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Stability of planetary orbits in binary systemsThe possible existence of stable orbits is investigated in binary systems using Hill's method. Analytical stability conditions are established for satellites, for inner planets and for outer planets, allowing arbitrary values for the mass-ratio of the binary.
Document ID
19800060772
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Szebehely, V. (Texas, University Austin, Tex., United States)
Date Acquired
August 10, 2013
Publication Date
July 1, 1980
Subject Category
Astronomy
Accession Number
80A44942
Distribution Limits
Public
Copyright
Other

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