Discovery of 17,18 O-rich material from meteorite by direct-imaging method using stigmatic-SIMS and 2D ion detector
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概要
- 論文の詳細を見る
We report a discovery of a chemically and isotopically unique material distributed ubiquitously in fine-grained matrix of a primitive carbonaceous chondrite Acfer 094. The observations were made in situ using a novel high precision imaging technique adopted direct-imaging method. The material is extremely enriched in heavy oxygen isotopes of O-17 and O-18 of +18% relative to the Earth's ocean while previously reported variation of oxygen isotopes is as large as a range from -8% to 0%. Based on the unique chemical composition of the material, the abundance of the material in the meteorite matrix is calculated to be 94 ± 20 (σ) ppm by volume using elemental mapping with a 7 μm2 spatial resolution by FE-SEM-EDS on the meteorite thin section. The average size of identified materials is 5 x 5 x 5 μm3. Therefore, isotope imaging capability over 500 x 500 μm2 area with micron resolution and an isotopic ratio precision of 1 percent is required to investigate about the presence of such material.
- Elsevier B.V.の論文
- 2008-12-15
著者
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Itoh Shoichi
Department Of Natural History Sciences Hokkaido University
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Yurimoto Hisayoshi
Department of Natural History Sciences, Hokkaido University
関連論文
- Remnants of the early solar system water enriched in heavy oxygen isotopes
- Discovery of 17,18 O-rich material from meteorite by direct-imaging method using stigmatic-SIMS and 2D ion detector
- Non-chondritic oxygen isotopic component of metals in a noble-gas-rich chondrite : vestige of stellar wind from the protosun?