Reflectance Spectroscopy of Ferric Sulfate-Bearing Montmorillonites as Mars Soil Analog Materials

Spectroscopic analyses have shown that smectites enhanced in the laboratory with additional ferric species exhibit important similarities to those of the soils on Mars. Ferrihydrite in these chemically treated smectites has features in the visible to near-infrared region that resemble the energies a...

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Veröffentlicht in:Icarus (New York, N.Y. 1962) N.Y. 1962), 1995-09, Vol.117 (1), p.101-119
Hauptverfasser: Bishop, Janice L., Pieters, Carlé M., Burns, Roger G., Edwards, John O., Mancinelli, Rocco L., Fröschl, Heinz
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container_end_page 119
container_issue 1
container_start_page 101
container_title Icarus (New York, N.Y. 1962)
container_volume 117
creator Bishop, Janice L.
Pieters, Carlé M.
Burns, Roger G.
Edwards, John O.
Mancinelli, Rocco L.
Fröschl, Heinz
description Spectroscopic analyses have shown that smectites enhanced in the laboratory with additional ferric species exhibit important similarities to those of the soils on Mars. Ferrihydrite in these chemically treated smectites has features in the visible to near-infrared region that resemble the energies and band strengths of features in reflectance spectra observed for several bright regions on Mars. New samples have been prepared with sulfate as well, because S was found by Viking to be a major component in the surface material on Mars. A suite of ferrihydrite-bearing and ferric sulfate-bearing montmorillonites, prepared with variable Fe 3+ and S concentrations and variable pH conditions, has been analyzed using reflectance spectroscopy in the visible and infrared regions, Mössbauer spectroscopy at room temperature and 4 K, differential thermal analysis, and X-ray diffraction. These analyses support the formation of ferrihydrite of variable crystallinity in the ferrihydrite-bearing montmorillonites and a combination of schwertmannite and ferrihydrite in the ferric sulfate-bearing montmorillonites. Small quantities of poorly crystalline or nanophase forms of other ferric materials may also be present in these samples. The chemical formation conditions of the ferrihydrite-bearing and ferric sulfate-bearing montmorillonites influence the character of the low temperature Mössbauer sextets and the visible reflectance spectra. An absorption minimum is observed at 0.88-0.89 μm in spectra of the ferric sulfate-bearing samples, and at 0.89-0.92 μm in spectra of the ferrihydrite-bearing montmorillonites. Mössbauer spectra of the ferric sulfate-bearing montmorillonites indicate variable concentrations of ferrihydrite and schwertmannite in the interlaminar spaces and along grain surfaces. Dehydration under reduced atmospheric pressure conditions induces a greater effect on the adsorbed and interlayer water in ferrihydrite-bearing montmorillonite than on the water in ferric sulfate-bearing montmorillonite. Reflectance spectra of ferric sulfate-bearing montmorillonite include a strong 3-μm band that is more resistant to dry atmospheric conditions than the 3-μm band in spectra of similarly prepared ferrihydrite-bearing montmorillonites.
doi_str_mv 10.1006/icar.1995.1145
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Ferrihydrite in these chemically treated smectites has features in the visible to near-infrared region that resemble the energies and band strengths of features in reflectance spectra observed for several bright regions on Mars. New samples have been prepared with sulfate as well, because S was found by Viking to be a major component in the surface material on Mars. A suite of ferrihydrite-bearing and ferric sulfate-bearing montmorillonites, prepared with variable Fe 3+ and S concentrations and variable pH conditions, has been analyzed using reflectance spectroscopy in the visible and infrared regions, Mössbauer spectroscopy at room temperature and 4 K, differential thermal analysis, and X-ray diffraction. These analyses support the formation of ferrihydrite of variable crystallinity in the ferrihydrite-bearing montmorillonites and a combination of schwertmannite and ferrihydrite in the ferric sulfate-bearing montmorillonites. 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Ferrihydrite in these chemically treated smectites has features in the visible to near-infrared region that resemble the energies and band strengths of features in reflectance spectra observed for several bright regions on Mars. New samples have been prepared with sulfate as well, because S was found by Viking to be a major component in the surface material on Mars. A suite of ferrihydrite-bearing and ferric sulfate-bearing montmorillonites, prepared with variable Fe 3+ and S concentrations and variable pH conditions, has been analyzed using reflectance spectroscopy in the visible and infrared regions, Mössbauer spectroscopy at room temperature and 4 K, differential thermal analysis, and X-ray diffraction. These analyses support the formation of ferrihydrite of variable crystallinity in the ferrihydrite-bearing montmorillonites and a combination of schwertmannite and ferrihydrite in the ferric sulfate-bearing montmorillonites. Small quantities of poorly crystalline or nanophase forms of other ferric materials may also be present in these samples. The chemical formation conditions of the ferrihydrite-bearing and ferric sulfate-bearing montmorillonites influence the character of the low temperature Mössbauer sextets and the visible reflectance spectra. An absorption minimum is observed at 0.88-0.89 μm in spectra of the ferric sulfate-bearing samples, and at 0.89-0.92 μm in spectra of the ferrihydrite-bearing montmorillonites. Mössbauer spectra of the ferric sulfate-bearing montmorillonites indicate variable concentrations of ferrihydrite and schwertmannite in the interlaminar spaces and along grain surfaces. Dehydration under reduced atmospheric pressure conditions induces a greater effect on the adsorbed and interlayer water in ferrihydrite-bearing montmorillonite than on the water in ferric sulfate-bearing montmorillonite. Reflectance spectra of ferric sulfate-bearing montmorillonite include a strong 3-μm band that is more resistant to dry atmospheric conditions than the 3-μm band in spectra of similarly prepared ferrihydrite-bearing montmorillonites.</abstract><cop>Headquarters</cop><pub>Elsevier Inc</pub><pmid>11538594</pmid><doi>10.1006/icar.1995.1145</doi><tpages>19</tpages></addata></record>
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identifier ISSN: 0019-1035
ispartof Icarus (New York, N.Y. 1962), 1995-09, Vol.117 (1), p.101-119
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source MEDLINE; Elsevier ScienceDirect Journals; NASA Technical Reports Server
subjects Aluminum Silicates - chemistry
Atmospheric Pressure
Bentonite - chemistry
Crystallization
Extraterrestrial Environment
Ferric Compounds - analysis
Gastrointestinal Agents - analysis
Hydrogen-Ion Concentration
Lunar And Planetary Science And Exploration
Mars
Models, Theoretical
Silicates
Soil - analysis
Space life sciences
Spectroscopy, Mossbauer
Spectrum Analysis
Temperature
X-Ray Diffraction
title Reflectance Spectroscopy of Ferric Sulfate-Bearing Montmorillonites as Mars Soil Analog Materials
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