4.4 Article

SPECTRAL AND HYDRATION PROPERTIES OF ALLOPHANE AND IMOGOLITE

Journal

CLAYS AND CLAY MINERALS
Volume 61, Issue 1-2, Pages 57-74

Publisher

SPRINGER
DOI: 10.1346/CCMN.2013.0610105

Keywords

Allophane; Emission Spectroscopy; Imogolite; Reflectance Spectroscopy; XRD

Funding

  1. NASA's Mars Fundamental Research program
  2. NASA Postdoctoral Program

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Allophane and imogolite are common alteration products of volcanic materials. Natural and synthetic allophanes and imogolites were characterized in the present study in order to clarify the short-range order of these materials and to gain an understanding of their spectral properties. Spectral analyses included visible/near-infrared (VNIR), and infrared (IR) reflectance of particulate samples and thermal-infrared (TIR) emissivity spectra of particulate and pressed pellets. Spectral features were similar but not identical for allophane and imogolite. In the near-infrared (NIR) region, allophane spectra exhibited a doublet near 7265 and 7120 cm(-1) (1.38 and 1.40 mu m) due to OH2 nu, a broad band near 5220 cm(-1) (1.92 mu m) due to H2O nu+delta, and a band near 4560 cm(-1) (2.19 mu m) due to OH nu+delta. Reflectance spectra of imogolite in this region included a doublet near 7295 and 7190 cm(-1) (1.37 and 1.39 mu m) due to OH2 nu, a broad band near 5200 cm(-1) (1.92 mu m) due to H2O nu+delta, and a band near 4565 cm(-1) (2.19 mu m) due to OH nu+delta. A strong broad band was also observed near 3200-3700 cm(-1) (similar to 2.8-3.1 mu m) which is a composite of OH nu, H2O nu, and H2O2 delta vibrations. Visible/near-infrared spectra were also collected under two relative humidity (RH) conditions. High-RH conditions resulted in increasing band strength for the H2O combination modes near 6900-6930 cm(-1) (1.45 mu m) and 5170-5180 cm(-1) (1.93 mu m) in the allophane and imogolite spectra due to increased abundances of adsorbed H2O molecules. Variation in adsorbed H2O content caused an apparent shift in the bands near 1.4 and 1.9 mu m. A doublet H2O delta vibration was observed at 1600-1670 cm(-1) (similar to 6.0-6.2 mu m) and a band due to OH bending for O3SiOH was observed at similar to 1350-1485 cm(-1) (similar to 6.7-7.4 mu m). The Si-O-Al stretching vibrations occurred near 1030 and 940 cm(-1) (similar to 9.7 and 10.6 mu m) for allophane and near 1010 and 930 cm(-1) (similar to 9.9 and 10.7 mu m) for imogolite. OH out-of-plane bending modes occurred near 610 cm(-1) (16.4 mu m) for allophane and at 595 cm(-1) (16.8 mu m) for imogolite. Features due to Si-O-Al bending vibrations were observed at 545, 420, and 335 cm(-1) (similar to 18, 24, and 30 mu m) for allophane and at 495, 415, and 335 cm(-1) (similar to 20, 24, and 30 mu m) for imogolite. The emissivity spectra were obtained from pressed pellets of the samples, which greatly enhanced the spectral contrast of the TIR absorptions. Predicted NIR bands were calculated from the mid-IR fundamental stretching and bending vibrations and compared with the measured NIR values. Controlled-RH X-ray diffraction (XRD) experiments were also performed in order to investigate changes in the mineral structure with changing RH conditions. Both allophane and imogolite exhibited decreasing low-angle XRD intensity with increasing RH, which was probably a result of interactions between H2O molecules and the curved allophane and imogolite structures.

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