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...

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Hlavní autor:	RR Thapa
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	Department of Physics, Mahendra Morang Adarsh Multiple Campus, Tribhuvan University 2014-05-01
Edice:	Bibechana
Témata:	Characteristic equation Non-trivial solution Oblate spheroid Sitnikov's restricted three body problem Stability
On-line přístup:	https://nepjol.info/index.php/BIBECHANA/article/view/10395
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