Libration Points in Schwarzschild's Circular Restricted Three-Body Problem
The restricted three-body problem in Schwarzschild's gravitational field is analyzed. The existen- ce of the equilibrium points in the orbital plane is discussed and the corresponding positions are established. There are three collinear libration points, and, if they exist, two triangular libra...
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| Veröffentlicht in: | Astrophysics and space science 2006-08, Vol.304 (1-4), p.101-103 |
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| creator | Rodica, Roman Vasile, Mioc |
| description | The restricted three-body problem in Schwarzschild's gravitational field is analyzed. The existen- ce of the equilibrium points in the orbital plane is discussed and the corresponding positions are established. There are three collinear libration points, and, if they exist, two triangular libration points (situated in the orbital plane of the primaries). If triangular points exist, they may not form equilateral triangles; the triangles are isosceles for equal masses of the primaries, and scalene else. |
| doi_str_mv | 10.1007/s10509-006-9083-2 |
| format | Article |
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| language | eng |
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| source | SpringerNature Journals |
| subjects | Astronomy Astrophysics |
| title | Libration Points in Schwarzschild's Circular Restricted Three-Body Problem |
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