The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials

Reflectance spectra are presented here for a variety of particulate, ferric-containing analogs to Martian soil (Fe(3+)-doped smectites and palagonites) to facilitate interpretation of remotely acquired spectra. The analog spectra were measured under differing environmental conditions to evaluate the...

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Main Authors: Pratt, S., Mustard, J., Bishop, J., Pieters, C., Murchie, S.
Format: Other/Unknown Material
Language:unknown
Published: 1993
Subjects:
Online Access:http://hdl.handle.net/2060/19940028689
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19940028689 2023-05-15T16:52:01+02:00 The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials Pratt, S. Mustard, J. Bishop, J. Pieters, C. Murchie, S. Unclassified, Unlimited, Publicly available JAN 1, 1993 application/pdf http://hdl.handle.net/2060/19940028689 unknown Document ID: 19940028689 Accession ID: 94N33195 http://hdl.handle.net/2060/19940028689 No Copyright CASI LUNAR AND PLANETARY EXPLORATION Lunar and Planetary Inst., Mars: Past, Present, and Future. Results from the MSATT Program, Part 1; p 4-6 1993 ftnasantrs 2019-07-21T08:20:20Z Reflectance spectra are presented here for a variety of particulate, ferric-containing analogs to Martian soil (Fe(3+)-doped smectites and palagonites) to facilitate interpretation of remotely acquired spectra. The analog spectra were measured under differing environmental conditions to evaluate the influence of exposure history on water content and absorption features due to H2O in these samples. Each of these materials contains structural OH bonded to metal cations, adsorbed H2O, and bound H2O (either in a glass, structural site, or bound to a cation). Previous experiments involving a variety of Mars analogs have shown that the 3 micron H2O band in spectra of palagonites is more resistant to drying than the 3 micron H2O band in spectra of montmorillonites. Other experiments have shown that spectra of ferrihydrite and montmorillonites doped with ferric sulfate also contain sufficient bound H2O to retain a strong 3 micron band under dry conditions. Once the effects of the environment on bound water in clays, oxides, and salts are better understood, the hydration bands measured via reflectance spectroscopy can be used to gain information about the chemical composition and moisture content of real soil systems. Such information would be especially useful in interpreting observations of Mars where subtle spatial variations in the strengths of metal-OH and H2O absorptions have been observed in telescopic and ISM spectra. We measured bidirectional reflectance spectra of several Mars soil analogs under controlled environmental conditions to assess the effects of moisture content on the metal-OH and H2O absorptions. The samples analyzed include chemically altered montmorillonites, ferrihydrite. and palagonites from Hawaii and Iceland. Procedures for preparation of the cation-exchanged montmorillonites, ferric-salt doped montmorillonites, and ferric oxyhydroxides are described in detail elsewhere. Other/Unknown Material Iceland NASA Technical Reports Server (NTRS)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic LUNAR AND PLANETARY EXPLORATION
spellingShingle LUNAR AND PLANETARY EXPLORATION
Pratt, S.
Mustard, J.
Bishop, J.
Pieters, C.
Murchie, S.
The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials
topic_facet LUNAR AND PLANETARY EXPLORATION
description Reflectance spectra are presented here for a variety of particulate, ferric-containing analogs to Martian soil (Fe(3+)-doped smectites and palagonites) to facilitate interpretation of remotely acquired spectra. The analog spectra were measured under differing environmental conditions to evaluate the influence of exposure history on water content and absorption features due to H2O in these samples. Each of these materials contains structural OH bonded to metal cations, adsorbed H2O, and bound H2O (either in a glass, structural site, or bound to a cation). Previous experiments involving a variety of Mars analogs have shown that the 3 micron H2O band in spectra of palagonites is more resistant to drying than the 3 micron H2O band in spectra of montmorillonites. Other experiments have shown that spectra of ferrihydrite and montmorillonites doped with ferric sulfate also contain sufficient bound H2O to retain a strong 3 micron band under dry conditions. Once the effects of the environment on bound water in clays, oxides, and salts are better understood, the hydration bands measured via reflectance spectroscopy can be used to gain information about the chemical composition and moisture content of real soil systems. Such information would be especially useful in interpreting observations of Mars where subtle spatial variations in the strengths of metal-OH and H2O absorptions have been observed in telescopic and ISM spectra. We measured bidirectional reflectance spectra of several Mars soil analogs under controlled environmental conditions to assess the effects of moisture content on the metal-OH and H2O absorptions. The samples analyzed include chemically altered montmorillonites, ferrihydrite. and palagonites from Hawaii and Iceland. Procedures for preparation of the cation-exchanged montmorillonites, ferric-salt doped montmorillonites, and ferric oxyhydroxides are described in detail elsewhere.
format Other/Unknown Material
author Pratt, S.
Mustard, J.
Bishop, J.
Pieters, C.
Murchie, S.
author_facet Pratt, S.
Mustard, J.
Bishop, J.
Pieters, C.
Murchie, S.
author_sort Pratt, S.
title The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials
title_short The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials
title_full The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials
title_fullStr The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials
title_full_unstemmed The importance of environmental conditions in reflectance spectroscopy of laboratory analogs for Mars surface materials
title_sort importance of environmental conditions in reflectance spectroscopy of laboratory analogs for mars surface materials
publishDate 1993
url http://hdl.handle.net/2060/19940028689
op_coverage Unclassified, Unlimited, Publicly available
genre Iceland
genre_facet Iceland
op_source CASI
op_relation Document ID: 19940028689
Accession ID: 94N33195
http://hdl.handle.net/2060/19940028689
op_rights No Copyright
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