Abstract
The elliptic restricted three-body problem is used to investigate the motion behavior of the smallest body (test particle), where the primaries move in elliptical orbits around their common center of mass. Here the primary is taken as a radiating oblate body and the secondary is considered as a dipole, while the third smallest body is varying its mass according to the Jeans law. Under these assumptions we determine the equations of motion and the quasi-Jacobian integral for the test particle which is moving in space under the gravitational forces of the primaries. The locations of stationary points and their stability states are determined and then, after regions of motion, Poincaré surfaces of section and basins of attraction are illustrated.
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ACKNOWLEDGMENTS
The authors are thankful to the editor and reviewer both for giving us opportunity to improve our paper up to the present form.
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We are thankful to The Deanship of scientific research, Majmaah University, KSA.
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Albidah, A.B., Ansari, A.A. Shapes and Mass Variation Effects of the Bodies in the Generalized Elliptic Restricted 3-Body Problem. Astron. Rep. 67, 393–403 (2023). https://doi.org/10.1134/S1063772923040017
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DOI: https://doi.org/10.1134/S1063772923040017