Abstract
We study a Poincaré map in the planar isosceles three-body problem, but we emphasize the mapping of areas in phase space over few iterations rather than single points over many iterations. This map, with a complementary symbol ic dynamics, l ea ds to global information. We identify a s table fixed poi nt of the mapping wi t h associat ed qu asi- perio dic motionion for sm alle r massss ratios. The invariant KAM region around this fixed point vanishes at an inverse period doubling bifurcation at m 3/m 1 ≅ 2.581. We also find a set on which a horseshoe map completely describes the motion. This simply chaotic set is destroyed at mass ratio m 3/m 1 ≅ 2.662 leading to an interesting global bifurcation. Ranges of the mass ratio are identified on which the dynamics is qualitatively similar in a global sense. We also study the motion at the limiting values of the mass ratio.
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© 1999 Springer Science+Business Media Dordrecht
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Chesley, S., Zare, K. (1999). Bifurcations in the Mass Ratio of the Planar Isosceles Three-Body Problem. In: Steves, B.A., Roy, A.E. (eds) The Dynamics of Small Bodies in the Solar System. NATO ASI Series, vol 522. Springer, Dordrecht. https://doi.org/10.1007/978-94-015-9221-5_42
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DOI: https://doi.org/10.1007/978-94-015-9221-5_42
Publisher Name: Springer, Dordrecht
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