Computer Science
Scientific paper
Feb 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988gecoa..52..499m&link_type=abstract
Geochimica et Cosmochimica Acta (ISSN 0016-7037), vol. 52, Feb. 1988, p. 499-504. NSF-supported research.
Computer Science
3
Beryllium Isotopes, Chondrites, Cosmic Rays, Meteoritic Composition, Stony Meteorites, Cross Sections, Mass Spectroscopy, Regression Analysis, Meteorites, Stony Meteorites, Beryllium 10, Composition, Formation, Spectrometry, Laboratory Studies, Production Rate, Procedure, Systematics, Isotopes
Scientific paper
The relationship between the production rate of Be-10 in stony meteorites and its element composition was investigated by measuring the contents of Be-10 in 21 samples from 17 meteorites with known major-element composition, and comparing the experimental Be-10 values with those obtained by the regression analysis. The Be-10 production was modeled by the equation of Stauffer (1962). The measured Be-10 contents were found to range from 16 dpm/kg in the oxygen- and magnesium-poor eucrites and the Indarch meteorite to 28 dpm/kg in the oxygen- and magnesium-rich aubrites and the mineral separates from Bruderheim. Using the regression analyses and taking in account various corrections, an equation was obtained which reproduces the measured Be-10 content with an accuracy of about 10 percent.
Herzog Gregory F.
Kruse T. H.
Moniot Robert K.
Pal D. K.
Savin W.
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