Stability analysis in the R3BP under the effect of heterogeneous spheroid

K Shalini, MJ Idrisi, JK Singh, MS Ullah - New Astronomy, 2023 - Elsevier
In this paper, we investigate motion of infinitesimal mass m in the restricted three-body
problem using heterogeneous spheroid with three layers. We consider the less massive …

Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three‐Body Problem under the Effect of Asteroids Belt

F Bouaziz-Kellil - Advances in Astronomy, 2020 - Wiley Online Library
The present paper deals with the study of the motion's properties of the infinitesimal variable
mass body moving in the same orbital plan as two massive bodies (considered as …

Albedo effects in the ER3BP with an oblate primary, a triaxial secondary and a potential due to belt

J Singh, TK Richard - Scientific Reports, 2023 - nature.com
We have examined the effects of Albedo in the Elliptic Restricted Three-Body Problem
(ER3BP) with an oblate primary, a triaxial secondary, and potential due to belt for the Earth …

Non-Linear Stability in the CR3B Problem under the Effects of Beyond-Newtonian Dynamics and Kerr Like Primaries

SN Prasad, Abdullah, B Singh, K Shalini - Astronomy Reports, 2024 - Springer
In the present research work, we have carried out an analysis of the non-linear stability of
the circular restricted three-body problem (CR3BP) with Kerr-like primaries. The model …

Effect of perturbed potential of heterogeneous triaxial rigid bodies of N layers on the stability of libration points in the R3BP

K Shalini, P Sharma, K Ranjana - New Astronomy, 2024 - Elsevier
In this paper, we investigate the motion of an infinitesimal mass m 3 in the restricted three-
body problem by taking both the primaries as heterogeneous triaxial rigid bodies with N …

[HTML][HTML] ALBEDO EFFECTS IN THE ELLIPTIC RESTRICTED THREE-BODY PROBLEM UNDER AN OBLATE PRIMARY, A TRIAXIAL SECONDARY AND A …

J Singh, RK Tyokyaa - 2022 - researchgate.net
We have examined the effects of Albedo in the elliptic restricted three-body problem under
an oblate primary, a triaxial secondary and a potential due to belt for the Earth-Moon system …