Mathematics
Scientific paper
Aug 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976cemec..14...73z&link_type=abstract
(Conference on Mathematical Methods in Celestial Mechanics, 5th, Oberwolfach, West Germany, Aug. 24-30, 1975.) Celestial Mechani
Mathematics
38
Celestial Mechanics, Equations Of Motion, Hamiltonian Functions, Manifolds (Mathematics), Three Body Problem, Angular Momentum, Canonical Forms, Measure And Integration, Momentum, Time Dependence
Scientific paper
Regions of possible motions are established for dynamical systems possessing time-independent Hamiltonians or for systems which are reducible to that form by means of integrals of the motion using only extended point transformations. The method is applied to the problem of three bodies in a plane and surfaces of zero velocity are found. The governing parameters are the energy, angular momentum and the masses of the participating bodies. The analytical and geometrical properties of these surfaces proved qualitative results for given constants of the motion.
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