Atlas of reflectance spectra of terrestrial, lunar, and meteoritic powders and frosts from 92 to 1800 NM

Details Atlas of reflectance spectra of terrestrial, lunar, and meteoritic powders and frosts from 92 to 1800 NM Atlas of reflectance spectra of terrestrial, lunar, and meteoritic powders and frosts from 92 to 1800 NM

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987icar...69...14w&link_type=abstract

Icarus (ISSN 0019-1035), vol. 69, Jan. 1987, p. 14-28. NASA-supported research.

Computer Science

75

Lunar Rocks, Lunar Soil, Meteorites, Spectral Reflectance, Spectroscopic Analysis, Achondrites, Chondrites, Feldspars, Meteoritic Composition, Minerals, Olivine, Pyroxenes, Planets, Reflectance, Spectra, Moon, Earth, Meteorites, Frost, 60025, Samples, Terrestrial, Samples, Lunar, Samples, Meteorites, Wavelengths, Minerals, Remote Sensing, Ultraviolet, Infrared, Spectroscopy, Feldspar, Experiments, Laboratory Studies, Theoretical Studies, Apollo Missions, Orthopyroxene, Clinopyroxene, Achondrites, Carbonaceo

Scientific paper

The spectra of samples of several powder and frost materials are presented to serve in a reference database for future far-UV scans of solar system bodies. The spectra cover in the 92-1800 nm wavelengths, i.e., wavenumbers 110,000-5600/cm and photon energies from 13.5-1.5 eV. Preparation procedures for the particulates are delineated. The survey includes feldspars, orthopyroxenes, clinopyroxenes, olivines, assorted minerals, achondrites, carbonaceous chondrites and ordinary chondrites, lunar soils and rocks. Frosts of H2O, CO2, NH3 and SO2 gases were also examined. The data are expected to aid in obtaining spectral matches for asteroids and meteoroids when far-UV telescopy of solar system bodies is performed.

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