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

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 orbi...

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Main Author: Ferdaous Bouaziz-Kellil
Format: Article
Language:English
Published: Wiley 2020-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2020/6684728
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author Ferdaous Bouaziz-Kellil
author_facet Ferdaous Bouaziz-Kellil
author_sort Ferdaous Bouaziz-Kellil
collection DOAJ
description 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.
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spelling doaj-art-7ca9c438794f45b78d1c644e3cc979342025-02-03T01:03:57ZengWileyAdvances in Astronomy1687-79691687-79772020-01-01202010.1155/2020/66847286684728Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids BeltFerdaous Bouaziz-Kellil0Department of Mathematics, College of Science and Arts, Qassim University, Buraydah, Saudi ArabiaThe 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.http://dx.doi.org/10.1155/2020/6684728
spellingShingle Ferdaous Bouaziz-Kellil
Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt
Advances in Astronomy
title Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt
title_full Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt
title_fullStr Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt
title_full_unstemmed Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt
title_short Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt
title_sort motion of the infinitesimal variable mass in the generalized circular restricted three body problem under the effect of asteroids belt
url http://dx.doi.org/10.1155/2020/6684728
work_keys_str_mv AT ferdaousbouazizkellil motionoftheinfinitesimalvariablemassinthegeneralizedcircularrestrictedthreebodyproblemundertheeffectofasteroidsbelt