{"@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/1363388846124215040.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1126/science.1168221"}},{"identifier":{"@type":"URI","@value":"https://www.science.org/doi/pdf/10.1126/science.1168221"}}],"dc:title":[{"@value":"Origin of Nucleosynthetic Isotope Heterogeneity in the Solar Protoplanetary Disk"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:p>Stable-isotope variations exist among inner solar system solids, planets, and asteroids, but their importance is not understood. We report correlated, mass-independent variations of titanium-46 and titanium-50 in bulk analyses of these materials. Because titanium-46 and titanium-50 have different nucleosynthetic origins, this correlation suggests that the presolar dust inherited from the protosolar molecular cloud was well mixed when the oldest solar system solids formed, but requires a subsequent process imparting isotopic variability at the planetary scale. We infer that thermal processing of molecular cloud material, probably associated with volatile-element depletions in the inner solar system, resulted in selective destruction of thermally unstable, isotopically anomalous presolar components, producing residual isotopic heterogeneity. This implies that terrestrial planets accreted from thermally processed solids with nonsolar isotopic compositions.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1383388846124214912","@type":"Researcher","foaf:name":[{"@value":"Anne Trinquier"}],"jpcoar:affiliationName":[{"@value":"Center for Stars and Planets, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark."},{"@value":"Bristol Isotope Group, Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK."},{"@value":"Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1383388846124214915","@type":"Researcher","foaf:name":[{"@value":"Tim Elliott"}],"jpcoar:affiliationName":[{"@value":"Center for Stars and Planets, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark."},{"@value":"Bristol Isotope Group, Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK."},{"@value":"Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1383388846124214916","@type":"Researcher","foaf:name":[{"@value":"David Ulfbeck"}],"jpcoar:affiliationName":[{"@value":"Center for Stars and Planets, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark."},{"@value":"Bristol Isotope Group, Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK."},{"@value":"Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1383388846124214913","@type":"Researcher","foaf:name":[{"@value":"Christopher Coath"}],"jpcoar:affiliationName":[{"@value":"Center for Stars and Planets, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark."},{"@value":"Bristol Isotope Group, Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK."},{"@value":"Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1383388846124215040","@type":"Researcher","foaf:name":[{"@value":"Alexander N. Krot"}],"jpcoar:affiliationName":[{"@value":"Center for Stars and Planets, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark."},{"@value":"Bristol Isotope Group, Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK."},{"@value":"Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, USA."}]},{"@id":"https://cir.nii.ac.jp/crid/1383388846124214914","@type":"Researcher","foaf:name":[{"@value":"Martin Bizzarro"}],"jpcoar:affiliationName":[{"@value":"Center for Stars and Planets, Natural History Museum of Denmark, University of Copenhagen, Copenhagen DK-1350, Denmark."},{"@value":"Bristol Isotope Group, Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK."},{"@value":"Hawai'i Institute of Geophysics and Planetology, University of Hawai'i at Manoa, HI 96822, 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":"2009-04-17","prism:volume":"324","prism:number":"5925","prism:startingPage":"374","prism:endingPage":"376"},"reviewed":"false","url":[{"@id":"https://www.science.org/doi/pdf/10.1126/science.1168221"}],"createdAt":"2009-04-16","modifiedAt":"2024-01-10","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050002212667840384","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Combined U-corrected Pb-Pb dating and ²⁶Al-²⁶Mg systematics of individual chondrules - Evidence for a reduced initial abundance of Al-26 amongst inner Solar System chondrules"},{"@value":"Combined U-corrected Pb-Pb dating and 26Al-26Mg 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