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Callisto - Disk temperature at 3.71-centimeter wavelengthWe observed the radio emission of Callisto with a three-element interferometer at the time of the 1973 opposition of Jupiter. Special care was taken to remove the residual, unresolved contribution from Jupiter itself in the antenna side lobes. The resulting disk temperature at a wavelength of 3.71 centimeters, assuming a radius of 2500 + or - 75 kilometers for Callisto, was 101 + or - 25 K. This temperature is much more consistent with emission from a simple dielectric sphere than the considerably higher temperatures that have been reported for wavelengths of 3.5 and 8.2 millimeters.
Document ID
19750036451
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Berge, G. L.
(Owens Valley Radio Observatory Pasadena, Calif., United States)
Muhleman, D. O.
(California Institute of Technology Pasadena, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
February 7, 1975
Publication Information
Publication: Science
Volume: 187
Subject Category
Lunar And Planetary Exploration
Accession Number
75A20523
Funding Number(s)
CONTRACT_GRANT: NSF GP-30400X
CONTRACT_GRANT: N00014-67-A-0094-0019
CONTRACT_GRANT: NGR-05-002-114
Distribution Limits
Public
Copyright
Other

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