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Mineralogy of three slightly palagonitized basaltic tephra samples from the summit of Mauna Kea, HawaiiThe paper characterizes the mineralogy and spectral properties of three slightly palagonitized basaltic tephra samples collected near the summit of Mauna Kea in order to contribute to the basis for inferring mineralogy and processes for Martian surface materials. The mineralogy of size fractions of these samples is examined by diffuse reflectance and FIR spectroscopy, optical microscopy, X-ray diffraction, Moessbauer spectroscopy, magnetic analysis, EMPA, TEM, and SEM. For the 20-1000 micron size fraction, sample HWMK11 (red) is essentially completely oxidized and has a hematite (Ti-hematite) pigment dispersed throughout the silicate matrix. Sample HWMK12 (black) has the lowest proportion of ferric-bearing phases and is thus least weathered. For HWMK11, the amount of hematite is essentially constant, and mica is present only in the coarse clay-sized fraction; smectites are low in structural Fe.
Document ID
19930046765
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Golden, D. C.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Morris, R. V.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Ming, D. W.
(NASA Johnson Space Center Houston, TX, United States)
Lauer, H. V., Jr.
(NASA Lyndon B. Johnson Space Center Houston, TX, United States)
Yang, S. R.
(Lockheed Engineering and Sciences Co. Houston, TX, United States)
Date Acquired
August 16, 2013
Publication Date
February 25, 1993
Publication Information
Publication: Journal of Geophysical Research
Volume: 98
Issue: E2
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
93A30762
Distribution Limits
Public
Copyright
Other

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