Series solutions of the Sitnikov restricted N+1-body problem: elliptic case

Following Giacaglia ( 1967 ), in Sect.  2 we have developed equation of motion of the Sitnikov restricted N +1-body problem in elliptic case. We assumed that the primaries are at the vertices of a regular N -gon so the distances of the primaries from center of mass are time depending. In Sect.  3 we...

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Veröffentlicht in:Astrophysics and space science 2015-06, Vol.357 (2), p.1-9, Article 166
Hauptverfasser: Shahbaz Ullah, M., Majda, B., Ullah, M. Zafar, Shahnawaz Ullah, M.
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Sprache:eng
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Zusammenfassung:Following Giacaglia ( 1967 ), in Sect.  2 we have developed equation of motion of the Sitnikov restricted N +1-body problem in elliptic case. We assumed that the primaries are at the vertices of a regular N -gon so the distances of the primaries from center of mass are time depending. In Sect.  3 we have linearized the equation of motion to obtain the Hill’s type equation and then find the approximate solution. In Sects.  4 and  5 the series solutions of the Sitnikov restricted N +1-body problem have been developed by the method of Lindstedt-Poincaré and iteration of Green’s function respectively. In Sect.  6 the two series solutions have been compared graphically by putting N =2, 3 and 4 for different eccentricity.
ISSN:0004-640X
1572-946X
DOI:10.1007/s10509-015-2275-x