Computer Science
Scientific paper
Mar 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..317c&link_type=abstract
In Lunar and Planetary Inst., Twenty-fourth Lunar and Planetary Science Conference. Part 1: A-F p 317-318 (SEE N94-12015 01-91)
Computer Science
2
Asteroids, Emission Spectra, Meteoritic Composition, Olivine, Spectral Reflectance, Spectrum Analysis, Metallicity, Meteoritic Microstructures, Stony-Iron Meteorites
Scientific paper
The recent acquisition of high resolution 0.3 - 2.6 micron reflectance spectra for a number of olivine-rich asteroids permits the analysis of their surface compositions to be made on the basis of new and existing laboratory spectral data for pallasitic olivines and olivine-metal mixtures. Analysis of the spectral data for the latter has revealed a number of spectral parameters which can be used to constrain olivine and metal abundances, grain sizes, and olivine compositions. The following topics are discussed in greater detail: pallasite olivine spectra, olivine-metal mixture spectra, and olivine-rich asteroid spectra.
No associations
LandOfFree
Olivine-rich asteroids, pallasitic olivine and olivine-metal mixtures: Comparisons of reflectance spectra does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Olivine-rich asteroids, pallasitic olivine and olivine-metal mixtures: Comparisons of reflectance spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Olivine-rich asteroids, pallasitic olivine and olivine-metal mixtures: Comparisons of reflectance spectra will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1447678