Other
Scientific paper
Feb 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985lpsc...15..805j&link_type=abstract
(Lunar and Planetary Institute, NASA, American Geophysical Union, et al., Lunar and Planetary Science Conference, 15th, Houston,
Other
11
Astronomical Spectroscopy, Lunar Composition, Lunar Rocks, Lunar Soil, Planetary Craters, Spectral Reflectance, Abundance, Basalt, Data Acquisition, Eigenvalues, Eigenvectors, Wavelengths, Planets, Reflectance, Analysis, Techniques, Spectra, Composition, Abundance, Mixing, Physical Properties, Telescopic Methods, Moon, Copernicus, Wavelengths, Models, Maria, Basalt, Soil, Highlands, Clinopyroxene, Samples, Lunar
Scientific paper
A technique is presented for quantitative analysis of planetary reflectance spectra as mixtures of particles on microscopic and macroscopic scales using principal components analysis. This technique allows for determination of the endmembers being mixed, their abundance, and the scale of mixing, as well as other physical parameters. Eighteen lunar telescopic reflectance spectra of the Copernicus crater region, from 600 nm to 1800 nm in wavelength, are modeled in terms of five likely endmembers: mare basalt, mature mare soil, anorthosite, mature highland soil, and clinopyroxene. These endmembers were chosen from a similar analysis of 92 lunar soil and rock samples. The models fit the data to within 2 percent rms. It is found that the goodness of fit is marginally better for intimate mixing over macroscopic mixing.
Adams Barclay J.
Johnson Paul E.
Smith Milton O.
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