全部 标题 作者
关键词 摘要

OALib Journal期刊
ISSN: 2333-9721
费用:99美元

查看量下载量

相关文章

更多...

Existence of Equilibrium Points in the R3BP with Variable Mass When the Smaller Primary is an Oblate Spheroid

DOI: 10.4236/ijaa.2017.72005, PP. 45-61

Keywords: Restricted Three-Body Problem, Jean’s Law, Space-Time Transformation, Oblateness, Equilibrium Points, Surface of Zero-Velocity

Full-Text   Cite this paper   Add to My Lib

Abstract:

The paper deals with the existence of equilibrium points in the restricted three-body problem when the smaller primary is an oblate spheroid and the infinitesimal body is of variable mass. Following the method of small parameters; the co-ordinates of collinear equilibrium points have been calculated, whereas the co-ordinates of triangular equilibrium points are established by classical method. On studying the surface of zero-velocity curves, it is found that the mass reduction factor has very minor effect on the location of the equilibrium points; whereas the oblateness parameter of the smaller primary has a significant role on the existence of equilibrium points.

References

[1]  Jeans, J.H. (1928) Astronomy and Cosmogony. Cambridge University Press, Cambridge.
[2]  Meshcherskii, L.V. (1949) Studies on the Mechanics of Bodies of Variable Mass, Gostekhizdat, Moscow.
[3]  Omarov, T.B. (1963) The Restricted Problem of Perturbed Motion of Two Bodies with Variable Mass. Soviet Astronomy, 8, 127.
[4]  Verhulst, F. (1972) Two-Body Problem with Slowly Decreasing Mass. Celestial Mechanics and Dynamical Astronomy, 5, 27-36.
https://doi.org/10.1007/bf01227820
[5]  Das, R.K., Shrivastav, A.K. and Ishwar, B. (1988) Equations of Motion of Elliptic Restricted Problem of Three Bodies with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 45, 387-393.
https://doi.org/10.1007/BF01245759
[6]  Shrivastava, A.K. and Ishwar, B. (1983) Equations of Motion of the Restricted Problem of Three Bodies with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 30, 323-328.
ttps://doi.org/10.1007/BF01232197
[7]  Lukyanov, L.G. (1990) The Stability of the Libration Points in the Restricted Three-Body Problem with Variable Mass. Astronomical Journal, 67, 167-172.
[8]  El-Shaboury, S.M. (1990) Equations of Motion of Elliptically-Restricted Problem of a Body with Variable Mass and Two Tri-Axial Bodies. Astrophysics and Space Science, 174, 291-296.
https://doi.org/10.1007/BF00642513
[9]  Plastino, A.R. and Muzzio, J.C. (1992) On the Use of and Abuse of Newton’s Second Law for Variable Mass Problems. Celestial Mechanics and Dynamical Astronomy, 53, 227-232.
https://doi.org/10.1007/BF00052611
[10]  Bekov, A.A. (1993) The Libration Points and Hill Surfaces in the Restricted Problem of Three Variable Mass Bodies. Proceedings of the International Astronomical Union Colloquium 132, New Delhi, 10-13 October 1993, 277-288.
https://doi.org/10.1017/S0252921100066173
[11]  Bekov, A.A. (1993) Problem of Physics of Stars and Extragalactic Astronomy. 91-114.
[12]  Singh, J. and Ishwar, B. (1985) Effect of Perturbations on the Stability of Triangular Points in the Restricted Problem of Three Bodies with Variable Mass. Celestial Mechanics and Dynamical Astronomy, 35, 201-207.
https://doi.org/10.1007/bf01227652

Full-Text

Contact Us

service@oalib.com

QQ:3279437679

WhatsApp +8615387084133