 point is …

In the present work, the periodic orbits around the relativistic restricted three-body problem
(in brief relativistic RTBP) is treated. The equations of motion of the relativistic restricted …

In the present article the effects of the relativistic, photogravitational and oblateness
perturbations in restricted three-body problem, in brief R3BP are investigated. The relativistic …

In this work the stability of all equilibrium points in the photogravitational relativistic restricted
three-body problem (RTBP) with oblate primaries is investigated for arbitrary RTBP systems …

In this paper we calculate the volume, mass, gravitational attraction to the Earth, angular
momentum the orbit of the Trojan asteroid (TK7)[1]. In this paper, we use classical …