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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 oblate...

Ausführliche Beschreibung

Gespeichert in:
1. Verfasser: RR Thapa
Format: Artigo
Sprache:Inglês
Veröffentlicht: Department of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan University 2014-05-01
Schriftenreihe:Bibechana
Schlagworte:
Characteristic equation
Non-trivial solution
Oblate spheroid
Sitnikov's restricted three body problem
Stability
Online-Zugang:https://nepjol.info/index.php/BIBECHANA/article/view/10395
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