Stabilization of Kepler's Problem
Abstract
A regularization of Kepler's problem due to Moser is used to ‘stabilize’ the equations of motion, that is, imbed a particular solution of Kepler's problem in a Lyapounov stable system.
 Publication:

Celestial Mechanics
 Pub Date:
 September 1977
 DOI:
 10.1007/BF01235725
 Bibcode:
 1977CeMec..16...27S
 Keywords:

 Kepler Laws;
 Liapunov Functions;
 Numerical Stability;
 Orbit Perturbation;
 Perturbation Theory;
 Canonical Forms;
 Hamiltonian Functions;
 Manifolds (Mathematics);
 Astronomy