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dc.contributor.authorCloutis, Edward A.
dc.contributor.authorGaffey, Michael J.
dc.contributor.authorJackowski, Timothy L.
dc.contributor.authorReed, Kevin L.
dc.date.accessioned2018-03-13T17:36:23Z
dc.date.available2018-03-13T17:36:23Z
dc.date.issued1986-10-10
dc.identifier.citationCloutis, E. A., M. J. Gaffey, T. L. Jackowski, and K. L. Reed. "Calibrations of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectra." Journal of Geophysical Research 91 (1986): 11,641-11,653.en_US
dc.identifier.issn0148-0227
dc.identifier.urihttp://hdl.handle.net/10680/1401
dc.description.abstractSpectral reflectance measurements of characterized (phase abundance, particle size) mixtures of olivine and orthopyroxene were utilized to define the correlations between spectral and albedo parameters of such assemblages and their mineralogical or textural properties. Thirty-three different spectral parameters falling into three general classes (relative or ratioed, absolute or albedo, and wavelength) were investigated for empirical sensitivity to one or more of the mixture properties. Theoretical considerations and previous experimental observations were utilized to understand their functional relationships. The ratio of areas for the 1- and 2-3µm absorption bands is shown to be a sensitive indicator of the olivine-orthopyroxene abundance and is very nearly independent of particle size and mineral composition. In conjunction with an abundance determination, the wavelength position of the 1-3tm absorption feature can be utilized to determine the molar iron contents of the olivine and orthopyroxene phases. This calibration is insensitive to particle size but will produce systematic deviations if the phases have significantly different iron contents or if more than a few percent of a clinopyroxene component is present. The spectral albedo in the 0.6- to 0.7-µm region is relatively insensitive to phase abundance and can be used to constrain particle size if phase composition has been determineden_US
dc.description.sponsorshipVarious portions of this work were supported at the University of Hawaii by NASA grant NSG-7312 and by a Sigma Xi Foundation grant to E.A.C. and at Rensselaer Polytechnic Institute by NASA grant NAGW-642. Planetary Geosciences Division, Hawaii Institute of Geophysics, University of Hawaii, publication4 70.en_US
dc.language.isoenen_US
dc.publisherAmerican Geophysical Unionen_US
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectOlivine-Orthopyroxene mixturesen_US
dc.titleCalibrations of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectraen_US
dc.typeArticleen_US


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