Other
Scientific paper
May 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85..573l&link_type=abstract
Astronomical Journal, vol. 85, May 1980, p. 573-585.
Other
35
Asteroids, Carbonaceous Chondrites, Hydration, Infrared Reflection, Planetary Composition, Data Reduction, Evaporation, Infrared Absorption, Infrared Spectra, Meteoritic Composition, Mineralogy, Water Vapor, Asteroids, Infrared, Wavelengths, Spectrum, Water, Hydration, Data, Reflectivity, Absorption, Comparisons, Mineralogy, Depth, Surface, Observations, Bands, Data Reduction, Evaporation, Catalogs, Albedo, Flux, Meteorites, Carbonaceous Chondrites, Silicates, Thermal Radiation, Frost, Clays, C Asteroids, U
Scientific paper
Infrared reflectance spectra have shown the presence of an absorption feature in the 3-4 micron region for seven C and U asteroids. By comparison with laboratory spectra of terrestrial silicates and meteorites, it is concluded that this band is probably due to water in the form of hydrated salts and silicates (clay minerals), implying that the surface material of these asteroids may be analogous to the CI and CM carbonaceous chondritic meteorites. The presence of other hydrated minerals, however, cannot be ruled out. The depths of the water bands in the spectra vary from asteroid to asteroid, though no asteroid spectrum shows a band as deep as was detected on 1 Ceres. On four other C asteroids, no water band was detected. The implications of these observations for the mineralogy of these asteroids are discussed
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