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• W2033759312 abstract "Abstract In order to characterize the planetary noble gas carrier Q, we separated a Q-rich floating fraction from the Allende meteorite into ten fractions by a combination of colloidal and density separations. All five noble gases in the separated fractions were analyzed by pyrolysis in 600 and 1600°C temperature steps. Half of Q in the floating fraction is concentrated in the fraction C1-8D with the density of 1.65 ± 0.04 g/cm 3 . All the separated fractions show similar isotopic ratios except for 40 Ar/ 36 Ar ratios. C1-8D has the lowest 38 Ar/ 36 Ar and 40 Ar/ 36 Ar ratios (0.18784 ± 0.00020 and 4.36 ± 0.15, respectively) in the 1600°C fraction, confirming that the fraction is enriched in Q. Most grains in C1-8D are carbonaceous with small amounts of F and O. These results imply either that the density of Q is 1.65 ± 0.04 g/cm 3 or that Q preferentially sticks to matter of that density. All the separates have similar Q to diamond ratios, indicating that Q and diamond are closely associated." @default.
• W2033759312 created "2016-06-24" @default.
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• W2033759312 date "2003-12-01" @default.
• W2033759312 modified "2023-09-23" @default.
• W2033759312 title "An attempt to separate Q from the Allende meteorite by physical methods" @default.
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• W2033759312 doi "https://doi.org/10.1016/j.gca.2003.08.009" @default.
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