This study was done to investigate the effect of perturbations of both oblate massive
primaries on the periodic orbit-attitude behavior of satellites at the three-body problem …

This paper deals with the existence of libration points and their linear stability when the more
massive primary is radiating and the smaller is an oblate spheroid. Our study includes the …

Abstract The Martian moon Phobos is becoming an appealing destination for future scientific
missions. The orbital dynamics around this planetary satellite is particularly complex due to …

This paper presents the study of the perturbed restricted problem of three bodies with an
elongated smaller primary and an oblate radiating bigger primary. The albedo effect and …

We explore a pseudo-Newtonian planar circular restricted three-body problem in which the
primaries are modeled using an approximate gravitational potential up to the second …

In the present work a systematic study has been presented in the context of the existence of
libration points, their linear stability, the regions of motion where the test particle can orbit …

The rotating mass dipole is possibly used to approximate the potential distribution of nearly
axisymmetrical elongated celestial bodies. To increase the accuracy of the approximation …

We locate and examine the stability of the 'out of plane'equilibrium points, L 6, 7 of an
infinitesimal body in the field of stellar-oblate binary systems moving in elliptic orbits around …

This study investigated periodic coupled orbit—attitude motions within the perturbed circular
restricted three-body problem (P-CRTBP) concerning the perturbations of a radiated …

As we know that the Sun is a source of radiation in our solar system, the other planets or
asteroids absorb some of the radiations incident on it and some reflected back into the …