Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid

The Sitnikov's problem is a special case of restricted three body problem if the primaries are of equal masses (m1 = m2 = 1/2) moving in circular orbits under Newtonian force of attraction and the third body of mass m3 moves along the line perpendicular to plane of motion of primaries. Here ob...

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Main Author: RR Thapa
Format: Article
Language:English
Published: Department of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan University 2014-05-01
Series:Bibechana
Subjects:
Online Access:https://www.nepjol.info/index.php/BIBECHANA/article/view/10395
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author RR Thapa
author_facet RR Thapa
author_sort RR Thapa
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description The Sitnikov's problem is a special case of restricted three body problem if the primaries are of equal masses (m1 = m2 = 1/2) moving in circular orbits under Newtonian force of attraction and the third body of mass m3 moves along the line perpendicular to plane of motion of primaries. Here oblate spheroid primaries are taken. The solution of the Sitnikov's circular restricted three body problem has been checked when the primaries are oblate spheroid. We observed that solution is depended on oblate parameter A of the primaries and independent variable τ = ηt. For this the stability of non-trivial solutions with the characteristic equation is studied. The general equation of motion of the infinitesimal mass under mutual gravitational field of two oblate primaries are seen at equilibrium points. Then the stability of infinitesimal third body m3 has been calculated. DOI: http://dx.doi.org/10.3126/bibechana.v11i0.10395 BIBECHANA 11(1) (2014) 149-156
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spelling doaj.art-b9da9d4f4f2d446980370fd4660c67d42024-04-23T13:05:41ZengDepartment of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan UniversityBibechana2091-07622382-53402014-05-011110.3126/bibechana.v11i0.10395Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroidRR Thapa0Department of Mathematics, Post Graduate Campus, Biratnagar Tribhuvan University The Sitnikov's problem is a special case of restricted three body problem if the primaries are of equal masses (m1 = m2 = 1/2) moving in circular orbits under Newtonian force of attraction and the third body of mass m3 moves along the line perpendicular to plane of motion of primaries. Here oblate spheroid primaries are taken. The solution of the Sitnikov's circular restricted three body problem has been checked when the primaries are oblate spheroid. We observed that solution is depended on oblate parameter A of the primaries and independent variable τ = ηt. For this the stability of non-trivial solutions with the characteristic equation is studied. The general equation of motion of the infinitesimal mass under mutual gravitational field of two oblate primaries are seen at equilibrium points. Then the stability of infinitesimal third body m3 has been calculated. DOI: http://dx.doi.org/10.3126/bibechana.v11i0.10395 BIBECHANA 11(1) (2014) 149-156 https://www.nepjol.info/index.php/BIBECHANA/article/view/10395Characteristic equationNon-trivial solutionOblate spheroidSitnikov's restricted three body problemStability
spellingShingle RR Thapa
Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid
Bibechana
Characteristic equation
Non-trivial solution
Oblate spheroid
Sitnikov's restricted three body problem
Stability
title Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid
title_full Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid
title_fullStr Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid
title_full_unstemmed Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid
title_short Stability of the Sitnikov's circular restricted three body problem when the primaries are oblate spheroid
title_sort stability of the sitnikov s circular restricted three body problem when the primaries are oblate spheroid
topic Characteristic equation
Non-trivial solution
Oblate spheroid
Sitnikov's restricted three body problem
Stability
url https://www.nepjol.info/index.php/BIBECHANA/article/view/10395
work_keys_str_mv AT rrthapa stabilityofthesitnikovscircularrestrictedthreebodyproblemwhentheprimariesareoblatespheroid