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Io - Ground-based observations of hot spotsObservations of Io in eclipse demonstrate conclusively that Io emits substantial amounts of radiation at 4.8 and 3.8 micrometers and a measurable amount at 2.2 micrometers. Color temperatures derived from the observations fit blackbody emission at 560 K. The required source area to yield the observed 4.8-micrometer flux is approximately 5 x 10 to the -5th of the disk of Io and is most likely comprised of small hot spots in the vicinity of the volcanoes.
Document ID
19810028944
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sinton, W. M.
(Hawaii Univ. Honolulu, HI, United States)
Tokunaga, A. T.
(Hawaii Univ. Honolulu, HI, United States)
Becklin, E. E.
(Hawaii, University Honolulu, Hawaii, United States)
Gatley, I.
(Hawaii Univ. Honolulu, HI, United States)
Lee, T. J.
(Edinburgh, Royal Observatory, U.K. Infrared Telescope Unit, Hilo Hawaii, United States)
Lonsdale, C. J.
(Edinburgh, University Edinburgh, United Kingdom)
Date Acquired
August 11, 2013
Publication Date
November 28, 1980
Publication Information
Publication: Science
Volume: 210
Subject Category
Lunar And Planetary Exploration
Accession Number
81A13348
Funding Number(s)
CONTRACT_GRANT: NGL-12-001-057
Distribution Limits
Public
Copyright
Other

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