Remnants of the Early Solar System Water Enriched in Heavy Oxygen Isotopes
Oxygen isotopic composition of our solar system is believed to have resulted from mixing of two isotopically distinct nebular reservoirs, ¹⁶O-rich and ¹⁷,¹⁸O-rich relative to Earth. The nature and composition of the ¹⁷,¹⁸O-rich reservoir are poorly constrained. We report an in situ discovery of a ch...
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 2007-07, Vol.317 (5835), p.231-233 |
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| creator | Sakamoto, Naoya Seto, Yusuke Itoh, Shoichi Kuramoto, Kiyoshi Fujino, Kiyoshi Nagashima, Kazuhide Krot, Alexander N Yurimoto, Hisayoshi |
| description | Oxygen isotopic composition of our solar system is believed to have resulted from mixing of two isotopically distinct nebular reservoirs, ¹⁶O-rich and ¹⁷,¹⁸O-rich relative to Earth. The nature and composition of the ¹⁷,¹⁸O-rich reservoir are poorly constrained. We report an in situ discovery of a chemically and isotopically unique material distributed ubiquitously in fine-grained matrix of a primitive carbonaceous chondrite Acfer 094. This material formed by oxidation of Fe,Ni-metal and sulfides by water either in the solar nebula or on a planetesimal. Oxygen isotopic composition of this material indicates that the water was highly enriched in ¹⁷O and ¹⁸O (δ¹⁷,¹⁸OSMOW = +180[per thousand] per mil), providing the first evidence for an extremely ¹⁷,¹⁸O-rich reservoir in the early solar system. |
| doi_str_mv | 10.1126/science.1142021 |
| format | Article |
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The nature and composition of the ¹⁷,¹⁸O-rich reservoir are poorly constrained. We report an in situ discovery of a chemically and isotopically unique material distributed ubiquitously in fine-grained matrix of a primitive carbonaceous chondrite Acfer 094. This material formed by oxidation of Fe,Ni-metal and sulfides by water either in the solar nebula or on a planetesimal. Oxygen isotopic composition of this material indicates that the water was highly enriched in ¹⁷O and ¹⁸O (δ¹⁷,¹⁸OSMOW = +180[per thousand] per mil), providing the first evidence for an extremely ¹⁷,¹⁸O-rich reservoir in the early solar system.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1142021</identifier><identifier>PMID: 17569827</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Astrophysics ; Carbonaceous chondrites ; Chemical composition ; Chondrites ; Cosmochemistry. Extraterrestrial geology ; Earth sciences ; Earth, ocean, space ; Exact sciences and technology ; Isotope geochemistry ; Isotope geochemistry. Geochronology ; Isotopes ; Magnetite ; Materials ; Meteorites. Tectites. 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The nature and composition of the ¹⁷,¹⁸O-rich reservoir are poorly constrained. We report an in situ discovery of a chemically and isotopically unique material distributed ubiquitously in fine-grained matrix of a primitive carbonaceous chondrite Acfer 094. This material formed by oxidation of Fe,Ni-metal and sulfides by water either in the solar nebula or on a planetesimal. Oxygen isotopic composition of this material indicates that the water was highly enriched in ¹⁷O and ¹⁸O (δ¹⁷,¹⁸OSMOW = +180[per thousand] per mil), providing the first evidence for an extremely ¹⁷,¹⁸O-rich reservoir in the early solar system.</description><subject>Astrophysics</subject><subject>Carbonaceous chondrites</subject><subject>Chemical composition</subject><subject>Chondrites</subject><subject>Cosmochemistry. 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Impactites</subject><subject>Meteoroids</subject><subject>Milky Way</subject><subject>Oxidation-Reduction</subject><subject>Oxygen</subject><subject>Oxygen - analysis</subject><subject>Oxygen Isotopes - analysis</subject><subject>Solar composition</subject><subject>Solar nebulae</subject><subject>Solar System</subject><subject>Solar systems</subject><subject>Water</subject><subject>Water - chemistry</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2007</creationdate><recordtype>article</recordtype><sourceid>EIF</sourceid><recordid>eNqF0s9rFDEUB_Agit1Wz57UUFBPY1-Sya-jlNVWCgXX4nF4O5O0s8xM1mRWnP_ebHew4MGeQnifvAfvG0JeMfjIGFdnqW7dULt8KTlw9oQsGFhZWA7iKVkACFUY0PKIHKe0Acg1K56TI6alsobrBfn6zfUDDmOiwdPxztElxm6iq9BhpKspja6nP3B0kS6H2NZ3rqHtQC8c_pro9e_p1g30MoUxbF16QZ557JJ7OZ8n5Obz8vv5RXF1_eXy_NNVgcqqsbC-FIw5bUtpXe1ryaERvgH0Apkw2jRSNKiMtoyBLLVo7NozbLAxa-FxLU7Ih0PfbQw_dy6NVd-m2nUdDi7sUqVLcb8MmeX7_0tQpixBPQqFYlZKUz4K81wLEniGp__ATdjFIe-l4kxIo6Tcjz07oDqGlKLz1Ta2PcapYlDt863mfKs53_zizdx2t-5d8-DnQDN4NwNMNXY-4lC36cEZy624d68PbpPGEP_W-f7LaNiv7u2h7jFUeBtzj5sVByYAtLGSWfEHw6y_cg</recordid><startdate>20070713</startdate><enddate>20070713</enddate><creator>Sakamoto, Naoya</creator><creator>Seto, Yusuke</creator><creator>Itoh, Shoichi</creator><creator>Kuramoto, Kiyoshi</creator><creator>Fujino, Kiyoshi</creator><creator>Nagashima, Kazuhide</creator><creator>Krot, Alexander N</creator><creator>Yurimoto, Hisayoshi</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>FBQ</scope><scope>IQODW</scope><scope>CGR</scope><scope>CUY</scope><scope>CVF</scope><scope>ECM</scope><scope>EIF</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>8BQ</scope><scope>8FD</scope><scope>C1K</scope><scope>F28</scope><scope>FR3</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9.</scope><scope>KR7</scope><scope>L7M</scope><scope>L~C</scope><scope>L~D</scope><scope>M7N</scope><scope>P64</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope><scope>7X8</scope></search><sort><creationdate>20070713</creationdate><title>Remnants of the Early Solar System Water Enriched in Heavy Oxygen Isotopes</title><author>Sakamoto, Naoya ; Seto, Yusuke ; Itoh, Shoichi ; Kuramoto, Kiyoshi ; Fujino, Kiyoshi ; Nagashima, Kazuhide ; Krot, Alexander N ; Yurimoto, Hisayoshi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a696t-9f4311e79459ecfc520d3fd0af3a13878d53da68791105473d9bf1adad8b3fab3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2007</creationdate><topic>Astrophysics</topic><topic>Carbonaceous chondrites</topic><topic>Chemical composition</topic><topic>Chondrites</topic><topic>Cosmochemistry. 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| identifier | ISSN: 0036-8075 |
| ispartof | Science (American Association for the Advancement of Science), 2007-07, Vol.317 (5835), p.231-233 |
| issn | 0036-8075 1095-9203 |
| language | eng |
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| source | Jstor Complete Legacy; MEDLINE; Science Magazine |
| subjects | Astrophysics Carbonaceous chondrites Chemical composition Chondrites Cosmochemistry. Extraterrestrial geology Earth sciences Earth, ocean, space Exact sciences and technology Isotope geochemistry Isotope geochemistry. Geochronology Isotopes Magnetite Materials Meteorites. Tectites. Impactites Meteoroids Milky Way Oxidation-Reduction Oxygen Oxygen - analysis Oxygen Isotopes - analysis Solar composition Solar nebulae Solar System Solar systems Water Water - chemistry |
| title | Remnants of the Early Solar System Water Enriched in Heavy Oxygen Isotopes |
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