TY - JOUR
T1 - Noble gas and oxygen isotopic compositions of Towada H6-chondrite from Aomori Prefecture, Japan
AU - Park, Jisun
AU - Okazaki, Ryuji
AU - Kusakabe, Minoru
AU - Nagao, Keisuke
AU - Yoneda, Shigekazu
PY - 2003
Y1 - 2003
N2 - Noble gas and oxygen isotopic compositions were studied for the Towada meteorite, a recent fall in Aomori Prefecture, Japan. The meteorite was classified as a H6 chondrite based on oxygen isotope ratios (δ17O = 2.82‰, δ18O = 4.03‰) and concentrations and elemental ratios of the heavy noble gases. The U, Th-He and K-Ar gas retention ages, calculated as 0.38 b.y. and 1.3 b.y., respectively, suggest preferential loss of 4He compared with 40Ar. Cosmic-ray exposure ages using cosmogenic 3He, 21Ne and 38Ar concentrations were 7.67, 31.1 and 18.6 m.y., respectively. The 3He and 4He loss observed for this meteorite may be due to heating by solar radiation during orbital motion around the Sun. The short nominal exposure age based on 38Ar may be due to 38Ar loss during weathering or due to chemical heterogeneity of the meteorite. Existence of excess fissiogenic 131-136Xe from extinct 244Pu is consistent with the presence of 129Xe produced from extinct 129I.
AB - Noble gas and oxygen isotopic compositions were studied for the Towada meteorite, a recent fall in Aomori Prefecture, Japan. The meteorite was classified as a H6 chondrite based on oxygen isotope ratios (δ17O = 2.82‰, δ18O = 4.03‰) and concentrations and elemental ratios of the heavy noble gases. The U, Th-He and K-Ar gas retention ages, calculated as 0.38 b.y. and 1.3 b.y., respectively, suggest preferential loss of 4He compared with 40Ar. Cosmic-ray exposure ages using cosmogenic 3He, 21Ne and 38Ar concentrations were 7.67, 31.1 and 18.6 m.y., respectively. The 3He and 4He loss observed for this meteorite may be due to heating by solar radiation during orbital motion around the Sun. The short nominal exposure age based on 38Ar may be due to 38Ar loss during weathering or due to chemical heterogeneity of the meteorite. Existence of excess fissiogenic 131-136Xe from extinct 244Pu is consistent with the presence of 129Xe produced from extinct 129I.
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U2 - 10.2343/geochemj.37.639
DO - 10.2343/geochemj.37.639
M3 - Article
AN - SCOPUS:0347900566
SN - 0016-7002
VL - 37
SP - 639
EP - 648
JO - Geochemical Journal
JF - Geochemical Journal
IS - 6
ER -