The influence of structural Fe, Al and Mg on the infrared OH bands in spectra of dioctahedral smectites

By Janice L. Bishop, J. Madejová, P. Komadel, H. Fröschl. Clay minerals, 2002

201 citations recorded by the source corpus.

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

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 octahedral and tetrahedral cation substitution on the structure of smectites and serpentines as observed through infrared spectroscopy (2002, methodology): “Phyllosilicates and iron oxides/oxyhydroxides are thought to be components of Martian surface material because they are alteration products of basalts that are ubiquitous on the Red Planet (e.g. Bell, 1996; Bishop & Murad, 1996; McSween & Keil, 2000; Bishop et al., 2002).”
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…”