Strength of mineral absorption features in the transmitted component of near-infrared reflected light - First results from RELAB. [spectrogoniometer for planetary and lunar surface composition experiments]

Bidirectional reflectance measurements are the only type of reflectance data available to the remote observer. For compositional interpretations, data are desired not only for identification of possible mineral components but also for modal abundance. The latter requires detailed information about the strength of absorption features. Using a new laboratory facility, the RELAB, laboratory data in the near infrared are presented that document effects of particle size, mineral mixtures, and viewing geometry for selected materials with well-developed absorption bands. The commonly observed increase in reflectance with decrease in particle size is also observed for absorption bands as well as a related decrease in absorption strength. For small particles in parts of the spectrum of maximum reflectance, however, a minor decrease in reflectance with a decrease in particle size is sometimes observed. Small particles dominate the observed characteristics of particulate surfaces, which contain a range of particle sizes. The mean optical path length (transmission through particles) of reflected radiation measured for a variety of particle sizes has an apparent upper limit of about 2 mm for particles <250 μm. The typical number of particles involved in the optical path is less than 50.

[1]  D. B. Nash,et al.  Vitrification darkening of rock powders: implications for optical properties of the lunar surface , 1973 .

[2]  G. Hunt Visible and near-infrared spectra of minerals and rocks : I silicate minerals , 1970 .

[3]  D. Vaughan,et al.  2 – POLARIZED ELECTRONIC SPECTRA , 1975 .

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

[5]  A. Goetz,et al.  Geologic remote sensing. , 1981, Science.

[6]  T. McCord,et al.  Spectrophotometric remote sensing of planets and satellites , 1981 .

[7]  T. McCord,et al.  Vitrification darkening in the lunar highlands and identification of Descartes material at the Apollo 16 site , 1973 .

[8]  David S. McKay,et al.  Grain size and the evolution of lunar soils. , 1977 .

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

[10]  H. Mao,et al.  ABSORPTION SPECTROSCOPY OF IONIC AND MOLECULAR UNITS IN CRYSTALS AND GLASSES , 1975 .

[11]  E Schreiber,et al.  Properties and Composition of Lunar Materials: Earth Analogies , 1970, Science.

[12]  Bonnie J. Buratti,et al.  The effects of scattering geometry on the spectrophotometric properties of powdered material , 1980 .

[13]  T. Gehrels,et al.  Planets, Stars and Nebulae Studied with Photopolarimetry , 1974 .

[14]  Carle M. Pieters,et al.  Moon: near-infrared spectral reflectance, a first good look. , 1981 .

[15]  C. Pieters Mare basalt types on the front side of the moon - A summary of spectral reflectance data , 1978 .

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

[17]  John B. Adams,et al.  4 – INTERPRETATION OF VISIBLE AND NEAR-INFRARED DIFFUSE REFLECTANCE SPECTRA OF PYROXENES AND OTHER ROCK-FORMING MINERALS , 1975 .

[18]  Wendell W. Mendell,et al.  Application of Kubelka-Munk theory of diffuse reflectance to geologic problems - The role of scattering , 1982 .

[19]  John B. Adams,et al.  Spectral reflectance 0.4 to 2.0 microns of silicate rock powders. , 1967 .

[20]  John B. Adams,et al.  Visible and near‐infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the solar system , 1974 .

[21]  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 .

[22]  B. Hapke,et al.  Bidirectional reflectance spectroscopy: 2. Experiments and observations , 1981 .

[23]  W. Wendlandt Modern Aspects of Reflectance Spectroscopy , 1968 .