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An exploratory 5-micron spectrum of UranusThe intensity peak at 4.8 microns characterizing the spectrum observed for the disk of Uranus near 5 microns, in June 1987, exhibits steep declines at shorter and longer wavelength. An exploratory discussion is presented of various models in view of these data; it is noted that some component of the radiation must originate near the 140 K atmospheric irrespective of the radiation's origin in sunlight or thermal emission; physical considerations dictate that it be at least partly thermal in origin. One model consistent with the data requires the presence of a cloud top at the 8-bar level.
Document ID
19890040721
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Orton, Glenn S.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Kaminski, Charles D.
(NASA Infrared Telescope Facility Hilo, HI, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1989
Publication Information
Publication: Icarus
Volume: 77
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0019-1035
Accession Number
89A28092
Distribution Limits
Public
Copyright
Other

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