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A discussion of Hill's method of secular perturbations and its application to the determination of the zero-rank effects in non- singular vectorial elements of a planetary motionPlanetary motion zero-rank effects numerical integration, using Hill secular perturbation method and trace of dyadics
Document ID
19700054588
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Musen, P.
Date Acquired
August 5, 2013
Publication Date
May 1, 1970
Subject Category
Space Sciences
Accession Number
70A30704
Distribution Limits
Public
Copyright
Other

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