Computer Science
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24.1581z&link_type=abstract
In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z p 1581-1582 (SEE N94-20636 05-91
Computer Science
Diffuse Radiation, Feldspars, Meteoritic Composition, Meteoritic Microstructures, Olivine, Pyroxenes, Radiation Spectra, Reflectance, Asteroids, Enstatite, Meteorites, Reflected Waves
Scientific paper
Although many similarities exist between meteorite spectra and 'primitive' asteroids, there are unexplained discrepancies. These discrepancies do not appear to arise from grain size effects. Assuming that primitive meteorites did in fact originate from the 'primitive' asteroids, we believe that there are two testable explanations for the observed spectral discrepancies: compositional or structural differences. We have begun to synthesize and collect reflectance and Mossbauer spectra of pertinent materials, beginning with olivine, pyroxene, and plagioclase (all found in primitive meteorites), and to assess the possible effects composition may have on spectral features. Our study focuses on the combination of composition and structural effects.
Galindo Carlos
Lauer V.
Le Linh
Morris Robert R.
Vilas Faith
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