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Ice and minerals on Callisto - A reassessment of the reflectance spectraThe results of a comparison of laboratory spectral reflectance measurements of particulate mixtures of both hydrated silicates and palagonite with water ice, on the one hand, with two previously unpublished reflectance spectra of Callisto, yield direct support for the hypothesis that the measured reflectance of Callisto includes a substantial nonice component. Hapke's (1981) equations are used in a theoretical model for thorough analysis of telescopic data; a comparison of the calculation results thus obtained with measured reflectance data for Callisto indicate that three-component, ice/magnetite/serpentine mixtures are a better match for telescopic data than two-component ice mixtures.
Document ID
19900057254
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Roush, T. L.
(NASA Ames Research Center Moffett Field, CA, United States)
Pollack, J. B.
(NASA Ames Research Center Moffett Field, CA, United States)
Witteborn, F. C.
(NASA Ames Research Center Moffett Field, CA, United States)
Bregman, J. D.
(NASA Ames Research Center Moffett Field, CA, United States)
Simpson, J. P.
(California, University Berkeley, United States)
Date Acquired
August 14, 2013
Publication Date
August 1, 1990
Publication Information
Publication: Icarus
Volume: 86
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
90A44309
Distribution Limits
Public
Copyright
Other

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