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- W1974323786 abstract "The unusual stone meteorites Winona, Mt. Morris (Wisconsin), Pontlyfni, Kakangari and Acapulco, plus a chondritic inclusion from the Cumberland Falls aubrite, have been analyzed for their carbon content and isotopic composition, in order to determine whether similarities exist between all, or some, of the meteorites. The technique employed for these determinations was one of combustion in steps from room temperature to 1200°C, allowing distinction between different carbon-containing species present. Winona, Mt. Morris (Wis), Pontlyfni and the chondritic inclusion from Cumberland Falls all behave in a common fashion during combustion; the major indigenous carbon component in these specimens is graphite, with a δ13C value of between −9.5 and −2.8%., close to the range reported for graphite in both enstatite chondrites and IAB irons. Thus the links proposed to exist between “winonaites”, silicates from IABs and E-chondrites from oxygen isotopes and major element chemistry are also apparent for carbon. Kakangari is clearly different from “winonaites”, and there is no basis for including this meteorite in any group with IAB irons or enstatite chondrites. Silicates from Acapulco may have some links with “winonaites”, but the carbon isotopic composition of graphite precipitated from metal (δ13C = −20%.) and from the element still in solid solution (δ13C = −28%.) suggest that the iron/nickel portions of the meteorites are unrelated." @default.
- W1974323786 created "2016-06-24" @default.
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- W1974323786 date "1986-02-01" @default.
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- W1974323786 title "Carbon isotope relationships in winonaites and forsterite chondrites" @default.
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- W1974323786 doi "https://doi.org/10.1016/0016-7037(86)90174-2" @default.
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