Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem

The oblateness and the photogravitational effects of both the primaries on the location and the stability of the triangular equilibrium points in the elliptical restricted three-body problem have been discussed. The stability of the triangular points under the photogravitational and oblateness effe...

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Main Authors: A. Narayan, Amit Shrivastava
Format: Article
Language:English
Published: Wiley 2013-01-01
Series:Journal of Mathematics
Online Access:http://dx.doi.org/10.1155/2013/936859
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author A. Narayan
Amit Shrivastava
author_facet A. Narayan
Amit Shrivastava
author_sort A. Narayan
collection DOAJ
description The oblateness and the photogravitational effects of both the primaries on the location and the stability of the triangular equilibrium points in the elliptical restricted three-body problem have been discussed. The stability of the triangular points under the photogravitational and oblateness effects of both the primaries around the binary systems Achird, Lyeten, Alpha Cen-AB, Kruger 60, and Xi-Bootis, has been studied using simulation techniques by drawing different curves of zero velocity.
format Article
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institution Kabale University
issn 2314-4629
2314-4785
language English
publishDate 2013-01-01
publisher Wiley
record_format Article
series Journal of Mathematics
spelling doaj-art-121cb050364e4a84bbae2e748091b5752025-02-03T07:25:19ZengWileyJournal of Mathematics2314-46292314-47852013-01-01201310.1155/2013/936859936859Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body ProblemA. Narayan0Amit Shrivastava1Department of Mathematics, Bhilai Institute of Technology, Durg 491001, IndiaDepartment of Mathematics, Rungta College of Engineering and Technology, Bhilai 490020, IndiaThe oblateness and the photogravitational effects of both the primaries on the location and the stability of the triangular equilibrium points in the elliptical restricted three-body problem have been discussed. The stability of the triangular points under the photogravitational and oblateness effects of both the primaries around the binary systems Achird, Lyeten, Alpha Cen-AB, Kruger 60, and Xi-Bootis, has been studied using simulation techniques by drawing different curves of zero velocity.http://dx.doi.org/10.1155/2013/936859
spellingShingle A. Narayan
Amit Shrivastava
Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem
Journal of Mathematics
title Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem
title_full Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem
title_fullStr Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem
title_full_unstemmed Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem
title_short Pulsating Different Curves of Zero Velocity around Triangular Equilibrium Points in Elliptical Restricted Three-Body Problem
title_sort pulsating different curves of zero velocity around triangular equilibrium points in elliptical restricted three body problem
url http://dx.doi.org/10.1155/2013/936859
work_keys_str_mv AT anarayan pulsatingdifferentcurvesofzerovelocityaroundtriangularequilibriumpointsinellipticalrestrictedthreebodyproblem
AT amitshrivastava pulsatingdifferentcurvesofzerovelocityaroundtriangularequilibriumpointsinellipticalrestrictedthreebodyproblem