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Equal-mass choreography
Periodic solutionLinearly stable
Figure-eight orbit
Orbit: three equal masses chase one another around the same horizontal figure-eight curve.
Status: linearly stable in the Hamiltonian, non-dissipative sense. Perturbations need not decay, but they do not immediately grow exponentially.
Source: classic Chenciner-Montgomery planar solution.
Thin dashed paths are numerical reference traces from the orbit's initial conditions.
Integrator
t = 0.00
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