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

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Let Γ∗(s)\Gamma^{\ast}(s), s≥0s\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), s≥0s\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.

References

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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