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Dynamics of Pluto and CharonThe dynamics of the Pluto-Charon system are reviewed from a historical perspective. Although Pluto's orbit crosses Neptune's, an intricate system of nested resonances keeps these planets apart. Pluto's orbit is apparently chaotic as well. Pluto always keeps the same face turned toward Charon, and vice versa. Tides also damp Charon's orbital eccentricity and inclination. Precession of Pluto's orbital plane causes Pluto's obliquity to vary periodically from formally prograde to retrograde. Pluto is probably an original member of the Solar system, but not an escaped satellite of Neptune.
Document ID
19900027049
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Dobrovolskis, Anthony R.
(NASA Ames Research Center Moffett Field; Lick Observatory, Santa Cruz, CA, United States)
Date Acquired
August 14, 2013
Publication Date
November 1, 1989
Publication Information
Publication: Geophysical Research Letters
Volume: 16
ISSN: 0094-8276
Subject Category
Astronomy
Accession Number
90A14104
Distribution Limits
Public
Copyright
Other

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