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

Author:

Bouaziz-Kellil Ferdaous1ORCID

Affiliation:

1. Department of Mathematics, College of Science and Arts, Qassim University, Buraydah, Saudi Arabia

Abstract

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 primaries). It is assumed that the massive bodies have radiating effects, have oblate shapes, and are moving in circular orbits around their common center of mass. Using the procedures established by Singh and Abouelmagd, we determined the equations of motion of the infinitesimal body for which we assumed that under the effects of radiation and oblateness of the primaries, its mass varies following Jean’s law. We evaluated analytically and numerically the locations of equilibrium points and examined the stability of these equilibrium points. Finally, we found that all the points are unstable.

Funder

Qassim University

Publisher

Hindawi Limited

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

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2. Existence and stability of libration points in the restricted three-body problem when the smaller primary is a triaxial rigid body and the bigger one an oblate spheroid;M. Khanna;Indian Journal of Pure and Applied Mathematics (IJPAM),1999

3. Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid

4. A note on the stability of the triangular points of the equilibrium in the restricted three-body problem;P. V. Subba Rao;Astronomy and Astrophysics,1975

5. The effect of oblateness in the perturbed restricted three-body problem

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