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Cometary dynamicsIn order to provide observers with accurate cometary ephemerides, up-to-date astrometric positions must be used to update the existing orbit and ephemeris for each object. In addition, nongravitational forces must be taken into account; these forces are assumed due to the rocket effect of outgassing cometary ices. Once successfully modeled, the cometary nucleus spin direction, spin axis evolution, and the volatility of the nucleus ices can be inferred. The predicted ephemerides also become far more accurate.
Document ID
19870003046
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Yeomans, D. K.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1986
Publication Information
Publication: NASA, Washington Reports of Planetary Astronomy, 1985
Subject Category
Astrophysics
Accession Number
87N12479
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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