Partially rigid motions in the planar three-body problem
Richard Moeckel

TL;DR
This paper investigates partially rigid motions in the planar three-body problem and proves that such motions cannot exist unless they are fully rigid, i.e., relative equilibria.
Contribution
It establishes that in the planar three-body problem with equal masses, partial rigidity implies full rigidity, ruling out partially rigid motions.
Findings
Partially rigid motions are impossible in the planar three-body problem with equal masses.
Any motion with even one constant mutual distance must be a relative equilibrium.
The result constrains the types of motions possible in this classical problem.
Abstract
A solution of the n-body problem in R^d is a relative equilibrium if all of the mutual distance between the bodies are constant. In other words, the bodies undergo a rigid motion. Here we investigate the possibility of partially rigid motions, where some but not all of the distances are constant. For the planar three-body problem with equal masses, we show that partially rigid motions are impossible -- if even one of the three mutual distances is constant, the motion must be a relative equilibrium.
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Taxonomy
TopicsSpacecraft Dynamics and Control · Astro and Planetary Science · Space Satellite Systems and Control
