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- W2053199089 abstract "The abundances of the 21 stable isotopes of neon, argon, krypton, and xenon were measured in the Costilla Peak iron meteorite. We observe a pronounced spallation component in all four of the gases; and that the neon and argon results agree with previous iron meteorite measurements. Integration of a recent Rudstam formula over the Arnold, Honda, and Lal cosmic ray spectra accurately predicts the isotopic composition of the observed spallation component in all cases except, possibly, neon. Calculated production rates for21Ne and38Ar give cosmic ray exposure ages of 560 m.y. and 500 m.y., respectively, for a sample depth of 100 g/cm2. We obtain large variations in the exposure ages based on krypton and xenon, which might be explained by lack of knowledge about target element abundances. The small and questionable amount of129Xe in addition to the trapped and spallation components indicates a longer129I-129Xe formation interval for Costilla Peak than for the Chondrites." @default.
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- W2053199089 date "1967-07-01" @default.
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- W2053199089 title "Spallation neon, argon, krypton, and xenon in an iron meteorite" @default.
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- W2053199089 doi "https://doi.org/10.1016/0012-821x(67)90146-x" @default.
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