Mathematics – Logic
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jgre..11312s43h&link_type=abstract
Journal of Geophysical Research, Volume 113, Issue E12, CiteID E12S43
Mathematics
Logic
8
Planetary Sciences: Solid Surface Planets: Composition (1060, 3672), Mineralogy And Petrology: Planetary Mineralogy And Petrology (5410), Mineralogy And Petrology: Alteration And Weathering Processes (1039), Planetary Sciences: Solid Surface Planets: Remote Sensing, Planetary Sciences: Solar System Objects: Mars
Scientific paper
We studied visible to near-infrared (VNIR, 0.35-2.5 μm) and middle infrared (MIR, 1800-250 cm-1, also called thermal infrared and vibrational) spectra of basaltic tephras from Mauna Kea volcano that were altered under ambient, hydrothermal (hydrolytic and acid sulfate), and dry heat conditions. Although models of MIR spectra of altered tephras generally produce fits whose quality is reduced compared to deconvolutions of primary lithologies, they successfully identify major alteration phases (cristobalite, oxide, phyllosilicate, and sulfate) except in palagonites. MIR spectra of the <45 μm fraction of all altered tephra samples exhibit an H2O peak at ~1640 cm-1, but it cannot be used as an indicator of H2O content. This feature is present with band strengths >1% in spectra of the 500-1000 μm fraction only if phyllosilicates are present. Although Mauna Kea palagonitic tephra is considered a VNIR analog to Martian dust, comparison of MIR altered tephra spectra (<45 μm fraction) to dust spectra retrieved from Mars Global Surveyor and Mars Exploration Rover instruments do not provide good spectral matches. The best MIR match is a tephra that has a strong plagioclase feldspar transparency feature and was altered under dry, high-temperature, oxidizing conditions. This sample is not a VNIR analog and is not a process analog, but it emphasizes the mineralogical importance of plagioclase feldspar in Martian dust. No single tephra is a good spectral analog across the VNIR and MIR. We found no evidence for substantial sulfates or phyllosilicates in Mini-Thermal Emission Spectrometer (Mini-TES) spectra from Gusev Crater.
Gruener John E.
Hamilton Victoria E.
Mertzman Stanley A.
Morris Richard V.
No associations
LandOfFree
Visible, near-infrared, and middle infrared spectroscopy of altered basaltic tephras: Spectral signatures of phyllosilicates, sulfates, and other aqueous alteration products with application to the mineralogy of the Columbia Hills of Gusev Crater, Mars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Visible, near-infrared, and middle infrared spectroscopy of altered basaltic tephras: Spectral signatures of phyllosilicates, sulfates, and other aqueous alteration products with application to the mineralogy of the Columbia Hills of Gusev Crater, Mars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Visible, near-infrared, and middle infrared spectroscopy of altered basaltic tephras: Spectral signatures of phyllosilicates, sulfates, and other aqueous alteration products with application to the mineralogy of the Columbia Hills of Gusev Crater, Mars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-969484