The influence of octahedral and tetrahedral cation substitution on the structure of smectites and serpentines as observed through infrared spectroscopy

By Janice L. Bishop, E. Murad, Melinda Darby Dyar. Clay minerals, 2002

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Mineralogical constraints on the high-silica martian surface component observed by TES (2005, methodology): “We draw an analogy between transmission spectral features, and the mineralogical interpretations made from them in previous work (Stubican and Roy, 1961; Farmer, 1974; Madejova and Komadel, 2001; Bishop, 2002; Bishop et al., 2002b), to the emission spectral features of clay minerals.”
Hydrous mineralogy of CM and CI chondrites from infrared spectroscopy and their relationship with low albedo asteroids (2010, background): “There is an abundant literature in the case of clay minerals (Madejova et al., 1994; Bishop et al., 2002a, 2002b), but little is known on the effect of the OH bounding cation on the IR spectra of serpentine.”
The influence of structural Fe, Al and Mg on the infrared OH bands in spectra of dioctahedral smectites (2002, background): “3 in Bishop et al., 2002, this issue).”
Reflectance and emission spectroscopy study of four groups of phyllosilicates: smectites, kaolinite-serpentines, chlorites and micas (2008, methodology): “…mm and no water band near 1.9 mm, while montmoril lonite has a single band near 2.21 2.22 mm (which varies considerably with AlFe-Mg abundance; see Bishop et al., 2002b) and a strong water band at 1.92 mm. Kaolinite has the greatest Al, smallest Fe and smallest Mg concentrations of all the…”