Abstract
We show by a general argument that periodic solutions of the planar problem of three bodies (with given masses) form one-parameter families. This result is confirmed by numerical investigations: two orbits found earlier by Standish and Szebehely are shown to belong to continuous one-parameter families of periodic orbits. In general these orbits have a non-zero angular momentum, and the configuration after one period is rotated with respect to the initial configuration. Similar general arguments whow that in the three-dimensional problem, periodic orbits form also one-parameter families; in the one-dimensional problem, periodic orbits are isolated.
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Hénon, M. Families of periodic orbits in the three-body problem. Celestial Mechanics 10, 375–388 (1974). https://doi.org/10.1007/BF01586865
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DOI: https://doi.org/10.1007/BF01586865