1982
DOI: 10.2343/geochemj.16.157
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Composition of the noble gases in Canyon Diablo.

Abstract: Five separate fractions of noble gases were extracted and analyzed as a 150g sample of the Canyon Diablo iron meteorite was heated to successively higher temperatures by direct coupling with an RF coil.Isotopic compositions of the light gases, He, Ne and Ar, demonstrate that essentially their entire inventory was produced by spallation reactions. Spallation products are also a prominent feature of the isotopes of Kr and Xe, but in each gas fraction the spallogenic heavy gases were mixed with a nonspallogenic c… Show more

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Cited by 3 publications
(1 citation statement)
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“…(Fe, Z = 26): Deep in the SN debris, iron meteorites and the cores of the terrestrial planets formed. Iron meteorites trapped "normal" Xe, like that on Earth [47]. The University of Tokyo [48], Harvard [49] and Cal Tech [50] have new data showing that iron meteorites did not form by the extraction of iron from an interstellar cloud.…”
mentioning
confidence: 99%
“…(Fe, Z = 26): Deep in the SN debris, iron meteorites and the cores of the terrestrial planets formed. Iron meteorites trapped "normal" Xe, like that on Earth [47]. The University of Tokyo [48], Harvard [49] and Cal Tech [50] have new data showing that iron meteorites did not form by the extraction of iron from an interstellar cloud.…”
mentioning
confidence: 99%