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Temperature of comet IRAS-Araki-Alcock (1983d)Comet 1983d was named IRAS-Araki-Alcock in honor of its codiscoverers, including the Infrared Astronomical Satellite (IRAS) and two amateur astronomers. It is pointed out that the apparition of Comet 1983d was the closest cometary approach to earth since the development of modern astronomy. Because of the evolution of electromagnetic detector technology, a large range of ground-based observations of this object were possible. In the present investigation, attention is given to observations and some interpretations of the spectrum of Comet IRAS-Araki-Alcock in the wavelength region from 1.5 to 20 microns. In addition to the observations made with a bolometer and discrete filters, spectrophotometric observations were made of the nuclear condensation of Comet 1983d in the 1.5- to 2.6-micron wavelength region at 5 percent resolution.
Document ID
19850056136
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Brown, R. H.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA; Hawaii, University Honolulu and Hilo, HI, United States)
Cruikshank, D. P.
(Hawaii, University Honolulu and Hilo, HI, United States)
Griep, D.
(Mauna Kea Observatory Hilo, HI, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Icarus
Volume: 62
ISSN: 0019-1035
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0019-1035
Accession Number
85A38287
Funding Number(s)
CONTRACT_GRANT: NGL-12-001-057
CONTRACT_GRANT: NSG-7312
CONTRACT_GRANT: NSG-7323
Distribution Limits
Public
Copyright
Other

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