TY - JOUR
T1 - Spectral reflectance (0.35–2.5 µm) properties of garnets
T2 - Implications for remote sensing detection and characterization
AU - Izawa, M. R.M.
AU - Cloutis, E. A.
AU - Rhind, T.
AU - Mertzman, S. A.
AU - Poitras, Jordan
AU - Applin, Daniel M.
AU - Mann, P.
N1 - Funding Information:
The University of Winnipeg's Planetary Spectrophotometer Facility was established with funding from the Canada Foundation for Innovation , the Manitoba Research Innovations Fund, the Natural Sciences and Engineering Research Council of Canada ( NSERC ), the Canadian Space Agency ( CSA ), and the University of Winnipeg ( UW ), whose support is gratefully acknowledged. This study was supported by research grants from NSERC , CSA , and UW . We thank Josep M. Trigo-Rodríguez and an anonymous reviewer for very helpful comments which led to many improvements in this manuscript. We also wish to thank Dr. Takahiro Hiroi and Dr. Carlé Pieters of the NASA-supported RELAB spectrometer facility at Brown University for acquiring reflectance spectra of a number of the samples used in this study. MRMI gratefully acknowledges funding from the NSERC CREATE Canadian Astrobiology Training Program and the Mineralogical Association of Canada.
Publisher Copyright:
© 2017 Elsevier Inc.
PY - 2018/1/15
Y1 - 2018/1/15
N2 - The utility of spectral reflectance for identification of the main end-member garnets: almandine (Fe2+ 3Al2Si3O12), andradite (Ca3Fe3+ 2Si3O12), grossular (Ca3Al2Si3O12), pyrope (Mg3Al2Si3O12), spessartine (Mn2+ 3Al2Si3O12), and uvarovite (Ca3Cr3+ 2Si3O12) was studied using a suite of 60 garnet samples. Compositional and structural data for the samples, along with previous studies, were used to elucidate the mechanisms that control their spectral reflectance properties. Various cation substitutions result in different spectral properties that can be determine the presence of various optically-active cations and help differentiate between garnet types. It was found that different wavelength regions are sensitive to different compositional and structural properties of garnets. Crystal-field absorptions involving Fe2+ and/or Fe3+ are responsible for the majority of spectral features in the garnet minerals examined here. There can also be spectral features associated with other cations and mechanisms, such as Fe2 +–Fe3+ and Fe2 +–Ti4+ intervalence charge transfers. The visible wavelength region is useful for identifying the presence of various cations, in particular, Fe (and its oxidation state), Ti4+, Mn2+, and Cr3+. In the case of andradite, spessartine and uvarovite, the visible region absorption bands are characteristic of these garnets in the sense that they are associated with the major cation that distinguishes each: [6]Fe3+ for andradite, [8]Mn2+ for spessartine, and [6]Cr3+ for uvarovite. For grossular, the presence of small amounts of Fe3+ leads to absorption bands near 0.370 and 0.435 µm. These bands are also seen in pyrope–almandine spectra, which also commonly have additional absorption bands, due to the presence of Fe2+. The common presence of Fe2+ in the dodecahedral site of natural garnets gives rise to three Fe2+ spin-allowed absorption bands in the 1.3, 1.7, and 2.3 µm regions, providing a strong spectral fingerprint for all Fe2+-bearing garnets studied here. Garnets containing Mn2+ have additional visible (∼0.41 µm) spectral features due to [8]Mn2+. Garnets containing Cr3+, exhibits two strong absorption bands near ∼0.7 µm due to spin-forbidden [6]Cr3+ transitions, as well as [6]Cr3+ spin-allowed features near 0.4–0.41 µm and 0.56–0.62 µm, and [6]Cr3+ spin-allowed transitions between 0.41 and 0.68 µm. Common silicate garnet spectra, in summary, are distinct from many other rock-forming silicates and can be spectrally distinct from one garnet species to another. Iron dominates the spectral properties of garnets, and the crystallographic site and oxidation state of the iron both affect garnet reflectance spectra.
AB - The utility of spectral reflectance for identification of the main end-member garnets: almandine (Fe2+ 3Al2Si3O12), andradite (Ca3Fe3+ 2Si3O12), grossular (Ca3Al2Si3O12), pyrope (Mg3Al2Si3O12), spessartine (Mn2+ 3Al2Si3O12), and uvarovite (Ca3Cr3+ 2Si3O12) was studied using a suite of 60 garnet samples. Compositional and structural data for the samples, along with previous studies, were used to elucidate the mechanisms that control their spectral reflectance properties. Various cation substitutions result in different spectral properties that can be determine the presence of various optically-active cations and help differentiate between garnet types. It was found that different wavelength regions are sensitive to different compositional and structural properties of garnets. Crystal-field absorptions involving Fe2+ and/or Fe3+ are responsible for the majority of spectral features in the garnet minerals examined here. There can also be spectral features associated with other cations and mechanisms, such as Fe2 +–Fe3+ and Fe2 +–Ti4+ intervalence charge transfers. The visible wavelength region is useful for identifying the presence of various cations, in particular, Fe (and its oxidation state), Ti4+, Mn2+, and Cr3+. In the case of andradite, spessartine and uvarovite, the visible region absorption bands are characteristic of these garnets in the sense that they are associated with the major cation that distinguishes each: [6]Fe3+ for andradite, [8]Mn2+ for spessartine, and [6]Cr3+ for uvarovite. For grossular, the presence of small amounts of Fe3+ leads to absorption bands near 0.370 and 0.435 µm. These bands are also seen in pyrope–almandine spectra, which also commonly have additional absorption bands, due to the presence of Fe2+. The common presence of Fe2+ in the dodecahedral site of natural garnets gives rise to three Fe2+ spin-allowed absorption bands in the 1.3, 1.7, and 2.3 µm regions, providing a strong spectral fingerprint for all Fe2+-bearing garnets studied here. Garnets containing Mn2+ have additional visible (∼0.41 µm) spectral features due to [8]Mn2+. Garnets containing Cr3+, exhibits two strong absorption bands near ∼0.7 µm due to spin-forbidden [6]Cr3+ transitions, as well as [6]Cr3+ spin-allowed features near 0.4–0.41 µm and 0.56–0.62 µm, and [6]Cr3+ spin-allowed transitions between 0.41 and 0.68 µm. Common silicate garnet spectra, in summary, are distinct from many other rock-forming silicates and can be spectrally distinct from one garnet species to another. Iron dominates the spectral properties of garnets, and the crystallographic site and oxidation state of the iron both affect garnet reflectance spectra.
KW - Garnet
KW - Reflectance spectroscopy
KW - Remote sensing
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U2 - 10.1016/j.icarus.2017.09.005
DO - 10.1016/j.icarus.2017.09.005
M3 - Article
AN - SCOPUS:85032728526
SN - 0019-1035
VL - 300
SP - 392
EP - 410
JO - Icarus
JF - Icarus
ER -