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Libration Points in the R3BP with a Triaxial Rigid Body as the Smaller Primary and a Variable Mass Infinitesimal Bod
Department of Mathematics, S. M. College, T. M. Bhagalpur University, Bhagalpur, India
T. M. Bhagalpur University, Bhagalpur, India
Department of Mathematics, P. G. Campus, Tribhuvan University, Biratnagar, Nepal
GTE, Bangalore, India
- 1 Department of Mathematics, S. M. College, T. M. Bhagalpur University, Bhagalpur, India
- 2 T. M. Bhagalpur University, Bhagalpur, India
- 3 Department of Mathematics, P. G. Campus, Tribhuvan University, Biratnagar, Nepal
- 4 GTE, Bangalore, India
International Journal of Astronomy and Astrophysics·Volume 09 (2019)·Pages 21–38·Published 23 January 2019·DOI10.4236/ijaa.2019.91003
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Abstract
The paper deals with the existence of the coplanar libration points in the restricted three-body problem when the smaller primary is a triaxial rigid body and the infinitesimal body is of variable mass. Following small parameter method, the coordinates of collinear libration points are established whereas the coordinates of triangular libration points are established by classical method. It is found that the mass reduction factor has small effect but triaxiality parameters of the smaller primary have great effects on the coordinates of the libration points.
KeywordsRestricted Three-Body ProblemJean’s LawSpace-Time TransformationTriaxialityMass Reduction FactorsLibration Points
- Jeans, J.H. (1928) Astronomy & Cosmogomy. Cambridge University Press, Cambridge.
- Meshcherskii, L.V. (1949) Studies on the Mechanics of Bodies of Variable Mass. Gostekhizdat, Moscow.
- Shrivastava, A.K. and Ishwar, B. (1983) Equations of Motion of the Restricted Three-Body Problem with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 30, 323-328. https://doi.org/10.1007/BF01232197
- Singh, J. and Ishwar, B. (1985) Effect of Perturbations on the Stability of Triangular Points in the Restricted Three-Body Problem with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 35, 201-207. https://doi.org/10.1007/BF01227652
- Das, R.K., Shrivastav, A.K. and Ishwar, B. (1988) Equations of Motion of Elliptic Restricted Three-Body Problem with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 45, 387-393. https://doi.org/10.1007/BF01245759
- Lukyanov, L.G. (1990) The Stability of the Libration Points in the Restricted Three-Body Problem with Variable Mass. Astronomical Journal, 67, 167-172.
- El-Shaboury, S.M. (1990) Equations of Motion of Elliptically-Restricted Problem of a Body with Variable Mass and Two Triaxial Bodies. Astrophysics and Space Science, 174, 291-296. https://doi.org/10.1007/BF00642513
- Singh, J. (2008) Non-Linear Stability of Libration Points in the Restricted Three-Body Problem with Variable Mass. Astrophysics and Space Science, 314, 281-289. https://doi.org/10.1007/s10509-008-9768-9
- Hassan, M.R., Kumari, S. and Hassan, M.A. (2017) Existence of Libration Points in the R3BP with Variable Mass when the Smaller Is an Oblate Spheroid. International Journal of Astronomy and Astrophysics, 7, 45-61. https://doi.org/10.4236/ijaa.2017.72005
- Volosov, V.M. (1972) Introductory Mathematics for Engineers. Mir Publishers, Moscow.
- Szebehely, V. (1967) Theory of Orbits—The Restricted Problem of Three Bodies. Academic Press, New York and London.