Abstract
We use a slightly modified version of McGehee's transformation to study the triple collisions of the isosceles three body problem in a way that allows us to let the mass ratio go to zero. We study the limiting case and show that the collision manifold changes topologically, which affects the behaviour of near collision orbits. We also obtain new information about the flow on the collision manifold when the mass ratio is small.
Similar content being viewed by others
References
R Devaney,Collision orbits in the anisotropic Kepler problem, Inventiones math.45, 221–251 (1978).
R. Devaney,Triple collision in the planar isosceles three body problem. Inventiones math.60, 249–267 (1980).
R. Devaney,Blowing up singularities in classical mechanical systems. American Math. Monthly,89, 8 (1982).
R. McGehee,Triple collision in the collinear three-body problem. Inventiones math.27, 191–227 (1974).
R. Moeckel,Orbits near triple collision in the three-body problem. Indiana Univ. Math. J.32, 2 (1983).
R. Moeckel,Heteroclinic phenomena in the isosceles three-body problem. SIAM J. Math. Anal.15, 5 (1984).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
ElBialy, M.S. Triple collisions in the isosceles three body problem with small mass ratio. Journal of Applied Mathematics and Physics (ZAMP) 40, 645–664 (1989). https://doi.org/10.1007/BF00945869
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00945869