The Relative Abundance of Some Light Nuclear Species as Determined from the Composition of Stony Meteorites

Details The Relative Abundance of Some Light Nuclear Species as Determined from the Composition of Stony Meteorites The Relative Abundance of Some Light Nuclear Species as Determined from the Composition of Stony Meteorites

Sep 1947

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1947phrv...72..456b&link_type=abstract

Physical Review, vol. 72, Issue 6, pp. 456-457

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Scientific paper

A statistical study has been made of the relative abundances of the major constituents of the silicate phase of stony meteorites. The results of that study, for the case of lithophile elements, have been combined with data on isotopic abundances, thus giving figures for the abundances, relative to one another, of several nuclear species. The abundance ratios of three isobaric pairs: K40-Ca40, Ca46-Ti46, and Ca48-Ti48, are given.

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