Spectral properties of mixtures of montmorillonite and dark carbon grains: Implications for remote sensing minerals containing chemically and physically adsorbed water

The spectral properties from 0.4 to 3μm of montmorillonite plus dark carbon grains (called opaques) of various sizes are studied as a function of the weight fraction of opaques present. The reflectance level and band depths of the 1.4-, 1.9-, 2.2-, and 2.8-μm water and/or OH absorption features are analyzed using derived empirical relationships and scattering theory. It is found that the absorption band depths and reflectance level are a very nonlinear function of the weight fraction of opaques present but can be predicted in many cases by simple scattering theory. The 2.8-μm bound water fundamental band is the most difficult absorption feature to suppress. The overtone absorptions are suppressed a greater amount than the fundamental but are still apparent even when 10–20 wt% opaques are present. Thus the band depth ratio of one overtone by the fundamental or other lower overtone varies as a function of the weight fraction of opaques present. The relationships observed and the simple scattering theory presented show that quantitative compositional remote sensing studies are feasible for surfaces containing complex mineral mixtures. The question of the uniqueness of quantitative remote sensing is discussed.

[1]  R. Clark,et al.  Spectral properties of ice‐particulate mixtures and implications for remote sensing: 1. Intimate mixtures , 1984 .

[2]  B. Hapke Bidirectional reflectance spectroscopy: 1. Theory , 1981 .

[3]  R. Clark,et al.  Reflectance spectroscopy: Quantitative analysis techniques for remote sensing applications , 1984 .

[4]  R. N. Clark,et al.  A LARGE-SCALE INTERACTIVE ONE-DIMENSIONAL ARRAY PROCESSING SYSTEM , 1980 .

[5]  M. Wolff Theory and application of the polarization-albedo rules , 1980 .

[6]  R. Clark,et al.  The infrared spectrum of Rhea , 1981 .

[7]  R. Clark,et al.  The spectral reflectance of water-mineral mixtures at low temperatures. [observed on natural satellites and other solar system objects] , 1981 .

[8]  R. Singer Near-infrared spectral reflectance of mineral mixtures - Systematic combinations of pyroxenes, olivine, and iron oxides , 1981 .

[9]  U. Fink,et al.  Remote spectroscopic identification of carbonaceous chondrite mineralogies: Applications to Ceres and Pallas , 1979 .

[10]  Joseph Veverka,et al.  When are spectral reflectance curves comparable , 1982 .

[11]  Paul E. Johnson,et al.  A semiempirical method for analysis of the reflectance spectra of binary mineral mixtures , 1983 .

[12]  D. B. Nash,et al.  Spectral reflectance systematics for mixtures of powdered hypersthene, labradorite, and ilmenite , 1974 .

[13]  R. Ashley,et al.  Spectra of altered rocks in the visible and near infrared , 1979 .

[14]  Roger N. Clark,et al.  Water frost and ice - The near-infrared spectral reflectance 0.65-2.5 microns. [observed on natural satellites and other solar system objects , 1981 .

[15]  Torrence V. Johnson,et al.  Optical properties of carbonaceous chondrites and their relationship to asteroids , 1973 .

[16]  L. Lebofsky,et al.  Spectroscopic evidence for aqueous alteration products on the surfaces of low-albedo asteroids , 1980 .