Partially rigid motions in the n-body problem
Richard Moeckel

TL;DR
This paper investigates the existence of partially rigid motions in the n-body problem, specifically proving that hinged solutions do not exist for n=3 or 4, regardless of the space dimension.
Contribution
It establishes the non-existence of hinged solutions in the 3- and 4-body problems, extending understanding of rigid motion constraints.
Findings
Hinged solutions do not exist for n=3.
Hinged solutions do not exist for n=4.
Results are independent of ambient space dimension.
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. In particular, a {\em hinged} solution is one such that exactly one mutual distance varies. The goal of this paper is to show that hinged solutions don't exist when n=3 or n=4. For n=3 this means that if 2 of the 3 distances are constant so is the third and for n=4, if 5 of the 6 distances are constant, so is the sixth. These results hold independent of the dimension d of the ambient space.
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Taxonomy
TopicsAstro and Planetary Science · Spacecraft Dynamics and Control · Space Satellite Systems and Control
