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Photographic observations of Comet Bennett, 1970II.Direct photography of Comet Bennett with a range of focal lengths shows structure in the coma and strong Type I and Type II tails. The Type I tail shows motion in 15 minutes. The inner coma contains spiral-shaped jets of a type observed visually on occasion in the past but not photographed before. The spiral shape is apparently due to the rotation of the nucleus. On the assumption that the outward velocity of the jets is 0.6 km/sec, as estimated by Delsemme, a rotation period of 1.4-1.5 days is derived for the nucleus. The rotation is direct (i.e., in the sense of the comet's orbital motion).
Document ID
19730029964
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Larson, S. M.
Minton, R. B.
(Arizona, University Tucson, Ariz., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1972
Subject Category
Space Sciences
Meeting Information
Meeting: Tucson Comet Conference
Location: Tucson, AZ
Start Date: April 8, 1970
End Date: April 9, 1970
Accession Number
73A14766
Funding Number(s)
CONTRACT_GRANT: NGL-03-002-002
Distribution Limits
Public
Copyright
Other

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