Abstract
We prove that any fixed configuration of N-1 masses in space with no three points collinear and no four points cocircular can be extended to a central configuration of N masses by adding a specified additional mass only in finitely many ways. This holds for a family of potential functions including the Newtonian gravitational case.
Original language | English (US) |
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Pages (from-to) | 610-622 |
Number of pages | 13 |
Journal | SIAM Journal on Applied Algebra and Geometry |
Volume | 7 |
Issue number | 3 |
DOIs | |
State | Published - 2023 |
Bibliographical note
Publisher Copyright:Copyright © 2023 Authors.
Keywords
- celestial mechanics
- central configurations
- n-body problem