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Radiometry of DeimosGround-based infrared photometry of Deimos at 4.8, 10, and 20 microns is reported. The observed fluxes are significantly brighter than predicted by the 'standard' thermal model. Recent recalibrations that modify the model beam pattern of the infrared emission are marginally consistent with the observations at 10 and 20, but not at 4.8 microns.
Document ID
19880032071
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/114574
Authors
Veeder, Glenn J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Matson, Dennis L. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Tedesco, Edward F. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Lebofsky, Larry A. (Arizona, University Tucson, United States)
Gradie, Jonathan C. (Hawaii, University Honolulu, United States)
Date Acquired
August 13, 2013
Publication Date
November 1, 1987
Publication Information
Publication: Astronomical Journal
Volume: 94
ISSN: 0004-6256
Subject Category
Lunar And Planetary Exploration
Accession Number
88A19298
Distribution Limits
Public
Copyright
Other

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