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Stabilization of Kepler's problemA 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.
Document ID
19780038968
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1007/BF01235725
Authors
Stokes, A. (NASA Goddard Space Flight Center Greenbelt, Md.; Georgetown University, Washington, D.C., United States)
Date Acquired
August 9, 2013
Publication Date
September 1, 1977
Publication Information
Publication: Celestial Mechanics
Volume: 16
Subject Category
Astronomy
Accession Number
78A22877
Distribution Limits
Public
Copyright
Other

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