More than six hundreds new families of Newtonian periodic planar collisionless three-body orbits
Xiaoming Li, Shijun Liao

TL;DR
This paper numerically discovers over 600 new families of Newtonian periodic three-body orbits with equal masses and zero angular momentum, significantly expanding the known solutions and suggesting a quasi Kepler's third law.
Contribution
The authors numerically identify more than 600 new families of periodic three-body orbits, vastly increasing the known solutions in this classical problem.
Findings
Discovered 695 families of periodic orbits, including known and new ones.
Proposed a quasi Kepler's third law for these orbits.
Provided visualizations and online resources for the orbits.
Abstract
The famous three-body problem can be traced back to Isaac Newton in 1680s. In the 300 years since this "three-body problem" was first recognized, only three families of periodic solutions had been found, until 2013 when \v{S}uvakov and Dmitra\v{s}inovi\'c [Phys. Rev. Lett. 110, 114301 (2013)] made a breakthrough to numerically find 13 new distinct periodic orbits, which belong to 11 new families of Newtonian planar three-body problem with equal mass and zero angular momentum. In this paper, we numerically obtain 695 families of Newtonian periodic planar collisionless orbits of three-body system with equal mass and zero angular momentum in case of initial conditions with isosceles collinear configuration, including the well-known Figure-eight family found by Moore in 1993, the 11 families found by \v{S}uvakov and Dmitra\v{s}inovi\'c in 2013, and more than 600 new families that have been…
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