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Spectral characterization of Martian soil analoguesAs previously reported, reflectance spectra of iron oxide precipitated as ultrafine particles, unlike ordinary fine grained hematite, have significant similarities to reflectance spectra from the bright regions of Mars. These particles were characterized according to composition, magnetic properties, and particle size distribution. Mossbauer, magnetic susceptibility, and optical data were obtained for samples with a range of concentrations of iron oxide in silica gel of varying pore diameters. To analyze the Mossbauer spectra, a versatile fitting program was enhanced to provide user friendly screen input and theoretical models appropriate for the superparamagnetic spectra obtained.
Document ID
19870017260
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Agresti, David G.
(Alabama Univ. Birmingham, AL, United States)
Date Acquired
September 5, 2013
Publication Date
June 1, 1987
Publication Information
Publication: NASA. Lyndon B.
Subject Category
Lunar And Planetary Exploration
Accession Number
87N26693
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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