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The outer solar system for 200 million yearsA special-purpose computer is used to integrate the orbits of the outer five planets for more than 100 Myr into the future and more than 100 Myr into the past. The strongest features in the Fourier transforms of the orbital elements of the Jovian planets can be identified with the frequencies predicted by linear secular theory. Many of the weaker features in the Fourier spectra are identified as linear combinations of the basic frequencies. Serious differences are noted between the present measurements and the predictions of Bretagnon (1974). The amplitude of the 3.796 Myr period libration of Pluto's longitude of perihelion is modulated with a period of 34 Myr. Very long periods, on the order of 137 Myr, are also seen. The orbit of Pluto is stable for the duration of the integration; the maximum Liapunov characteristic exponent is less than 10 to the -6.8 power/yr.
Document ID
19860060859
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Applegate, J. H.
(Columbia University New York, United States)
Douglas, M. R.
(California Institute of Technology Pasadena, United States)
Gursel, Y.
(Columbia Univ. New York, NY, United States)
Sussman, G. J.
(Columbia Univ. New York, NY, United States)
Wisdom, J.
(MIT Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
July 1, 1986
Publication Information
Publication: Astronomical Journal
Volume: 92
ISSN: 0004-6256
Subject Category
Astrophysics
Accession Number
86A45597
Funding Number(s)
CONTRACT_GRANT: NAGW-706
Distribution Limits
Public
Copyright
Other

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