Minimum energy configurations in Celestial Mechanics are investigated. It is shown that this is not a well defined problem for point-mass celestial mechanics but well-posed for finite density distributions. This naturally leads to a granular mechanics extension of usual Celestial Mechanics questions such as relative equilibria and stability. This paper specifically studies and finds all relative equilibria and minimum energy configurations for N = 1, 2, 3 and develops hypotheses on the relative equilibria and minimum energy configurations for N ≫ 1 bodies. © 2012 Springer Science+Business Media B.V.
CITATION STYLE
Scheeres, D. J. (2012). Minimum energy configurations in the N-body problem and the celestial mechanics of granular systems. Celestial Mechanics and Dynamical Astronomy, 113(3), 291–320. https://doi.org/10.1007/s10569-012-9416-0
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