On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary

We consider a version of the relativistic restricted three-body problem (R3BP) which includes the effects of oblateness of the secondary and radiation of the primary. We determine the positions and analyze the stability of the triangular points. We find that these positions are affected by relativis...

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Main Authors: Nakone Bello, Jagadish Singh
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2015/489120
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author Nakone Bello
Jagadish Singh
author_facet Nakone Bello
Jagadish Singh
author_sort Nakone Bello
collection DOAJ
description We consider a version of the relativistic restricted three-body problem (R3BP) which includes the effects of oblateness of the secondary and radiation of the primary. We determine the positions and analyze the stability of the triangular points. We find that these positions are affected by relativistic, oblateness, and radiation factors. It is also seen that both oblateness of the secondary and radiation of the primary reduce the size of stability region. Further, a numerical exploration computing the positions of the triangular points and the critical mass ratio of some binaries systems consisting of the Sun and its planets is given in the tables.
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institution Kabale University
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spelling doaj-art-e481b2b3c6d3493ea34c1ed062d1cf252025-02-03T01:02:33ZengWileyAdvances in Astronomy1687-79691687-79772015-01-01201510.1155/2015/489120489120On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating PrimaryNakone Bello0Jagadish Singh1Department of Mathematics, Faculty of Science, Usmanu Danfodiyo University, PMB 2346, Sokoto, NigeriaDepartment of Mathematics, Faculty of Science, Ahmadu Bello University, PMB 1044, Zaria, Kaduna State, NigeriaWe consider a version of the relativistic restricted three-body problem (R3BP) which includes the effects of oblateness of the secondary and radiation of the primary. We determine the positions and analyze the stability of the triangular points. We find that these positions are affected by relativistic, oblateness, and radiation factors. It is also seen that both oblateness of the secondary and radiation of the primary reduce the size of stability region. Further, a numerical exploration computing the positions of the triangular points and the critical mass ratio of some binaries systems consisting of the Sun and its planets is given in the tables.http://dx.doi.org/10.1155/2015/489120
spellingShingle Nakone Bello
Jagadish Singh
On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary
Advances in Astronomy
title On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary
title_full On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary
title_fullStr On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary
title_full_unstemmed On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary
title_short On the Stability of L4,5 in the Relativistic R3BP with Oblate Secondary and Radiating Primary
title_sort on the stability of l4 5 in the relativistic r3bp with oblate secondary and radiating primary
url http://dx.doi.org/10.1155/2015/489120
work_keys_str_mv AT nakonebello onthestabilityofl45intherelativisticr3bpwithoblatesecondaryandradiatingprimary
AT jagadishsingh onthestabilityofl45intherelativisticr3bpwithoblatesecondaryandradiatingprimary