Abstract
Possibility of exchange is discussed for a rectilinear three-body system with zero energy. By introducing some reguralized coordinates which relate to McGehee s ones and using a separability of the reguralized coordinates in the equations of motion, we can get a boundary manifold T2 which describes the motion of configuration of the system. The fixed points of the flow on T2 correspond to parabolic escape, hyperbolic-elliptic escape and triple collision. By using the correspondence between an orbit and an evolution of the system and introducing a concept of “Critical System”, we can obtain a result that all of HE--HE+ orbit are exchange type in critical system whose orbits of parabolic-parabolic escape type experience odd times of binary collision and no exchange occurs in critical systems whose orbits of parabolic-parabolic escape type experience even times of binary collision. Moreover, in non-critical system, we can find the both orbits of exchange type and non-exchange type.
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References
Chazy, J.: 1932, ‘Sur l’allure final du movement dans le problème des trios corps.’ Bull. Astronom. 8, 403–436.
Lacomba, E. A. and Simó, C.: 1982, ‘Boundary manifolds for energy surfaces in celestial mechanics.’ celest. Mech. 28, 37–48.
McGehee, R.: 1974, ‘Triple collision in the collinear three-body problem.’ Inventions Math. 27, 191–227.
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© 1988 Kluwer Academic Publishers
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Koda, E. (1988). Possibility of Exchange of a Rectilinear Three-Body System with Zero Energy. In: Valtonen, M.J. (eds) The Few Body Problem. Astrophysics and Space Science Library, vol 140. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2917-3_10
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DOI: https://doi.org/10.1007/978-94-009-2917-3_10
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7813-9
Online ISBN: 978-94-009-2917-3
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