Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..55..369c&link_type=abstract
Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 55, no. 4, p. 369-386.
Astronomy and Astrophysics
Astronomy
Eccentricity, Gravitational Fields, Many Body Problem, Orbits, Angular Momentum, Perturbation, Two Body Problem
Scientific paper
For N = 2 of the N-body problem, two families of symmetries S1 and S2 are defined which change the eccentricity of a solution. S1 is associated with arbitrary choice of the zero level of the potential while S2 is related to a possible affinity of the configuration space. S1 and S2 are described by a spatial transformation product of an instantaneous homothethy and an instantaneous rotation completed by a change of the temporal variable. S1 may related unbounded and bounded central solutions of the same type, and S2 may regularize multiple collisions among central solutions of the same type. Thus any central solution is equivalent to a central circular solution of the same type. This is a form of regularization.
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