Reflectance and emission spectroscopy study of four groups of phyllosilicates: smectites, kaolinite-serpentines, chlorites and micas

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Characterization of phyllosilicates observed in the central Mawrth Vallis region, Mars, their potential formational processes, and implications for past climate (2009, background): “A ferrous mica such as celadonite or glauconite or a chlorite such as chamosite (see Bishop et al. [2008a] for spectral properties) is most likely to be causing this feature because they form under conditions similar to the clay minerals observed at Mawrth Vallis.”
Estimating the soil clay content and organic matter by means of different calibration methods of vis-NIR diffuse reflectance spectroscopy (2016, unknown): “The strong absorptions near 1416 nm and 1911 nm in the spectra indicate the presence of water bound in the interlayer lattices (Bishop et al., 2008).”