Abstract
This paper investigates the motion of a test particle around the out-of-plane equilibrium points in the circular photogravitational restricted three-body problem when the effect of radiation pressure from the smaller primary and its Poynting-Robertson (P-R) drag are taken into account, and the bigger primary is modeled as an oblate spheroid. These points lie in the xz-plane almost directly above and below the center of the oblate primary. The equilibrium points are sought, and we observe that, there are two coordinate points L 6,7 which depend on the oblateness of the bigger primary, and the radiation pressure force and P-R drag of the smaller primary. The positions and linear stability of the problem are investigated both analytically and numerically for the binary system Cen X-4. The out-of-plane equilibrium points are found to be unstable in the sense of Lyapunov due to the presence of a positive real root.
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Singh, J., Amuda, T.O. Out-of-Plane Equilibrium Points in the Photogravitational CR3BP with Oblateness and P-R Drag. J Astrophys Astron 36, 291–305 (2015). https://doi.org/10.1007/s12036-015-9336-y
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DOI: https://doi.org/10.1007/s12036-015-9336-y