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- W2068190178 abstract "Abstract After correcting for cosmic-ray produced spallation and (n, γ) components the isotopic composition of Kr in the investigated 3 unequilibrated and 2 gas-rich chondrites is similar. The average δ-values relative to atmospheric Kr in percent are: δ 86 78 = −4.05 ± 1.1 ; δ 86 80 = −1.25 ± 0.8 ; δ 86 82 = −2.05 ± 0.5 ; δ 86 83 = −1.55 ± 0.5 ; δ 86 84 = −1.6 ± 0.4 . The low 78 Kr abundance appears to exclude the possibility that an addition of fission Kr alone is responsible for the observed differences. Mass fractionation, together with some Kr from neutron capture on Br, could just within the experimental uncertainties explain the results. A model combining mass fractionation and the addition of fission Kr would, however, explain the experimental data much better. Some other processes which could have influenced the terrestrial or meteoritic Kr isotopic composition are also discussed, but their contributions are likely to be negligible." @default.
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- W2068190178 date "1967-08-01" @default.
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- W2068190178 title "The isotopic composition of krypton in unequilibrated and gas rich chondrites" @default.
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- W2068190178 doi "https://doi.org/10.1016/0012-821x(67)90178-1" @default.
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