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The effective temperature of UranusUranus was observed in the spectral region from 40 to 250 microns with a 102-cm balloon-borne telescope, and the results were interpreted in terms of model atmosphere calculations to yield an effective temperature of 58 plus or minus 3 K; this sets an upper limit of about 28 per cent on the relative contribution of an internal heat source to the total thermal radiation. On the same flight, the brightness temperatures of Venus (215 plus or minus 13 K) and Jupiter (135 plus or minus 6 K) were also measured, thus reconfirming the existence of an internal heat source for Jupiter.
Document ID
19770027905
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Fazio, G. G.
(Arizona Univ. Tucson, AZ, United States)
Traub, W. A.
(Harvard College Observatory and Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Low, F. J.
(Arizona, University Tucson, Ariz., United States)
Trafton, L.
(Texas, University Austin, Tex., United States)
Wright, E. L.
(Arizona Univ. Tucson, AZ, United States)
Date Acquired
August 8, 2013
Publication Date
October 15, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 209
Subject Category
Lunar And Planetary Exploration
Accession Number
77A10757
Funding Number(s)
CONTRACT_GRANT: NGR-09-015-047
CONTRACT_GRANT: NGR-44-012-152
CONTRACT_GRANT: NGR-22-007-270
Distribution Limits
Public
Copyright
Other

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