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Non-linear stability around the triangular libration pointsThe configuration space around the triangular libration points in the Earth-Moon system is partitioned according to the stability of the motion. The regions around L4 and L5 are established where particles placed with zero initial velocity will librate. The complexity of the partitioning is revealed.
Document ID
19810044223
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Mckenzie, R.
(Texas Univ. Austin, TX, United States)
Szebehely, V.
(Texas, University Austin, Tex., United States)
Date Acquired
August 11, 2013
Publication Date
March 1, 1981
Publication Information
Publication: Celestial Mechanics
Volume: 23
Subject Category
Astronomy
Accession Number
81A28627
Distribution Limits
Public
Copyright
Other

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