{"@context":{"@vocab":"https://cir.nii.ac.jp/schema/1.0/","rdfs":"http://www.w3.org/2000/01/rdf-schema#","dc":"http://purl.org/dc/elements/1.1/","dcterms":"http://purl.org/dc/terms/","foaf":"http://xmlns.com/foaf/0.1/","prism":"http://prismstandard.org/namespaces/basic/2.0/","cinii":"http://ci.nii.ac.jp/ns/1.0/","datacite":"https://schema.datacite.org/meta/kernel-4/","ndl":"http://ndl.go.jp/dcndl/terms/","jpcoar":"https://github.com/JPCOAR/schema/blob/master/2.0/"},"@id":"https://cir.nii.ac.jp/crid/1363388844310290048.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1126/science.1228858"}},{"identifier":{"@type":"URI","@value":"https://www.science.org/doi/pdf/10.1126/science.1228858"}}],"dc:title":[{"@value":"Unique Meteorite from Early Amazonian Mars: Water-Rich Basaltic Breccia Northwest Africa 7034"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>So Different and So Similar</jats:title>\n          <jats:p>\n            Most known meteorites from Mars fit into one class.\n            <jats:bold>\n              Agee\n              <jats:italic>et al.</jats:italic>\n            </jats:bold>\n            (p.\n            <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" issue=\"6121\" page=\"780\" related-article-type=\"in-this-issue\" vol=\"339\" xlink:href=\"10.1126/science.1228858\">780</jats:related-article>\n            , published online 3 January; see the Perspective by\n            <jats:bold>\n              <jats:related-article xmlns:xlink=\"http://www.w3.org/1999/xlink\" ext-link-type=\"doi\" issue=\"6121\" page=\"771\" related-article-type=\"in-this-issue\" vol=\"339\" xlink:href=\"10.1126/science.1232490\">Humayun</jats:related-article>\n            </jats:bold>\n            ) describe a meteorite, NWA 7034, which shares some characteristics with other martian meteorites but does not fit within the usual classification. NWA 7034 matches the composition of Mars' surface but is also richer in water than other martian meteorites, and has different oxygen isotope composition, which suggests the existence of multiple oxygen isotopic reservoirs within Mars. Its radiometric age of 2.1 billion years makes it a unique sample of the Amazonian period on Mars.\n          </jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380017675662175370","@type":"Researcher","foaf:name":[{"@value":"Carl B. Agee"}],"jpcoar:affiliationName":[{"@value":"Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA."},{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175361","@type":"Researcher","foaf:name":[{"@value":"Nicole V. Wilson"}],"jpcoar:affiliationName":[{"@value":"Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA."},{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175373","@type":"Researcher","foaf:name":[{"@value":"Francis M. McCubbin"}],"jpcoar:affiliationName":[{"@value":"Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA."},{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175360","@type":"Researcher","foaf:name":[{"@value":"Karen Ziegler"}],"jpcoar:affiliationName":[{"@value":"Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175372","@type":"Researcher","foaf:name":[{"@value":"Victor J. Polyak"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175374","@type":"Researcher","foaf:name":[{"@value":"Zachary D. Sharp"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175371","@type":"Researcher","foaf:name":[{"@value":"Yemane Asmerom"}],"jpcoar:affiliationName":[{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175364","@type":"Researcher","foaf:name":[{"@value":"Morgan H. Nunn"}],"jpcoar:affiliationName":[{"@value":"Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175365","@type":"Researcher","foaf:name":[{"@value":"Robina Shaheen"}],"jpcoar:affiliationName":[{"@value":"Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175367","@type":"Researcher","foaf:name":[{"@value":"Mark H. Thiemens"}],"jpcoar:affiliationName":[{"@value":"Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175366","@type":"Researcher","foaf:name":[{"@value":"Andrew Steele"}],"jpcoar:affiliationName":[{"@value":"Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175375","@type":"Researcher","foaf:name":[{"@value":"Marilyn L. Fogel"}],"jpcoar:affiliationName":[{"@value":"Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175369","@type":"Researcher","foaf:name":[{"@value":"Roxane Bowden"}],"jpcoar:affiliationName":[{"@value":"Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175368","@type":"Researcher","foaf:name":[{"@value":"Mihaela Glamoclija"}],"jpcoar:affiliationName":[{"@value":"Geophysical Lab, Carnegie Institution of Washington, Washington, DC 20005, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175362","@type":"Researcher","foaf:name":[{"@value":"Zhisheng Zhang"}],"jpcoar:affiliationName":[{"@value":"Department of Chemistry and Biochemistry, University of California, San Diego, La Jolla, CA 92093, USA."},{"@value":"School of Environmental Science and Engineering, Sun Yat-Sen University, Guangzhou 510275, China."}]},{"@id":"https://cir.nii.ac.jp/crid/1380017675662175363","@type":"Researcher","foaf:name":[{"@value":"Stephen M. Elardo"}],"jpcoar:affiliationName":[{"@value":"Institute of Meteoritics, University of New Mexico, Albuquerque, NM 87131, USA."},{"@value":"Department of Earth and Planetary Sciences, University of New Mexico, Albuquerque, NM 87131, USA."}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00368075"},{"@type":"EISSN","@value":"10959203"}],"prism:publicationName":[{"@value":"Science"}],"dc:publisher":[{"@value":"American Association for the Advancement of Science (AAAS)"}],"prism:publicationDate":"2013-02-15","prism:volume":"339","prism:number":"6121","prism:startingPage":"780","prism:endingPage":"785"},"reviewed":"false","url":[{"@id":"https://www.science.org/doi/pdf/10.1126/science.1228858"}],"createdAt":"2013-01-04","modifiedAt":"2024-01-10","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050307746540945536","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"The Mars 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