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- W2005161893 abstract "Halite crystals from the Zag H3-6 chondrite contain essentially pure (monoisotopic) xenon-129 ( 129 Xe) produced in the early history of the solar system by the decay of short-lived iodine-129 ( 129 I) (half-life = 15.7 million years). Correlated release of 129 Xe and 128 Xe, produced artificially from 127 I by neutron irradiation, corresponds to an initial ( 129 I/ 127 I) ratio of (1.35 ± 0.05) × 10 −4 , close to the most primitive early solar system value. If the 129 Xe was produced by in situ decay, then the halite formed from an aqueous fluid within 2 million years of the oldest known solar system minerals." @default.
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- W2005161893 date "2000-06-09" @default.
- W2005161893 modified "2023-09-24" @default.
- W2005161893 title "Extinct <sup>129</sup> I in Halite from a Primitive Meteorite: Evidence for Evaporite Formation in the Early Solar System" @default.
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- W2005161893 doi "https://doi.org/10.1126/science.288.5472.1819" @default.
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