The conjecture on triple-collision shape curves and their first eclipses

Let Γ(s)\Gamma^{\ast}(s), s0s\geq 0, denote a triple-collision shape curve, and let the equator circle be the locus representing the first eclipse. Triple-collision shape-curve conjecture. The different triple-collision shape curves Γ(s)\Gamma^{\ast}(s), s0s\geq 0, intersect the equator circle for the first time at different points; moreover, each point on the circle is reached by a unique curve. The curves do not intersect one another, except possibly after the first eclipse. This is proposed as an open problem because a stronger version of the surrounding geometric theorem appears close, but its proof requires further elaboration.

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Primary source

W. Y. Hsiang and E. Straume, “Kinematic geometry of triangles and the study of the three-body problem”, arXiv:math-ph/0608060 (2006).

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