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Solution of the N-body problem with recurrent power series.Adaptation of Steffensen's method of solution of both the restricted and general three-body problems in terms of power series in time to the solution of the equations of motion of N planets around the sun. The key feature of this adaptation lies in the introduction of N new variables and in the use of new relations which contain the time derivatives and can thus be treated as differential equations.
Document ID
19720026348
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Broucke, R.
(California, University Los Angeles; California Institute of Technology, Jet Propulsion Laboratory, Pasadena, Calif., United States)
Date Acquired
August 6, 2013
Publication Date
September 1, 1971
Publication Information
Publication: Celestial Mechanics
Volume: 4
Subject Category
Space Sciences
Accession Number
72A10014
Distribution Limits
Public
Copyright
Other

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