Re, Os and Ir in Antarctic unequilibrated ordinary chondrites and implications for the solar system abundance of Re

The concentrations of Re, Os and Ir in Antarctic unequilibrated ordinary chondrites (UOC) were determined by radiochemical neutron activation analysis. Large fractionations among these elements were found in Antarctic UOC. This is quite different from non‐Antarctic UOC and equilibrated ordinary chon...

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Published inGeophysical research letters Vol. 22; no. 16; pp. 2167 - 2170
Main Authors Ebihara, Mitsuru, Ozaki, Hiromasa
Format Journal Article
LanguageEnglish
Published Washington, DC Blackwell Publishing Ltd 15.08.1995
American Geophysical Union
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Abstract The concentrations of Re, Os and Ir in Antarctic unequilibrated ordinary chondrites (UOC) were determined by radiochemical neutron activation analysis. Large fractionations among these elements were found in Antarctic UOC. This is quite different from non‐Antarctic UOC and equilibrated ordinary chondrites (EOC). Average Re/Os and Re/Ir ratios in ordinary chondrites are 25–30% higher than those in C1 chondrites and 10–15% higher than those in C2 and C3 chondrites. In contrast, the Os/Ir ratio is not variable among these chondrite groups. It is therefore suggested that Re is fractionated among ordinary and carbonaceous chondrites. Atom abundances of Os and Ir relative to 106 Si atoms of H chondrites are nearly equal to those of C1 chondrites, but their Re value is 30% higher than the C1 value. Considering that the currently accepted value for solar system abundance of Re (0.517 atom relative to 106 Si atoms) [Anders and Grevesse, 1989] is the lowest value among (Sinormalized) Re abundances in C1, C2, C3 and H chondrites, its value should be changed to a larger value. If C2 chondrites are adopted as the solar system standard, the solar system abundance of Re is changed to 0.0589, with those of Os and Ir being 0.740 and 0.685, respectively, at the same time.
AbstractList The concentrations of Re, Os and Ir in Antarctic unequilibrated ordinary chondrites (UOC) were determined by radiochemical neutron activation analysis. Large fractionations among these elements were found in Antarctic UOC. This is quite different from non-Antarctic UOC and equilibrated ordinary chondrites (EOC). Average Re/Os and Re/Ir ratios in ordinary chondrites are 25-30% higher than those in C1 chondrites and 10-15% higher than those in C2 and C3 chondrites. In contrast, the Os/Ir ratio is not variable among these chondrite groups. It is therefore suggested that Re is fractionated among ordinary and carbonaceous chondrites. Atom abundances of Os and Ir relative to 10 super(6) Si atoms of H chondrites are nearly equal to those of C1 chondrites, but their Re value is 30% higher than the C1 value. Considering that the currently accepted value for solar system abundance of Re (0.517 atom relative to 10 super(6) Si atoms) [Anders and Grevesse, 1989] is the lowest value among (Sinormalized) Re abundances in C1, C2, C3 and H chondrites, its value should be changed to a larger value. If C2 chondrites are adopted as the solar system standard, the solar system abundance of Re is changed to 0.0589, with those of Os and Ir being 0.740 and 0.685, respectively, at the same time.
The concentrations of Re, Os and Ir in Antarctic unequilibrated ordinary chondrites (UOC) were determined by radiochemical neutron activation analysis. Large fractionations among these elements were found in Antarctic UOC. This is quite different from non‐Antarctic UOC and equilibrated ordinary chondrites (EOC). Average Re/Os and Re/Ir ratios in ordinary chondrites are 25–30% higher than those in C1 chondrites and 10–15% higher than those in C2 and C3 chondrites. In contrast, the Os/Ir ratio is not variable among these chondrite groups. It is therefore suggested that Re is fractionated among ordinary and carbonaceous chondrites. Atom abundances of Os and Ir relative to 10 6 Si atoms of H chondrites are nearly equal to those of C1 chondrites, but their Re value is 30% higher than the C1 value. Considering that the currently accepted value for solar system abundance of Re (0.517 atom relative to 10 6 Si atoms) [ Anders and Grevesse, 1989] is the lowest value among (Sinormalized) Re abundances in C1, C2, C3 and H chondrites, its value should be changed to a larger value. If C2 chondrites are adopted as the solar system standard, the solar system abundance of Re is changed to 0.0589, with those of Os and Ir being 0.740 and 0.685, respectively, at the same time.
The concentrations of Re, Os and Ir in Antarctic unequilibrated ordinary chondrites (UOC) were determined by radiochemical neutron activation analysis. Large fractionations among these elements were found in Antarctic UOC. This is quite different from non‐Antarctic UOC and equilibrated ordinary chondrites (EOC). Average Re/Os and Re/Ir ratios in ordinary chondrites are 25–30% higher than those in C1 chondrites and 10–15% higher than those in C2 and C3 chondrites. In contrast, the Os/Ir ratio is not variable among these chondrite groups. It is therefore suggested that Re is fractionated among ordinary and carbonaceous chondrites. Atom abundances of Os and Ir relative to 106 Si atoms of H chondrites are nearly equal to those of C1 chondrites, but their Re value is 30% higher than the C1 value. Considering that the currently accepted value for solar system abundance of Re (0.517 atom relative to 106 Si atoms) [Anders and Grevesse, 1989] is the lowest value among (Sinormalized) Re abundances in C1, C2, C3 and H chondrites, its value should be changed to a larger value. If C2 chondrites are adopted as the solar system standard, the solar system abundance of Re is changed to 0.0589, with those of Os and Ir being 0.740 and 0.685, respectively, at the same time.
Author Ozaki, Hiromasa
Ebihara, Mitsuru
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Cites_doi 10.1029/RG012i001p00071
10.1016/0016-7037(82)90123-5
10.1016/0016-7037(89)90286-X
10.1016/0016-7037(78)90220-X
10.1016/0016-7037(67)90130-5
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10.1016/0016-7037(82)90208-3
10.1007/BF02042947
10.1016/0016-7037(83)90048-0
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Issue 16
Keywords meteorites
rhenium
neutron activation analysis
solar system
abundance
osmium
chemical fractionation
H chondrites
iridium
Yamato Meteorites
carbonaceous chondrites
Allan Hills Meteorites
Allende Meteorite
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American Geophysical Union
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Snippet The concentrations of Re, Os and Ir in Antarctic unequilibrated ordinary chondrites (UOC) were determined by radiochemical neutron activation analysis. Large...
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SubjectTerms Abundance
Antarctica
Carbonaceous chondrites
Chondrites
Cosmochemistry. Extraterrestrial geology
Distillation
Earth sciences
Earth, ocean, space
Exact sciences and technology
Iridium
Meteorites. Tectites. Impactites
Silicon
Solar system
Title Re, Os and Ir in Antarctic unequilibrated ordinary chondrites and implications for the solar system abundance of Re
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