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 |
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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. |
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ISSN: | 0004-640X 1572-946X |
DOI: | 10.1007/s10509-015-2275-x |