Skip to main content Accessibility help
×
Hostname: page-component-848d4c4894-2pzkn Total loading time: 0 Render date: 2024-06-07T12:49:35.438Z Has data issue: false hasContentIssue false

4 - Visible and Near-Infrared Reflectance Spectroscopy

Laboratory Spectra of Geologic Materials

from Part I - Theory of Remote Compositional Analysis Techniques and Laboratory Measurements

Published online by Cambridge University Press:  15 November 2019

Janice L. Bishop
Affiliation:
SETI Institute, California
James F. Bell III
Affiliation:
Arizona State University
Jeffrey E. Moersch
Affiliation:
University of Tennessee, Knoxville
Get access

Summary

Visible/near-infrared (VNIR) reflectance spectra are used in laboratory, field, and airborne studies to characterize geologic materials. This chapter covers the region 0.3–5 µm and describes the species responsible for the absorption of radiation at specific wavelengths that create spectral features used to identify minerals, rocks, and other geologic materials. Fe contributes greatly to VNIR spectral signatures, producing features near 1 and 2 µm for Fe2+ in spectra of pyroxene and glass, while a broad, strong band from ~0.9 to 1.3 µm is characteristic of Fe2+ in olivine, carbonate, and many sulfates; a weak band near 1.2 µm is due to Fe2+ in feldspar; and bands near 0.6 and 0.9 µm arise from Fe3+ in ferric oxides/hydroxides. Water bands occur near 0.96, 1.15, 1.4, 1.9, and 2.9 µm, depending on the mineral structure, while structural OH bands occur near 1.4, 2.1–2.5, and 2.7 µm. Additional features are observed for carbonates, nitrates, sulfates, phosphates, chlorides, and perchlorates. The spectral signatures of geologic samples are also affected by how photons interact with particles in the sample. Factors such as grain size, coatings and mixtures influence the reflectance, transmittance, and absorption of photons at grain boundaries and contribute to the VNIR spectral properties of geologic materials.

Type
Chapter
Information
Remote Compositional Analysis
Techniques for Understanding Spectroscopy, Mineralogy, and Geochemistry of Planetary Surfaces
, pp. 68 - 101
Publisher: Cambridge University Press
Print publication year: 2019

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Adams, J.B. (1974) Visible and near-infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the Solar System. Journal of Geophysical Research, 79, 48294836.Google Scholar
Adams, J.B. (1975) Interpretation of visible and near-infrared diffuse reflectance spectra of pyroxenes and other rock-forming minerals. In: Infrared and Raman spectroscopy of lunar and terrestrial minerals (Karr, C., ed.). Academic Press, New York, 91116.CrossRefGoogle Scholar
Adams, J.B. & Filice, A.L. (1967) Spectral reflectance 0.4 to 2.0 microns of silicate rock powders. Journal of Geophysical Research, 72, 57055715.CrossRefGoogle Scholar
Adams, J.B. & Goullaud, L.H. (1978) Plagioclase feldspars: Visible and near infrared diffuse reflectance spectra as applied to remote sensing. Proceedings of the 9th Lunar and Planetary Science Conference, 29012909.Google Scholar
Allen, C.C., Gooding, J.L., Jercinovic, M., & Keil, K. (1981) Altered basaltic glass: A terrestrial analog to the soil of Mars. Icarus, 45, 347369.Google Scholar
Amador, E.S., Bishop, J.L., McKeown, N.K., Parente, M., & Clark, J.T. (2009) Detection of Kaolinite at Mawrth Vallis, Mars: Analysis of laboratory mixtures and development of remote sensing parameters. 40th Lunar Planet. Sci. Conf., Abstract #2188.Google Scholar
Anderson, J.H. & Wickersheim, K.A. (1964) Near infrared characterization of water and hydroxyl groups on silica surfaces. Surface Science, 2, 252260.Google Scholar
Baker, L.L., Strawn, D.G., McDaniel, P.A., et al. (2011) Poorly crystalline, iron-bearing aluminosilicates and their importance on Mars. 42nd Lunar Planet. Sci. Conf., Abstract #1939.Google Scholar
Bell, J.F., III, Morris, R.V. & Adams, J.B. (1993) Thermally altered palagonitic tephra: A spectral and process analog to the soil and dust of Mars. Journal of Geophysical Research, 98, 33733385.Google Scholar
Bigham, J.M., Schwertmann, U., Traina, S.J., Winland, R.L., & Wolf, M. (1996) Schwertmannite and the chemical modeling of iron in acid sulfate waters. Geochimica Cosmochimica Acta, 60, 21112121.Google Scholar
Bish, D. & Carey, J.W. (2001) Thermal behavior of natural zeolites. In: Natural zeolites: Occurrence, properties, and applications. Mineralogical Society of America Reviews in Mineralogy and Geochemistry (Bish, D.L. & Ming, D.W., eds.). Mineralogical Society of America, Washington, DC, 403–452.Google Scholar
Bish, D.L., Carey, J.W., Vaniman, D.T., & Chipera, S.J. (2003) Stability of hydrous minerals on the martian surface. Icarus, 164, 96103.CrossRefGoogle Scholar
Bishop, J.L. (2005) Hydrated minerals on Mars. In: Water on Mars and life. Advances in Astrobiology and Biogeophysics. (Tokano, T., ed.). Springer, Berlin, 65–96.Google Scholar
Bishop, J.L. & Murad, E. (1996) Schwertmannite on Mars? Spectroscopic analyses of schwertmannite, its relationship to other ferric minerals, and its possible presence in the surface material on Mars. In: Mineral spectroscopy: A tribute to Roger G. Burns (Dyar, M.D., McCammon, C., & Schaefer, M.W., eds.). The Geochemical Society, Houston, TX, 337358.Google Scholar
Bishop, J.L. & Murad, E. (2002) Spectroscopic and geochemical analyses of ferrihydrite from hydrothermal springs in Iceland and applications to Mars. In: Volcano–ice interactions on Earth and Mars (Smellie, J.L. & Chapman, M.G., eds.). Special Publication No.202. Geological Society, London, 357370.Google Scholar
Bishop, J.L. & Murad, E. (2005) The visible and infrared spectral properties of jarosite and alunite. American Mineralogist, 90, 11001107.Google Scholar
Bishop, J.L. & Pieters, C.M. (1995) Low-temperature and low atmospheric pressure infrared reflectance spectroscopy of Mars soil analog materials. Journal of Geophysical Research, 100, 53695379.Google Scholar
Bishop, J.L. & Rampe, E.B. (2016) Evidence for a changing martian climate from the mineralogy at Mawrth Vallis. Earth and Planetary Science Letters, 448, 4248.Google Scholar
Bishop, J.L., Pieters, C.M., & Burns, R.G. (1993) Reflectance and Mössbauer spectroscopy of ferrihydrite-montmorillonite assemblages as Mars soil analog materials. Geochimica Cosmochimica Acta, 57, 45834595.Google Scholar
Bishop, J.L., Pieters, C.M., & Edwards, J.O. (1994) Infrared spectroscopic analyses on the nature of water in montmorillonite. Clays and Clay Minerals, 42, 702716.CrossRefGoogle Scholar
Bishop, J.L., Fröschl, H., & Mancinelli, R.L. (1998a) Alteration processes in volcanic soils and identification of exobiologically important weathering products on Mars using remote sensing. Journal of Geophysical Research, 103, 31,45731,476.CrossRefGoogle ScholarPubMed
Bishop, J.L., Pieters, C.M., Hiroi, T., & Mustard, J.F. (1998b) Spectroscopic analysis of martian meteorite Allan Hills 84001 powder and applications for spectral identification of minerals and other soil components on Mars. Meteoritics and Planetary Science, 33, 699708.Google Scholar
Bishop, J.L., Mustard, J.F., Pieters, C.M., & Hiroi, T. (1998c) Recognition of minor constituents in reflectance spectra of Allan Hills 84001 chips and the importance for remote sensing on Mars. Meteoritics and Planetary Science, 33, 693698.Google Scholar
Bishop, J.L., Murad, E., Madejová, J., Komadel, P., Wagner, U., & Scheinost, A. (1999) Visible, Mössbauer and infrared spectroscopy of dioctahedral smectites: Structural analyses of the Fe-bearing smectites Sampor, SWy-1 and SWa-1. 11th International Clay Conference, June, 1997 (Kodama, H., Mermut, A.R., & Torrance, J.K., eds.). Ottawa, 413419.Google Scholar
Bishop, J.L., Lougear, A., Newton, J., et al. (2001) Mineralogical and geochemical analyses of Antarctic sediments: A reflectance and Mössbauer spectroscopy study with applications for remote sensing on Mars. Geochimica Cosmochimica Acta, 65, 28752897.CrossRefGoogle Scholar
Bishop, J.L., Schiffman, P., & Southard, R.J. (2002a) Geochemical and mineralogical analyses of palagonitic tuffs and altered rinds of pillow lavas on Iceland and applications to Mars. In: Volcano–ice interactions on Earth and Mars (Smellie, J.L. & Chapman, M.G., eds.). Special Publication No. 202. Geological Society, London, 371392.Google Scholar
Bishop, J.L., Murad, E., & Dyar, M.D. (2002b) The influence of octahedral and tetrahedral cation substitution on the structure of smectites and serpentines as observed through infrared spectroscopy. Clay Minerals, 37, 617628.CrossRefGoogle Scholar
Bishop, J.L., Madeová, J., Komadel, P., & Fröschl, H. (2002c) The influence of structural Fe, Al and Mg on the infrared OH bands in spectra of dioctahedral smectites. Clay Minerals, 37, 607616.Google Scholar
Bishop, J.L., Minitti, M.E., Lane, M.D., & Weitz, C.M. (2003) The influence of glassy coatings on volcanic rocks from Mauna Iki, Hawaii and applications to rocks on Mars. 34th Lunar Planet. Sci. Conf., Abstract #1516.Google Scholar
Bishop, J.L., Murad, E., Lane, M.D., & Mancinelli, R.L. (2004) Multiple techniques for mineral identification on Mars: A study of hydrothermal rocks as potential analogues for astrobiology sites on Mars. Icarus, 169, 331–323.Google Scholar
Bishop, J.L., Dyar, M.D., Lane, M.D., & Banfield, J.F. (2005) Spectral identification of hydrated sulfates on Mars and comparison with acidic environments on Earth. International Journal of Astrobiology, 3, 275285.CrossRefGoogle Scholar
Bishop, J.L., Schiffman, P., Murad, E., Dyar, M.D., Drief, A., & Lane, M.D. (2007) Characterization of alteration products in tephra from Haleakala, Maui: A visible-infrared spectroscopy, Mössbauer spectroscopy, XRD, EPMA and TEM study. Clays and Clay Minerals, 55, 117.Google Scholar
Bishop, J.L., Dyar, M.D., Sklute, E.C., & Drief, A. (2008a) Physical alteration of antigorite: A Mössbauer spectroscopy, reflectance spectroscopy and TEM study with applications to Mars. Clay Minerals, 43, 5567.CrossRefGoogle Scholar
Bishop, J.L., Lane, M.D., Dyar, M.D., & Brown, A.J. (2008b) Reflectance and emission spectroscopy study of four groups of phyllosilicates: Smectites, kaolinite-serpentines, chlorites and micas. Clay Minerals, 43, 3554.Google Scholar
Bishop, J.L., Parente, M., Weitz, C.M., et al. (2009) Mineralogy of Juventae Chasma: Sulfates in the light-toned mounds, mafic minerals in the bedrock, and hydrated silica and hydroxylated ferric sulfate on the plateau. Journal of Geophysical Research, 114, E00D09, DOI:10.1029/2009JE003352.Google Scholar
Bishop, J.L., Parente, M., & Hamilton, V.E. (2011a) Spectral signatures of martian meteorites and what they can tell us about rocks on Mars. Meteoritical Society 74th Annual Meeting, Abstract #5393.Google Scholar
Bishop, J.L., Gates, W.P., Makarewicz, H.D., McKeown, N.K., & Hiroi, T. (2011b) Reflectance spectroscopy of beidellites and their importance for Mars. Clays and Clay Minerals, 59, 376397.Google Scholar
Bishop, J.L., Schelble, R.T., McKay, C.P., Brown, A.J., & Perry, K.A. (2011c) Carbonate rocks in the Mojave Desert as an analog for martian carbonates. International Journal of Astrobiology, 10, 349358, DOI:10.1017/S1473550411000206.Google Scholar
Bishop, J.L., Perry, K.A., Dyar, M.D., et al. (2013a) Coordinated spectral and XRD analyses of magnesite-nontronite-forsterite mixtures and implications for carbonates on Mars. Journal of Geophysical Research, 118, 635650.Google Scholar
Bishop, J.L., Rampe, E.B., Bish, D.L., et al. (2013b) Spectral and hydration properties of allophane and imogolite. Clays and Clay Minerals, 61, 5774.Google Scholar
Bishop, J.L., Quinn, R.C., & Dyar, M.D. (2014a) Spectral and thermal properties of perchlorate salts and implications for Mars. American Mineralogist, 99, 15801592.CrossRefGoogle ScholarPubMed
Bishop, J.L., Lane, M.D., Dyar, M.D., King, S.J., Brown, A.J., & Swayze, G. (2014b) Spectral properties of Ca-sulfates: Gypsum, bassanite and anhydrite. American Mineralogist, 99, 21052115.Google Scholar
Bishop, J.L., Murad, E., & Dyar, M.D. (2015) Akaganéite and schwertmannite: Spectral properties, structural models and geochemical implications of their possible presence on Mars. American Mineralogist, 100, 738746.Google Scholar
Bishop, J.L., Davila, A., Hanley, J., & Roush, T.L. (2016a) Dehydration-rehydration experiments with Cl salts mixed into Mars analog materials and the effects on their VNIR spectral properties. 47th Lunar Planet. Sci. Conf., Abstract #1645.Google Scholar
Bishop, J.L., Schiffman, P., Gruendler, L., et al. (2016b) Formation of opal, clays and sulfates from volcanic ash at Kilauea Caldera as an analog for surface alteration on Mars. Clay Minerals Society 53rd Annual Meeting.Google Scholar
Bishop, J.L., King, S.J., Lane, M.D., et al. (2017) Spectral properties of anhydrous carbonates and nitrates. 48th Lunar Planet. Sci. Conf., Abstract #2362.Google Scholar
Bishop, J.L., King, S.J., Lane, M.D., et al. (2019) Spectral properties of anhydrous carbonates and nitrates. Journal of Geophysical Research, submitted.Google Scholar
Brindley, G.W. & Brown, G. (1980) Crystal structures of clay minerals and their X-ray identification. Mineralogical Society, London.Google Scholar
Burns, R.G. (1970) Crystal field spectra and evidence of cation ordering in olivine minerals. American Mineralogist, 55, 16081632.Google Scholar
Burns, R.G. (1993) Mineralogical applications of crystal field theory. Cambridge University Press, Cambridge.Google Scholar
Burns, R.G. & Huggins, F.E. (1972) Cation determinative curves for Mg-Fe-Mn olivines from vibrational spectra. American Mineralogist, 57, 967985.Google Scholar
Calvin, W.M. & King, T.V.V. (1997) Spectral characteristics of Fe-bearing phyllosilicates: Comparison to Orgueil (C11), Murchison and Murray (CM2). Meteoritics and Planetary Science, 32, 693701.Google Scholar
Calvin, W.M., King, T.V.V., & Clark, R.N. (1994) Hydrous carbonates on Mars? Evidence from Mariner 6/7 infrared spectrometer and groundbased telescopic spectra. Journal of Geophysical Research, 99, 1465914675.Google Scholar
Cannon, K.M., Mustard, J.F., Parman, S.W., Sklute, E.C., Dyar, M.D., & Cooper, R.F. (2017) Spectral properties of martian and other planetary glasses and their detection in remotely sensed data. Journal of Geophysical Research, 122, 249268.Google Scholar
Cariati, F., Erre, L., Gessa, C., Micera, G., & Piu, P. (1981) Water molecules and hydroxyl groups in montmorillonites as studied by near infrared spectroscopy. Clays and Clay Minerals, 29, 157159.CrossRefGoogle Scholar
Chapman, C.R. & Salisbury, J.W. (1973) Comparisons of meteorite and asteroid spectral reflectivities. Icarus, 19, 507522.Google Scholar
Cheek, L.C., Pieters, C.M., Dyar, M.D., & Milam, K.A. (2009) Revisiting plagioclase optical properties for lunar exploration. 40th Lunar Planet. Sci. Conf., Abstract #1928.Google Scholar
Clark, J.T., Bishop, J.L., Parente, M., Brown, A.J., & McKeown, N.K. (2008) Constraining sulfate abundances on Mars using CRISM spectra and laboratory mixtures. 39th Lunar Planet. Sci. Conf., Abstract #1540.Google Scholar
Clark, R.N. (1983) Spectral properties of mixtures of montmorillonite and dark carbon grains: Implications for remote sensing minerals containing chemically and physically adsorbed water. Journal of Geophysical Research, 88, 1063510644.Google Scholar
Clark, R.N. (1999) Spectroscopy of rocks and minerals, and principles of spectroscopy. In: Manual of remote sensing, 3: Remote sensing for the Earth sciences (Rencz, A.N., ed.). John Wiley & Sons, New York, 358.Google Scholar
Clark, R.N. & Roush, T.L. (1984) Reflectance spectroscopy: Quantitative analysis techniques for remote sensing applications. Journal of Geophysical Research, 89, 63296340.Google Scholar
Clark, R.N., King, T.V.V., Klejwa, M., & Swayze, G.A. (1990) High spectral resolution reflectance spectroscopy of minerals. Journal of Geophysical Research, 95, 1265312680.Google Scholar
Clark, R.N., Swayze, G.A., Livo, K.E., et al. (2003) Imaging spectroscopy: Earth and planetary remote sensing with the USGS Tetracorder and expert systems. Journal of Geophysical Research, 108, 5131, DOI:10.1029/2002JE001847.CrossRefGoogle Scholar
Cloutis, E.A. & Gaffey, M.J. (1991) Pyroxene spectroscopy revisited: Spectral-compositional correlations and relationships to geothermometry. Journal of Geophysical Research, 96, 2280922826.Google Scholar
Cloutis, E.A., Gaffey, M.J., Jackowski, T., & Reed, K. (1986) Calibration of phase abundance, composition, and particle size distribution for olivine-orthopyroxene mixtures from reflectance spectra. Journal of Geophysical Research, 91, 1164111653.CrossRefGoogle Scholar
Cloutis, E.A., Asher, P.M., & Mertzman, S.A. (2002) Spectral reflectance properties of zeolites and remote sensing implications. Journal of Geophysical Research, 107, 5067, DOI:10.1029/2000JE001467.Google Scholar
Cloutis, E.A., Sunshine, J.M., & Morris, R.V. (2004) Spectral reflectance-compositional properties of spinels and chromites: Implications for planetary remote sensing and geothermometry. Meteoritics and Planetary Science, 39, 545565.Google Scholar
Cloutis, E.A., Hawthorne, F.C., Mertzman, S.A., et al. (2006) Detection and discrimination of sulfate minerals using reflectance spectroscopy. Icarus, 184, 121157.Google Scholar
Cloutis, E.A., Craig, M.A., Kruzelecky, R.V., et al. (2008) Spectral reflectance properties of minerals exposed to simulated Mars surface conditions. Icarus, 195, 140168.Google Scholar
Cloutis, E.A., Hardersen, P.S., Bish, D.L., Bailey, D.T., Gaffey, M.J., & Craig, M.A. (2010a) Reflectance spectra of iron meteorites: Implications for spectral identification of their parent bodies. Meteoritics and Planetary Science, 45, 304332.Google Scholar
Cloutis, E.A., Hudon, P., Romanek, C.S., et al. (2010b) Spectral reflectance properties of ureilites. Meteoritics and Planetary Science, 45, 16681694.Google Scholar
Cloutis, E.A., Hiroi, T., Gaffey, M.J., Alexander, C.M.O.D., & Mann, P. (2011a) Spectral reflectance properties of carbonaceous chondrites: 1. CI chondrites. Icarus, 212, 180209.CrossRefGoogle Scholar
Cloutis, E.A., Hudon, P., Hiroi, T., Gaffey, M.J., & Mann, P. (2011b) Spectral reflectance properties of carbonaceous chondrites: 2. CM chondrites. Icarus, 216, 309346.Google Scholar
Cloutis, E.A., Hudon, P., Hiroi, T., & Gaffey, M.J. (2012a) Spectral reflectance properties of carbonaceous chondrites: 3. CR chondrites. Icarus, 217, 389407.Google Scholar
Cloutis, E.A., Hudon, P., Hiroi, T., & Gaffey, M.J. (2012b) Spectral reflectance properties of carbonaceous chondrites: 7. CK chondrites. Icarus, 221, 911924.Google Scholar
Cloutis, E.A., Hudon, P., Hiroi, T., Gaffey, M.J., & Mann, P. (2012c) Spectral reflectance properties of carbonaceous chondrites: 8. “Other” carbonaceous chondrites: CH, ungrouped, polymict, xenolithic inclusions, and R chondrites. Icarus, 221, 9841001.Google Scholar
Cloutis, E., Berg, B., Mann, P., & Applin, D. (2016) Reflectance spectroscopy of low atomic weight and Na-rich minerals: Borates, hydroxides, nitrates, nitrites, and peroxides. Icarus, 264, 2036.Google Scholar
Cornell, R.M. & Schwertmann, U. (2003) The iron oxides: Structure, properties, reactions, occurrences and uses, 2nd edn. Wiley-VCH, Weinheim.Google Scholar
Cotton, F.A. (1990) Chemical applications of group theory, 3rd edn. Wiley-Interscience, New York.Google Scholar
Crowley, J.K. (1991) Visible and near-infrared (0.4–2.5 μm) reflectance spectra of Playa evaporite minerals. Journal of Geophysical Research, 96, 1623116240.Google Scholar
Crowley, J.K., Williams, D.E., Hammarstrom, J.M., Piatak, N., Chou, I.-M. & Mars, J.C. (2003) Spectral reflectance properties (0.4–2.5 µm) of secondary Fe-oxide, Fe-hydroxide, and Fe-sulphate-hydrate minerals associated with sulphide-bearing mine wastes. Geochemistry: Exploration, Environment, Analysis, 3, 219228.Google Scholar
Cuadros, J., Michalski, J.R., Dekov, V., Bishop, J., Fiore, S., & Dyar, M.D. (2013) Crystal-chemistry of interstratified Mg/Fe-clay minerals from seafloor hydrothermal sites. Chemical Geology, 360361, 142158.Google Scholar
Dalton, J.B. (2003) Spectral behavior of hydrated sulfate salts: Implications for Europa Mission spectrometer design. Astrobiology, 3, 771784.CrossRefGoogle ScholarPubMed
Davis, A.C., Bishop, J.L., Veto, M., et al. (2014) Comparing VNIR and TIR spectra of clay-bearing rocks. 45th Lunar Planet. Sci. Conf., Abstract #2699.Google Scholar
De Angelis, S., Manzari, P., De Sanctis, M.C., Ammannito, E., & Di Iorio, T. (2016) VIS-IR study of brucite–clay–carbonate mixtures: Implications for Ceres surface composition. Icarus, 280, 315327.Google Scholar
Decarreau, A., Petit, S., Martin, F., Vieillard, P., & Joussein, E. (2008) Hydrothermal synthesis, between 75 and 150C, of high-charge ferric nontronites. Clays and Clay Mineral, 56, 322337.Google Scholar
Deer, W.A., Howie, R.A., & Zussman, J. (1992) An introduction to the rock-forming minerals. Longman, London.Google Scholar
Dyar, M.D., Sklute, E.C., Menzies, O.N., et al. (2009) Spectroscopic characteristics of synthetic olivine: An integrated multi-wavelength and multi-technique approach. American Mineralogist, 94, 883898.Google Scholar
Ehlmann, B.L., Mustard, J.F., & Poulet, F. (2009) Modeling modal mineralogy of laboratory mixtures of nontronite and mafic minerals from visible near-infrared spectra data. 40th Lunar Planet. Sci. Conf., Abstract #1771.Google Scholar
Ehlmann, B.L., Bish, D.L., Ruff, S.W., & Mustard, J.F. (2012) Mineralogy and chemistry of altered Icelandic basalts: Application to clay mineral detection and understanding aqueous environments on Mars. Journal of Geophysical Research, 117, E00J16, DOI:10.1029/2012JE004156.Google Scholar
Farrand, W.H. & Singer, R.B. (1992) Alteration of hydrovolcanic basaltic ash: Observations with visible and near-infrared spectrometry. Journal of Geophysical Research, 97, 1739317408.Google Scholar
Fernandez-Martinez, A., Timon, V., Roman-Ross, G., Cuello, G.J., Daniels, J.E., & Ayora, C. (2010) The structure of schwertmannite, a nanocrystalline iron oxyhydroxysulfate. American Mineralogist, 95, 13121322.Google Scholar
Fischer, E. & Pieters, C.M. (1993) The continuum slope of Mars: Bi-directional reflectance investigations and applications to Olympus Mons. Icarus, 102, 185202.Google Scholar
Fraeman, A.A., Ehlmann, B.L., Northwood-Smith, G.W.D., Liu, Y., Wadhwa, M., & Greenberger, R.N. (2016) Using VSWIR microimaging spectroscopy to explore the mineralogical diversity of HED meteorites. 8th Workshop on Hyperspectral Image and Signal Processing: Evolution in Remote Sensing (WHISPERS), 1–5.Google Scholar
Gaffey, M.J. (1976) Spectral reflectance characteristics of the meteorite classes. Journal of Geophysical Research, 81, 905920.Google Scholar
Gaffey, S.J. (1987) Spectral reflectance of carbonate minerals in the visible and near infared (0.35–2.55 µm): Anhydrous carbonate minerals. Journal of Geophysical Research, 92, 14291440.Google Scholar
Gaffey, S.J., McFadden, L.A., Nash, D. & Pieters, C.M. (1993) Ultraviolet, visible, and near-infrared reflectance spectroscopy: Laboratory spectra of geologic materials. In: Remote geochemical analysis: Elemental and mineralogical composition (Pieters, C.M & Englert, P.A.J., eds.). Cambridge University Press, Cambridge, 4377.Google Scholar
Gates, W.P. (2005) Infrared spectroscopy and the chemistry of dioctahedral smectites. In: The application of vibrational spectroscopy to clay minerals and layered double hydroxides (Kloprogge, J.T., ed.). Clay Minerals Society, Aurora, CO, 125168.Google Scholar
Goryniuk, M.C., Rivard, B.A., & Jones, B. (2004) The reflectance spectra of opal-A (0.5–25 μm) from the Taupo Volcanic Zone: Spectra that may identify hydrothermal systems on planetary surfaces. Geophysical Research Letters, 31, DOI:10.1029/2004GL021481.Google Scholar
Hanley, J., Dalton, J.B., Chevrier, V.F., Jamieson, C.S., & Barrows, R.S. (2014) Reflectance spectra of hydrated chlorine salts: The effect of temperature with implications for Europa. Journal of Geophysical Research, 119, 23702377.Google Scholar
Hanley, J., Chevrier, V.F., Barrows, R.S., Swaffer, C., & Altheide, T.S. (2015) Near- and mid-infrared reflectance spectra of hydrated oxychlorine salts with implications for Mars. Journal of Geophysical Research, 120, 14151426.Google Scholar
Hapke, B. (1993) Theory of reflectance and emittance spectroscopy. Cambridge University Press, Cambridge.Google Scholar
Harner, P.L. & Gilmore, M.S. (2015) Visible–near infrared spectra of hydrous carbonates, with implications for the detection of carbonates in hyperspectral data of Mars. Icarus, 250, 204214.Google Scholar
Herzberg, G. (1945) Molecular spectra and molecular structure. II. Infrared and Raman spectra of polyatomic molecules. D. Van Nostrand, New York.Google Scholar
Hiroi, T. & Pieters, C.M. (1994) Estimation of grain sizes and mixing ratios of fine powder mixtures of common geologic minerals. Journal of Geophysical Research, 99, 10,86710,879.Google Scholar
Hiroi, T., Miyamoto, M., Mikouchi, T., & Ueda, Y. (2005) Visible and near-infrared reflectance spectroscopy of the Yamato 980459 meteorite in comparison with some shergottites. Antarctic Metorite Research, 18, 8395.Google Scholar
Hiroi, T., Jenniskens, P.M., Bishop, J.L., Shatir, T.S.M., Kudoda, A.M., & Shaddad, M.H. (2010) Bidirectional visible-NIR and biconical FT-IR reflectance spectra of Almahata Sitta meteorite samples. Meteoritics and Planetary Science, 45, 18361845.Google Scholar
Honma, A., Bishop, J.L., McKeown, N.K., Brown, A.J., & Parente, M. (2008) Constraining phyllosilicate abundances on Mars using CRISM spectra and laboratory mixtures. 39th Lunar Planet. Sci. Conf., Abstract #1457.Google Scholar
Huheey, J.E., Keiter, E.A., & Keiter, R.I. (1993) lnorganic chemistry: Principles of structure and reactivity, 4th edn. HarperCollins, New York.Google Scholar
Hunt, G.R. & Ashley, R.P. (1979) Spectra of altered rocks in the visible and near infrared. Economic Geology, 74, 16131629.Google Scholar
Hunt, G.R. & Salisbury, J.W. (1970) Visible and near-infrared spectra of minerals and rocks: 1. Silicate minerals. Modern Geology, 1, 283300.Google Scholar
Hunt, G.R. & Salisbury, J.W. (1971) Visible and near-infrared spectra of minerals and rocks: II. Carbonates. Modern Geology, 2, 2330.Google Scholar
Hunt, G.R., Salisbury, J.W., & Lenhoff, C.J. (1971a) Visible and near-infrared spectra of minerals and rocks: III. Oxides and hydroxides. Modern Geology, 2, 195205.Google Scholar
Hunt, G.R., Salisbury, J.W., & Lenhoff, C.J. (1971b) Visible and near-infrared spectra of minerals and rocks: IV. Sulphides and sulphates. Modern Geology, 3, 114.Google Scholar
Isaacson, P.J., Liu, Y., Patchen, A., Pieters, C.M., & Taylor, L.A. (2009) Integrated analyses of Lunar meteorites: Expanded data for lunar ground truth. 40th Lunar Planet. Sci. Conf., Abstract #2119.Google Scholar
Isaacson, P.J., Liu, Y., Patchen, A.D., Pieters, C.M., & Taylor, L.A. (2010) Spectroscopy of Lunar meteorites as constraints for ground truth: Expanded sample collection diversity. 41st Lunar Planet. Sci. Conf., Abstract #1927.Google Scholar
Isaacson, P.J., Basu Sarbadhikari, A., Pieters, C.M., et al. (2011) The lunar rock and mineral characterization consortium: Deconstruction and integrated mineralogical, petrologic, and spectroscopic analyses of mare basalts. Meteoritics and Planetary Science, 46, 228251.CrossRefGoogle Scholar
Isaacson, P.J., Klima, R.L., Sunshine, J.M., et al. (2014) Visible to near-infrared optical properties of pure synthetic olivine across the olivine solid solution. American Mineralogist, 99, 467478.Google Scholar
Jenniskens, P., Shaddad, M.H., Numan, D., et al. (2009) The impact and recovery of asteroid 2008 TC3. Nature, 458, 485488.Google Scholar
Jeute, T.J., Baker, L.L., Abidin, Z., Bishop, J.L., & Rampe, E.B. (2017) Characterizing nanophase materials on Mars: Spectroscopic studies of allophane and imogolite. 48th Lunar Planet. Sci. Conf., Abstract #2738.Google Scholar
Johnson, J.R. & Hörz, F. (2003) Visible/near-infrared spectra of experimentally shocked plagioclase feldspars. Journal of Geophysical Research, 108, 5120, DOI:10.1029/2003JE002127, E11.Google Scholar
King, S.J., Bishop, J.L., Fenton, L.K., Lafuente, B., Garcia, G.C., & Horgan, B.H. (2013) VNIR reflectance spectra of gypsum mixtures for comparison with White Sands National Monument, New Mexico (WSNM) dune samples as an analog study of the Olympia Undae region of Mars. AGU Fall Meeting, Abstract #P23C-1800.Google Scholar
King, T.V.V. & Clark, R.N. (1989) Spectral characteristics of chlorites and Mg-serpentines using high-resolution reflectance spectroscopy. Journal of Geophysical Research, 94, 13,99714,008.Google Scholar
Klima, R.L., Pieters, C.M., & Dyar, M.D. (2007) Spectroscopy of synthetic Mg-Fe pyroxenes I: Spin-allowed and spin-forbidden crystal field bands in the visible and near-infrared. Meteoritics and Planetary Science, 42, 235253.Google Scholar
Klima, R.L., Pieters, C.M., & Dyar, M.D. (2008) Characterization of the 1.2 micrometer M1 pyroxene band: Extracting cooling history from near-IR spectra of pyroxenes and pyroxene-dominated rocks. Meteoritics and Planetary Science, 43, 15911604.Google Scholar
Klima, R.L., Dyar, M.D., & Pieters, C.M. (2011) Near-infrared spectra of clinopyroxenes: effects of calcium content and crystal structure. Meteoritics and Planetary Science, 46, 379395.Google Scholar
Lane, M.D. & Christensen, P.R. (1997) Thermal infrared emission spectroscopy of anhydrous carbonates. Journal of Geophysical Research, 102, 2558125592.Google Scholar
Lane, M.D., Dyar, M.D., & Bishop, J.L. (2007) Spectra of phosphate minerals as obtained by visible-near infrared reflectance, thermal infrared emission, and Mössbauer laboratory analyses. 38th Lunar Planet. Sci. Conf., Abstract #2210.Google Scholar
Lane, M.D., Bishop, J.L., Dyar, M.D., et al. (2015) Mid-infrared emission spectroscopy and visible/near-infrared reflectance spectroscopy of Fe-sulfate minerals. American Mineralogist, 100, 6682.Google Scholar
Lapotre, M.G.A., Ehlmann, B.L., & Minson, S.E. (2017) A probabilistic approach to remote compositional analysis of planetary surfaces. Journal of Geophysical Research, 122, 9831009.Google Scholar
Lauretta, D.S. & McSween, H.Y. Jr. (2006) Meteorites and the early solar system II. The University of Arizona Press, Tucson, AZ.Google Scholar
Lin, T.J., Ver Eecke, H.C., Breves, E.A., et al. (2016) Linkages between mineralogy, fluid chemistry, and microbial communities within hydrothermal chimneys from the Endeavour Segment, Juan de Fuca Ridge. Geochemistry, Geophysics, Geosystems, 17, 300323.Google Scholar
McFadden, L.A. & Cline, T.P. (2005) Spectral reflectance of martian meteorites: Spectral signatures as a template for locating source region on Mars. Meteoritics and Planetary Science, 40, 151172.Google Scholar
McFadden, L.A., Gaffey, M.J., & Takeda, H. (1980) Reflectance spectra of some newly found, unusual meteorites and their bearing on the surface mineralogy of asteroids. Proceedings of the 13th Lunar and Planetary Symposium, Tokyo, 273–280.Google Scholar
McKeown, N.K., Bishop, J.L., Cuadros, J., et al. (2011) Interpretation of reflectance spectra of clay mineral-silica mixtures: Implications for martian clay mineralogy at Mawrth Vallis. Clays and Clay Mineral, 59, 400415.Google Scholar
Milliken, R.E. & Mustard, J.F. (2005) Quantifying absolute water content of minerals using near-infrared reflectance spectroscopy. Journal of Geophysical Research, 110, E12001, DOI:10.1029/2005JE002534.Google Scholar
Milliken, R.E., Swayze, G.A., Arvidson, R.E., et al. (2008) Opaline silica in young deposits on Mars. Geology, 36, 847850.Google Scholar
Minitti, M.E. & Rutherford, M.J. (2000) Genesis of the Mars Pathfinder “sulfur-free” rock from SNC parental liquids. Geochimica Cosmochimica Acta, 64, 25352547.CrossRefGoogle Scholar
Minitti, M.E., Mustard, J.F., & Rutherford, M.J. (2002) The effects of glass content and oxidation on the spectra of SNC-like basalts: Application to Mars remote sensing. Journal of Geophysical Research, 107(E5), DOI:10.1029/2001JE001518.Google Scholar
Minitti, M.E., Weitz, C.M., Lane, M.D., & Bishop, J.L. (2007) Morphology, chemistry, and spectral properties of Hawaiian rock coatings and implications for Mars. Journal of Geophysical Research, 112, E05015, DOI: 10.1029/2006JE002839.Google Scholar
Moroz, L., Schade, U., & Wäsch, R. (2000) Reflectance spectra of olivine-orthopyroxene-bearing assemblages at decreased temperatures: Implications for remote sensing of asteroids. Icarus, 147, 7993.Google Scholar
Morris, R.V., Lauer, H.V. Jr., Lawson, C.A., Gibson, E.K. Jr., Nace, G.A., & Stewart, C. (1985) Spectral and other physicochemical properties of submicron powders of hematite (a-Fe2O3), maghemite (g-Fe2O3), magnetite (Fe3O4), goethite (a-FeOOH), and lepidocrocite (g-FeOOH). Journal of Geophysical Research, 90, 31263144.Google Scholar
Morris, R.V., Agresti, D.G., Lauer, H.V. Jr., Newcomb, J.A., Shelfer, T.D., & Murali, A.V. (1989) Evidence for pigmentary hematite on Mars based on optical, magnetic and Mössbauer studies of superparamagnetic (nanocrystalline) hematite. Journal of Geophysical Research, 94, 27602778.Google Scholar
Morris, R.V., Gooding, J.L., Lauer, H.V. Jr., & Singer, R.B. (1990) Origins of Marslike spectral and magnetic properties of a Hawaiian palagonitic soil. Journal of Geophysical Research, 95, 14,42714,434.Google Scholar
Morris, R.V., Schulze, D.G., Lauer, H.V. Jr., Agresti, D.G., & Shelfer, T.D. (1992) Reflectivity (visible and near IR), Mössbauer, static magnetic, and X ray diffraction properties of aluminum-substituted hematites. Journal of Geophysical Research, 97, 1025710266.Google Scholar
Morris, R.V., Golden, D.C., Bell, J.F. III, & Lauer, H.V. Jr. (1995) Hematite, pyroxene, and phyllosilicates on Mars: Implications from oxidized impact melt rocks from Manicouagan crater, Quebec, Canada. Journal of Geophysical Research, 100, 53195328.Google Scholar
Morris, R.V., Golden, D.C., & Bell, J.F. III (1997) Low-temperature reflectivity spectra of red hematite and the color of Mars. Journal of Geophysical Research, 102, 91259133.Google Scholar
Morris, R.V., Golden, D.C., Shelfer, T.D., & Lauer, H.V. Jr. (1998) Lepidocrocite to maghemite to hematite: A pathway to magnetic and hematitic martian soil. Meteoritics and Planetary Science, 33, 743751.Google Scholar
Morris, R.V., Graff, T.G., Mertzman, S.A., Lane, M.D., & Christensen, P.R. (2003) Palagonitic (not Andesitic) Mars: Evidence from thermal emission and VNIR spectra of Palagonitic alteration rinds on basaltic rock. 6th Int. Conf. on Mars, Abstract #3211.Google Scholar
Mustard, J.F. (1992) Chemical analysis of actinolite from reflectance spectra. American Mineralogist, 77, 345358.Google Scholar
Mustard, J.F. & Hays, J.E. (1997) Effects of hyperfine particles on reflectance spectra from 0.3 to 25 µm. Icarus, 125, 145163.Google Scholar
Mustard, J.F. & Pieters, C.M. (1987) Abundance and distribution of ultramafic microbreccia in moses rock dike: Quantitative application of mapping spectroscopy. Journal of Geophysical Research, 92, 1037610390.Google Scholar
Mustard, J.F. & Pieters, C.M. (1989) Photometric phase functions of common geologic minerals and applications to quantitative analysis of mineral mixture reflectance spectra. Journal of Geophysical Research, 94, 1361913634.Google Scholar
Mustard, J.F., Sunshine, J.M., Pieters, C.M., Hoppin, A., & Pratt, S.F. (1993) From minerals to rocks: Toward modeling lithologies with remote sensing. 24th Lunar Planet. Sci. Conf., Abstract, 1041–1042.Google Scholar
Mustard, J.F., Murchie, S.L., Erard, S., & Sunshine, J.M. (1997) In situ compositions of martian volcanics: Implications for the mantle. Journal of Geophysical Research, 102, 25,60525,615.Google Scholar
Nash, D.B. & Conel, J.E. (1974) Spectral reflectance systematics for mixtures of powdered hypersthene, labradorite, and ilmenite. Journal of Geophysical Research, 79, 16151621.Google Scholar
Nwaodua, E.C., Ortiz, J.D., & Griffith, E.M. (2014) Diffuse spectral reflectance of surficial sediments indicates sedimentary environments on the shelves of the Bering Sea and western Arctic. Marine Geology, 355, 218233.Google Scholar
Ody, A., Poulet, F., Quantin, C., Bibring, J.P., Bishop, J.L, & Dyar, M.D. (2015) Candidates source regions of martian meteorites as identified by OMEGA/MEx. Icarus, 258, 366383.Google Scholar
Orenberg, J. & Handy, J. (1992) Reflectance spectroscopy of palagonite and iron-rich montmorillonite clay mixtures: Implications for the surface composition of Mars. Icarus, 96, 219225.Google Scholar
Papike, J.J. (1989) Planetary materials. In: Reviews in mineralogy, 36. Mineralogical Society of America, Chantilly, VA.Google Scholar
Parente, M., Makarewicz, H.D., & Bishop, J.L. (2011) Decomposition of mineral absorption bands using nonlinear least squares curve fitting: Application to martian meteorites and CRISM data. Planetary and Space Science, 59, 423442.Google Scholar
Parfitt, R.L. (2009) Allophane and imogolite: Role in soil biogeochemical processes. Clay Minerals, 44, 135155.Google Scholar
Petit, S., Madejova, J., Decarreau, A., & Martin, F. (1999) Characterization of octahedral subsitutions in kaolinites using near infrared spectroscopy. Clays and Clay Minerals, 47, 103108.CrossRefGoogle Scholar
Petit, S., Decarreau, A., Martin, F., & Buchet, R. (2004a) Refined relationship between the position of the fundamental OH stretching and the first overtones for clays. Physics and Chemistry of Minerals, 31, 585592.Google Scholar
Petit, S., Martin, F., Wiewiora, A., de Parseval, P., & Decarreau, A. (2004b) Crystal-chemistry of talc: A near infrared (NIR) spectroscopy study. American Mineralogist, 89, 319326.Google Scholar
Pieters, C.M. (1983) Strength of mineral absorption features in the transmitted component of near-infrared reflected light: First results from RELAB. Journal of Geophysical Research, 88, 95349544.Google Scholar
Pieters, C.M. (1996) Plagioclase and maskelynite diagnostic features. 27th Lunar Planet. Sci. Conf., Abstract #1031.Google Scholar
Pieters, C.M. & Hiroi, T. (2004) RELAB (Reflectance Experiment Laboratory): A NASA multiuser spectroscopy facility. 35th Lunar Planet. Sci. Conf., Abstract #1720.Google Scholar
Pieters, C.M. & Mustard, J.F. (1988) Exploration of crustal/mantle material for the Earth and Moon using reflectance spectroscopy. Remote Sensing Environment, 24, 151178.Google Scholar
Pieters, C.M., Hawke, B.R., Gaffey, M., & McFadden, L.A. (1983) Possible lunar source areas of meteorite ALHA81005: Geochemical remote sensing information. Geophysical Research Letters, 10, 813816.Google Scholar
Pieters, C.M., Mustard, J.F., Pratt, S.F., Sunshine, J.M., & Hoppin, A. (1993) Visible-infrared properties of controlled laboratory soils. 24th Lunar Planet. Sci. Conf., Abstract, 1147–1148.Google Scholar
Pieters, C.M., Mustard, J.F., & Sunshine, J.M. (1996) Quantitative mineral analyses of planetary surfaces using reflectance spectroscopy. In: Mineral spectroscopy: A tribute to Roger G. Burns (Dyar, M.D., McCammon, C., & Schaefer, M.W., eds.). The Geochemical Society, Houston, TX, 307325.Google Scholar
Pieters, C.M., Klima, R.L., Hiroi, T., et al. (2008) The origin of brown olivine in martian dunite NWA 2737: Integrated spectroscopic analyses of brown olivine. Journal of Geophysical Research, 113, E06004, DOI:10.1029/2007JE002939.Google Scholar
Post, J.L. (1984) Saponite from near Ballarat, California. Clays and Clay Minerals, 32, 147152.Google Scholar
Post, J.L. & Noble, P.N. (1993) The near-infrared combination band frequencies of dioctahedral smectites, micas, and illites. Clays and Clay Minerals, 41, 639644.Google Scholar
Post, J.L., Cupp, B.L., & Madsen, F.T. (1997) Beidellite and associated clays from the DeLamar mine and Florida mountain area, Idaho. Clays and Clay Mineral, 45, 240250.Google Scholar
Powers, D.A., Rossman, G.R., Schugar, H.J., & Gray, H.B. (1975) Magnetic behavior and infrared spectra of jarosite, basic iron sulfate, and their chromate analogs. Journal of Solid State Chemistry, 13, 113.Google Scholar
Rice, M.S., Cloutis, E.A., Bell, J.F. III, et al. (2013) Reflectance spectra diversity of silica-rich materials: Sensitivity to environment and implications for detections on Mars. Icarus, 223, 499533.Google Scholar
Ross, S.D. (1974) Phosphates and Other Oxyanions of Group V. In: The infrared spectra of minerals (Farmer, V.C., ed.). The Mineralogical Society, London, 383422.Google Scholar
Roush, T.L., Bishop, J.L., Brown, A.J., Blake, D.F., & Bristow, T.F. (2015) Laboratory reflectance spectra of clay minerals mixed with Mars analog materials: Toward enabling quantitative clay abundances from Mars spectra. Icarus, 258, 454466.Google Scholar
Ruesch, O., Hiesinger, H., Cloutis, E., et al. (2015) Near infrared spectroscopy of HED meteorites: Effects of viewing geometry and compositional variations. Icarus, 258, 384401.Google Scholar
Salisbury, J.W. & Hunt, G.R. (1974) Meteorite spectra and weathering. Journal of Geophysical Research, 79, 4493–4441.Google Scholar
Salisbury, J.W., D’Aria, D.M., & Jarosewich, E. (1991) Midinfrared (2.5–13.5 µm) reflectance spectra of powdered stony meteorites. Icarus, 92, 280297.Google Scholar
Saper, L. & Bishop, J.L. (2011) Reflectance spectroscopy of nontronite and ripidolite mineral mixtures in context of phyllosilicate unit composition at Mawrth Vallis. 42nd Lunar Planet. Sci. Conf., Abstract #2029.Google Scholar
Schade, U. & Wäsch, R. (1999) Near-infrared reflectance spectra from bulk samples of the two martian meteorites Zagami and Nakhla. Meteoritics and Planetary Science, 34, 417424.Google Scholar
Schade, U., Wäsch, R., & Moroz, L. (2004) Near-infrared reflectance spectroscopy of Ca-rich clinopyroxenes and prospects for remote spectral characterization of planetary surfaces. Icarus, 168, 8092.Google Scholar
Scheinost, A.C., Chavernas, A., Barrón, V., & Torrent, J. (1998) Use and limitations of second-derivative diffuse reflectance spectroscopy in the visible to near-infrared range to identify and quantify Fe oxide minerals in soils. Clays and Clay Minerals, 46, 528536.Google Scholar
Sherman, D.M. & Waite, T.D. (1985) Electronic spectra of Fe3+ oxides and oxide hydroxides in the near IR to near UV. American Mineralogist, 70, 12621269.Google Scholar
Sherman, D.M., Burns, R.G., & Burns, V.M. (1982) Spectral characteristics of the iron oxides with application to the martian bright region mineralogy. Journal of Geophysical Research, 87, 1016910180.Google Scholar
Shkuratov, Y.G. & Grynko, Y.S. (2005) Light scattering by media composed of semitransparent particles of different shapes in ray optics approximation: Consequences for spectroscopy, photometry, and polarimetry of planetary regoliths. Icarus, 173, 1628.Google Scholar
Singer, R.B. (1981) Near-infrared spectral reflectance of mineral mixtures: Systematic combinations of pyroxenes, olivine, and iron oxides. Journal of Geophysical Research, 86, 79677982.Google Scholar
Singer, R.B. & Roush, T.L. (1983) Spectral reflectance properties of particulate weathered coatings on rocks: Laboratory modeling and applicability to Mars. 14th Lunar Planet. Sci. Conf., Abstract, 708–709.Google Scholar
Singer, R.B. & Roush, T.L. (1985) Effects of temperature on remotely sensed mineral absorption features. Journal of Geophysical Research, 90, 12,43412,444.Google Scholar
Song, X. & Boily, J.-F. (2012) Variable hydrogen bond strength in akaganéite. The Journal of Physical Chemistry C, 116, 23032312.Google Scholar
Song, X. & Boily, J.-F. (2013) Water vapor diffusion into a nanostructured iron oxyhydroxide. Inorganic Chemistry, 52, 71077113.Google Scholar
Sugihara, T., Ohtake, M., Owada, A., Ishii, T., Otsuki, M., & Takeda, H. (2004) Petrology and reflectance spectroscopy of lunar meteorite Yamato 981031: Implications for the source region of the meteorite and remote-sensing spectroscopy. Antarctic Meteorite Research, 17, 209230.Google Scholar
Sun, V.Z., Milliken, R.E., & Robertson, K.M. (2016) Hydrated silica on Mars: Relating geologic setting to degree of hydration, crystallinity, and maturity through coupled orbital and laboratory studies. 47th Lunar Planet. Sci. Conf., Abstract #2416.Google Scholar
Sunshine, J.M. & Pieters, C.M. (1993) Estimating modal abundances from the spectra of natural and laboratory pyroxene mixtures using the Modified Gaussian Model. Journal of Geophysical Research, 98, 90759087.Google Scholar
Sunshine, J.M. & Pieters, C.M. (1998) Determining the composition of olivine from reflectance spectroscopy. Journal of Geophysical Research, 103, 13,67513,688.Google Scholar
Sunshine, J.M., Pieters, C.M., & Pratt, S.F. (1990) Deconvolution of mineral absorption bands: An improved approach. Journal of Geophysical Research, 95, 69556966.Google Scholar
Sunshine, J.M., McFadden, L.A., & Pieters, C.M. (1993) Reflectance spectra of the Elephant Moraine A79001 meteorite: Implications for remote sensing of planetary bodies. Icarus, 105, 7991.Google Scholar
Sunshine, J.M., Bus, S.J., McCoy, T.J., Burbine, T.H., Corrigan, C.M., & Binzel, P. (2004) High-calcium pyroxene as an indicator of igneous differentiation in asteroids and meteorites. Meteoritics and Planetary Science, 39, 13431357.Google Scholar
Sunshine, J.M., Bus, S.J., Corrigan, C.M., McCoy, T.J., & Burbine, T.H. (2007) Olivine-dominated asteroids and meteorites: Dinstinguishing nebular and igneous histories. Meteoritics and Planetary Science, 42, 155170.Google Scholar
Swayze, G.A., Lowers, H.A., Benzel, W.M., et al. (2018) Characterizing the source of potentially asbestos-bearing commercial vermiculite insulation using in situ IR spectroscopy. American Mineralogist, 103, 517549.Google Scholar
Tarantola, A. & Valette, B. (1982) Generalized nonlinear inverse problems solved using the least squares criterion. Reviews of Geophysics and Space Physics, 20, 219232.Google Scholar
van Olphen, H. & Fripiat, J.J. (1979) Data handbook for clay materials and other non-metallic minerals. Pergamon Press, Oxford.Google Scholar
Wang, F., Bowen, B.B., Seo, J.-H., & Michalski, G. (2018) Laboratory and field characterization of visible to near-infrared spectral reflectance of nitrate minerals from the Atacama Desert, Chile, and implications for Mars. American Mineralogist, 103, 197206.Google Scholar
Wasson, J.T. (1985) Meteorites: Their record of early Solar System history. W.H. Freeman, New York.Google Scholar
Weir, C.E. & Lippincott, E.R. (1961) Infrared studies of aragonite, calcite, and vaterite type structures in the borates, carbonates, and nitrates. Journal of Research of the National Bureau of Standards A: Physics and Chemistry, 65A, 173183.Google Scholar

Save book to Kindle

To save this book to your Kindle, first ensure coreplatform@cambridge.org is added to your Approved Personal Document E-mail List under your Personal Document Settings on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part of your Kindle email address below. Find out more about saving to your Kindle.

Note you can select to save to either the @free.kindle.com or @kindle.com variations. ‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi. ‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.

Find out more about the Kindle Personal Document Service.

Available formats
×

Save book to Dropbox

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Dropbox.

Available formats
×

Save book to Google Drive

To save content items to your account, please confirm that you agree to abide by our usage policies. If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account. Find out more about saving content to Google Drive.

Available formats
×