NASA NTRS · 19780038968
Stabilization of Kepler's problem
Abstract
A regularization of Kepler's problem due to Moser (1970) is used to stabilize the equations of motion. In other words, a particular solution of Kepler's problem is imbedded in a Liapunov stable system. Perturbations can be introduced into the stabilized equations.
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Stokes, A.. 1977-09-01. Stabilization of Kepler's problem. https://ntrs.nasa.gov/citations/19780038968
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