{"@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/1390282679531453952.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.2343/geochemj.2.0401"}},{"identifier":{"@type":"NDL_BIB_ID","@value":"027080367"}},{"identifier":{"@type":"URI","@value":"http://id.ndl.go.jp/bib/027080367"}},{"identifier":{"@type":"URI","@value":"https://ndlsearch.ndl.go.jp/books/R000000004-I027080367"}},{"identifier":{"@type":"URI","@value":"https://www.jstage.jst.go.jp/article/geochemj/50/1/50_2.0401/_pdf"}},{"identifier":{"@type":"NAID","@value":"130005124703"}}],"dc:title":[{"@language":"en","@value":"Nucleosynthetic isotope anomalies and their cosmochemical significance"}],"dc:language":"en","description":[{"type":"abstract","notation":[{"@language":"en","@value":"Unlike most terrestrial rocks, some meteorites and their mineral components show isotope compositions that are clearly associated with nucleosynthetic processes in stars other than the Sun. Although isotope anomalies of nucleosynthetic origin have been an active research area of isotope cosmochemistry for the past few decades, only recently have planetary-scale isotope anomalies been discovered and confirmed for elements other than the noble gases. The discovery of isotope anomalies of nucleosynthetic origin, especially at the planetary scale, provides new constraints on the evolution of the young Solar System. They are the most direct evidence for tracing the origin of extraterrestrial samples, understanding their genetic relationships, and deciphering the stellar environment of Solar System formation. In this paper, we review the progress that has been made in the field of nucleosynthetic isotope anomalies and their cosmochemical significance."}],"abstractLicenseFlag":"disallow"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1410282679531453952","@type":"Researcher","personIdentifier":[{"@type":"NRID","@value":"9000314803957"}],"foaf:name":[{"@language":"en","@value":"Qin Liping"}],"jpcoar:affiliationName":[{"@language":"en","@value":"CAS Key Laboratory of Crust-Mantle Materials and Environment, University of Science and Technology of China"}]},{"@id":"https://cir.nii.ac.jp/crid/1410282679531453953","@type":"Researcher","personIdentifier":[{"@type":"NRID","@value":"9000314803958"}],"foaf:name":[{"@language":"en","@value":"Carlson Richard W."}],"jpcoar:affiliationName":[{"@language":"en","@value":"Department of Terrestrial Magnetism, Carnegie Institution for Science"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00167002"},{"@type":"LISSN","@value":"00167002"},{"@type":"EISSN","@value":"18805973"},{"@type":"NDL_BIB_ID","@value":"000000128646"},{"@type":"ISSN","@value":"00167002"},{"@type":"NCID","@value":"AA00654975"}],"prism:publicationName":[{"@language":"en","@value":"GEOCHEMICAL JOURNAL"},{"@language":"ja","@value":"ＧＥＯＣＨＥＭＩＣＡＬ　ＪＯＵＲＮＡＬ"},{"@language":"en","@value":"Geochem. J."},{"@language":"ja","@value":"Ｇｅｏｃｈｅｍ．　Ｊ．"}],"dc:publisher":[{"@language":"en","@value":"GEOCHEMICAL SOCIETY OF JAPAN"},{"@language":"ja","@value":"一般社団法人日本地球化学会"}],"prism:publicationDate":"2016","prism:volume":"50","prism:number":"1","prism:startingPage":"43","prism:endingPage":"65"},"reviewed":"false","url":[{"@id":"http://id.ndl.go.jp/bib/027080367"},{"@id":"https://ndlsearch.ndl.go.jp/books/R000000004-I027080367"},{"@id":"https://www.jstage.jst.go.jp/article/geochemj/50/1/50_2.0401/_pdf"}],"availableAt":"2016","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=isotope%20anomalies","dc:title":"isotope anomalies"},{"@id":"https://cir.nii.ac.jp/all?q=nucleosynthetic%20effects","dc:title":"nucleosynthetic effects"},{"@id":"https://cir.nii.ac.jp/all?q=metal%20isotopes","dc:title":"metal isotopes"}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050001335841052544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Major element composition of an Early Enriched Reservoir: Constraints from 142Nd/144Nd isotope systematics in the early Earth and high pressure melting experiments of a primitive peridotite"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143589063296","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"An Overview of Isotopic Anomalies in Extraterrestrial Materials and Their Nucleosynthetic Heritage"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011143964436608","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"TUNGSTEN ISOTOPIC COMPOSITIONS IN STARDUST SiC GRAINS FROM THE MURCHISON METEORITE: CONSTRAINTS ON THE<i>s</i>-PROCESS IN THE Hf-Ta-W-Re-Os REGION"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144128862208","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Solar Nebula Heterogeneity in p-Process Samarium and Neodymium Isotopes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144287998720","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nucleosynthesis in Massive Stars with Improved Nuclear and Stellar Physics"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011144609389184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ruthenium endemic isotope effects in chondrites and differentiated meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145108310400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Calcium isotopic anomalies in the Allende meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145396862080","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Extreme 54Cr-rich nano-oxides in the CI chondrite Orgueil – Implication for a late supernova injection into the solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145828474240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Isotopic composition of uranium in chondritic meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011145852409216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<sup>48</sup>\n                    Ca HETEROGENEITY IN DIFFERENTIATED METEORITES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360011146277018368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"48Ca Production in Matter Expanding from High Temperature and Density"}]},{"@id":"https://cir.nii.ac.jp/crid/1360285709360138368","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"INTERSTELLAR DUST PROPERTIES OF M51 FROM<i>AKARI</i>MID-INFRARED IMAGES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619563383168","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Trace‐element concentrations in single circumstellar silicon carbide grains from the Murchison meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619738848768","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The p-process of stellar nucleosynthesis: astrophysics and nuclear physics status"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292619924892160","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Collisional erosion and the non-chondritic composition of the terrestrial planets"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620056181248","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Initial Abundance of\n                    <sup>60</sup>\n                    Fe in the Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620155944704","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ubiquitous isotopic anomalies in Ti from normal Allende inclusions"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620187750400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Non-nucleosynthetic heterogeneity in non-radiogenic stable Hf isotopes: Implications for early solar system chronology"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292620863961344","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nucleosynthetic osmium isotope anomalies in acid leachates of the Murchison meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292621132766336","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Endemic isotopic anomalies in titanium"}]},{"@id":"https://cir.nii.ac.jp/crid/1360292621329805184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"INJECTION OF SUPERNOVA DUST IN NEARBY PROTOPLANETARY DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360299770893362816","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Impact mixing among rocky planetesimals in the early Solar System from angrite oxygen isotopes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574093849257856","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Osmium isotope evidence for uniform distribution of s- and r-process components in the early solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094159525376","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Iron 60 Evidence for Early Injection and Efficient Mixing of Stellar Debris in the Protosolar Nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094163533952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Initial strontium isotopic abundances and the resolution of small time differences in the formation of planetary objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094795489280","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ca ISOTOPE EFFECTS IN ORGUEIL LEACHATES AND THE IMPLICATIONS FOR THE CARRIER PHASES OF\n                    <sup>54</sup>\n                    Cr ANOMALIES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094846260864","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Molybdenum Evidence for Inherited Planetary Scale Isotope Heterogeneity of the Protosolar Nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095079449216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Geochemical arguments for an Earth-like Moon-forming impactor"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095270476032","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Trapped neon in meteorites — II"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095658710784","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Mass-Independent Fractionation of Oxygen: A Novel Isotope Effect and Its Possible Cosmochemical Implications"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095788400128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Galactic Evolution of Sr, Y, and Zr: A Multiplicity of Nucleosynthetic Processes"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095899055360","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Diverse supernova sources of pre-solar material inferred from molybdenum isotopes in meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096391595648","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence of heavy element nucleosynthesis early in the history of the galaxy: The ultra-metal-poor star CS 22892-052"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096397795200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Presolar Grains"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574096440355072","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Fe–Ni and Al–Mg isotope records in UOC chondrules: Plausible stellar source of 60Fe and other short-lived nuclides in the early Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1360846642063711488","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Meteorite zircon constraints on the bulk Lu−Hf isotope composition and early differentiation of the Earth"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848658644017408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The curious case of Mars’ formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360848659312051584","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"PLANETARY-SCALE STRONTIUM ISOTOPIC HETEROGENEITY AND THE AGE OF VOLATILE DEPLETION OF EARLY SOLAR SYSTEM MATERIALS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568732523264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CHROMIUM ISOTOPE SYSTEMATICS OF ACHONDRITES: CHRONOLOGY AND ISOTOPIC HETEROGENEITY OF THE INNER SOLAR SYSTEM BODIES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855568793228800","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Early history of Earth's crust–mantle system inferred from hafnium isotopes in chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855569240097792","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Neutron capture on Pt isotopes in iron meteorites and the Hf–W chronology of core formation in planetesimals"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570147601536","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"147Sm–143Nd and 176Lu–176Hf in eucrites and the differentiation of the HED parent body"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855570933268736","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Confirmation of mass-independent Ni isotopic variability in iron meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571094227328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Contributors to chromium isotope variation of meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571135529600","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"NUCLEOSYNTHETIC TUNGSTEN ISOTOPE ANOMALIES IN ACID LEACHATES OF THE MURCHISON CHONDRITE: IMPLICATIONS FOR HAFNIUM-TUNGSTEN CHRONOMETRY"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571251681920","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Dating the First Stage of Planet Formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360855571538007936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ZIRCONIUM—HAFNIUM ISOTOPE EVIDENCE FROM METEORITES FOR THE DECOUPLED SYNTHESIS OF LIGHT AND HEAVY NEUTRON-RICH NUCLEI"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137043479759232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evolution of the Solar Nebula. VI. Mixing and Transport of Isotopic Heterogeneity"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137043599828480","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The proto-Earth as a significant source of lunar material"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137044818399744","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<sup>146</sup>\n            Sm–\n            <sup>142</sup>\n            Nd systematics measured in enstatite chondrites reveals a heterogeneous distribution of\n            <sup>142</sup>\n            Nd in the solar nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045293769472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evolution and Nucleosynthesis in Low‐Mass Asymptotic Giant Branch Stars. II. Neutron Capture and the<i>s</i>‐Process"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045360427264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Presolar stardust in meteorites: recent advances and scientific frontiers"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137045622518016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Absolute isotopic abundances of Ti in meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046145852032","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Interstellar diamonds in meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1361137046259272960","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chondrite Barium, Neodymium, and Samarium Isotopic Heterogeneity and Early Earth Differentiation"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518738951040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Osmium Isotope Evidence for an\n            <i>s</i>\n            -Process Carrier in Primitive Chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418518965069440","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nucleosynthesis and remnants in massive stars of solar metallicity"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418519368787200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"IRON-60 HETEROGENEITY AND INCOMPLETE ISOTOPE MIXING IN THE EARLY SOLAR SYSTEM"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520020659712","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"s-Process Zirconium in Presolar Silicon Carbide Grains"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520549395328","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Isotopically anomalous TI in presolar SiC from the Murchison meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418520813105024","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Genesis of the Heaviest Elements in the Milky Way Galaxy"}]},{"@id":"https://cir.nii.ac.jp/crid/1361418521236290944","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for supernova injection into the solar nebula and the decoupling of\n            <i>r</i>\n            -process nucleosynthesis"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699993847129984","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<sup>60</sup>\n                    Fe in Chondrites: Debris from a Nearby Supernova in the Early Solar System?"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994279226496","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chromium isotopic anomalies in the Allende meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699994736858752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mass‐Independent Isotope Fractionation of Molybdenum and Ruthenium and the Origin of Isotopic Anomalies in Murchison"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995187942912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Stable-isotopic anomalies and the accretionary assemblage of the Earth and Mars: A subordinate role for carbonaceous chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995342786688","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"<sup>238</sup>\n            U/\n            <sup>235</sup>\n            U Variations in Meteorites: Extant\n            <sup>247</sup>\n            Cm and Implications for Pb-Pb Dating"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995399666816","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"In search of live 247Cm in the early solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995526383232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"NEUTRON-POOR NICKEL ISOTOPE ANOMALIES IN METEORITES"}]},{"@id":"https://cir.nii.ac.jp/crid/1361699995527736320","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Correlated nucleosynthetic isotopic variability in Cr, Sr, Ba, Sm, Nd and Hf in Murchison and QUE 97008"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981468910540672","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Coupled W–Os–Pt isotope systematics in IVB iron meteorites: In situ neutron dosimetry for W isotope chronology"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981469020281472","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The isotopic composition of titanium in the Allende and Leoville meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981469710464256","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Injection of Radioactivities into the Presolar Cloud: Convergence Testing"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981470358671872","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Thoroughly anomalous chromium in Orgueil"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981471190066688","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The identification of meteorite inclusions with isotope anomalies"}]},{"@id":"https://cir.nii.ac.jp/crid/1361981471314342400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Low-temperature isotopic fractionation of uranium"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943466334464","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Interaction of Supernova Ejecta with Nearby Protoplanetary Disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943856621696","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"NEUTRON-RICH CHROMIUM ISOTOPE ANOMALIES IN SUPERNOVA NANOPARTICLES"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262943990311552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Stellar (<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mrow><mml:mi>n</mml:mi><mml:mo>,</mml:mo><mml:mi>γ</mml:mi></mml:mrow></mml:math>) cross sections of<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mmultiscripts><mml:mi mathvariant=\"normal\">Hf</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>174</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>and radioactive<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mmultiscripts><mml:mi mathvariant=\"normal\">Hf</mml:mi><mml:mprescripts/><mml:none/><mml:mrow><mml:mn>182</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944150990208","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evolution of the Solar Nebula. VIII. Spatial and Temporal Heterogeneity of Short‐lived Radioisotopes and Stable Oxygen Isotopes"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944315932544","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"147,146Sm–143,142Nd, 176Lu–176Hf, and 87Rb–87Sr systematics in the angrites: Implications for chronology and processes on the angrite parent body"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944683591552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for live 247Cm in the early Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944721403904","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"More anomalies from the Allende Meteorite: Samarium"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262944961629056","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nickel isotope heterogeneity in the early Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1362262946178011264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Age and isotopic relationships among the angrites Lewis Cliff 86010 and Angra dos Reis"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544418690309632","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Strontium isotopic anomalies in the Allende Meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419043044096","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Prompt Iron Enrichment, Two [ITAL]r[/ITAL]-Process Components, and Abundances in Very Metal-Poor Stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544419248983680","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"O-16 excesses in Murchison and Murray hibonites - A case against a late supernova injection origin of isotopic anomalies in O, Mg, Ca, and TI"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544420958457216","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Synthesis of the Elements in Stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1362544421105585152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The s-process in low-metallicity stars - II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825893581815936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Zirconium isotope evidence for the heterogeneous distribution of s-process materials in the solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894031548672","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Lead Isotopic Ages of Chondrules and Calcium-Aluminum-Rich Inclusions"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894522169344","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Ultra--Metal-poor, Neutron-Capture--rich Giant Star CS 22892-052"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825894606796160","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Excess hafnium‐176 in meteorites and the early Earth zircon record"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895141114240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Molybdenum Isotopic Composition of Individual Presolar Silicon Carbide Grains from the Murchison Meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895300550656","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nucleosynthetic Nd isotope anomalies in primitive enstatite chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825895330737408","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"On the origins of trapped helium, neon and argon isotopic variations in meteorites—II. Carbonaceous meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1362825896169586816","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ca isotopes in refractory inclusions"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368476298624","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nucleosynthesis in Asymptotic Giant Branch Stars: Relevance for Galactic Enrichment and Solar System Formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368612750976","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"correlated O And Mg isotopic anomalies in Allende Inclusions: II. Magnesium"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368659707008","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence of Multiple [CLC][ITAL]r[/ITAL][/CLC]-Process Sites in the Early Galaxy: New Observations of CS 22892−052"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107368845016320","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"S-process BA isotopic compositions in presolar SiC from the Murchison meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369061002240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for a Late Supernova Injection of\n            <sup>60</sup>\n            Fe into the Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369262087936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Ru isotope heterogeneity in the solar protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369418908672","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Extremely Metal‐poor, Neutron Capture–rich Star CS 22892‐052: A Comprehensive Abundance Analysis"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369517866112","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nucleosynthetic components of the early solar system inferred from Ba isotopic compositions in carbonaceous chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369767206400","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Isotopic search for live 135Cs in the early solar system and possibility of 135Cs–135Ba chronometer"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107369787591424","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Calcium-48 isotopic anomalies in bulk chondrites and achondrites: Evidence for a uniform isotopic reservoir in the inner protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370097023232","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nuclear field vs. nucleosynthetic effects as cause of isotopic anomalies in the early Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370158195200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The supernova trigger for formation of the solar system"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107370503354368","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Widespread<sup>54</sup>Cr Heterogeneity in the Inner Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1363107371066399744","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843461767040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Supernovae as the Site of the<i>r</i>‐Process: Implications for Gamma‐Ray Astronomy"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843519677056","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Efficient mixing of the solar nebula from uniform Mo isotopic composition of meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843855045888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Origin of isotopic heterogeneity in the solar nebula by thermal processing and mixing of nebular dust"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388843967105792","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Component of Primitive Nuclear Composition in Carbonaceous Meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844110070912","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Solar system isotopic anomalies: Supernova neighbor or presolar carriers?"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844145824128","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Model of Metallicity Evolution in the Early Universe"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844210677888","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Tungsten Nuclear Anomalies in Planetesimal Cores"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844276375552","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Clues to early Solar System history from chromium isotopes in carbonaceous chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388844590491264","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mn‐Cr isotope systematics of the D'Orbigny angrite"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845670721792","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Presolar isotopic and chemical signatures in hibonite-bearing refractory inclusions from the Murchison carbonaceous chondrite"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845736325504","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Abundance, distribution, and origin of 60Fe in the solar protoplanetary disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845759361152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Rb–Sr chronology of volatile depletion in differentiated protoplanets: BABI, ADOR and ALL revisited"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845829766144","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Injection of Radioactivities into the Forming Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388845862802816","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Lu–Hf and Sm–Nd isotopic composition of CHUR: Constraints from unequilibrated chondrites and implications for the bulk composition of terrestrial planets"}]},{"@id":"https://cir.nii.ac.jp/crid/1363388846124215040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Origin of Nucleosynthetic Isotope Heterogeneity in the Solar Protoplanetary Disk"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670318972927616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The uranium isotopic composition of the Earth and the Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670318992444544","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ORIGIN OF EXCESS<sup>176</sup>Hf IN METEORITES"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319060544512","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319526763136","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"IDENTIFICATION OF AN\n                    <sup>\n                      <b>84</b>\n                    </sup>\n                    Sr-DEPLETED CARRIER IN PRIMITIVE METEORITES AND IMPLICATIONS FOR THERMAL PROCESSING IN THE SOLAR PROTOPLANETARY DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319550401024","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Thermal Ionization Mass Spectrometry"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670319687133312","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mainstream silicon carbide grains from meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670320449940352","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Manganese—chromium isotope systematics and the development of the early Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/1363670321175311872","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"NanoSIMS isotopic analysis of small presolar grains: Search for Si3N4 grains from AGB stars and Al and Ti isotopic compositions of rare presolar SiC grains"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793165429120","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence against a chondritic Earth"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793272260224","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Osmium isotope anomalies in chondrites: Results for acid residues and related leachates"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793886202240","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"53Mn–53Cr systematics of the early Solar System revisited"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951793987949056","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Neutron Capture in Low‐Mass Asymptotic Giant Branch Stars: Cross Sections and Abundance Signatures"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951794973226752","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A search for isotopic anomalies in uranium"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795283558016","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Strontium Isotopic Composition in Individual Circumstellar Silicon Carbide Grains: A Record of<mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" display=\"inline\"><mml:mi mathvariant=\"italic\">s</mml:mi></mml:math>-Process Nucleosynthesis"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795405032448","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"In search of extant Tc in the early solar system: 98Ru and 99Ru abundances in iron meteorites and chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795576935936","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Self-shielding in the solar nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795647975040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Molybdenum Nucleosynthetic Dichotomy Revealed in Primitive Meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1363951795663235200","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Evidence for homogeneous distribution of osmium in the protosolar nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268247169152","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Mixing and Homogenization in the Early Solar System: Clues from Sr, Ba, Nd, and Sm Isotopes in Meteorites"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268401381120","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Nuclear Reactions in Stars and Nucleogenesis"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233268428455680","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"CALCIUM ISOTOPE COMPOSITION OF METEORITES, EARTH, AND MARS"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269257741568","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"ISOTOPE ANOMALIES IN THE FE-GROUP ELEMENTS IN METEORITES AND CONNECTIONS TO NUCLEOSYNTHESIS IN AGB STARS"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233269691415040","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chromium isotopic anomalies in Allende Refractory Inclusions"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270002804864","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Intrinsic W nucleosynthetic isotope variations in carbonaceous chondrites: Implications for W nucleosynthesis and nebular vs. parent body processing of presolar materials"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270419471616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Zirconium isotope evidence for incomplete admixing of r -process components in the solar nebula"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270716852224","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The Weak s-Component and Nucleosynthesis in Massive Stars"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270783245568","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Barium and neodymium isotopic anomalies in the Allende meteorite"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270864492928","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Hf–W mineral isochron for Ca,Al-rich inclusions: Age of the solar system and the timing of core formation in planetesimals"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233270908719616","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The cosmic molybdenum–ruthenium isotope correlation"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233271024189568","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Early solar system timescales according to 53Mn-53Cr systematics"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233271071007488","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Large Ca-48 anomalies are associated with Ti-50 anomalies in Murchison and Murray hibonites"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233271133997184","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Manganese–chromium isotope systematics of carbonaceous chondrites"}]},{"@id":"https://cir.nii.ac.jp/crid/1364233271157373952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Chemical Evolution of the Juvenile Universe"}]},{"@id":"https://cir.nii.ac.jp/crid/1390282679531451008","@type":"Article","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Preface: Evolution of the early solar system: Presolar cosmochemical fingerprints and the formation of watery rocky planets"}]}],"dataSourceIdentifier":[{"@type":"JALC","@value":"oai:japanlinkcenter.org:2000857891"},{"@type":"NDL_SEARCH","@value":"oai:ndlsearch.ndl.go.jp:R000000004-I027080367"},{"@type":"CROSSREF","@value":"10.2343/geochemj.2.0401"},{"@type":"CIA","@value":"130005124703"},{"@type":"CROSSREF","@value":"10.1038/s41550-023-01968-0_references_DOI_MNbWhEzgSH8pwa6qpdtMcS4TspZ"},{"@type":"CROSSREF","@value":"10.1051/0004-6361/201833148_references_DOI_MNbWhEzgSH8pwa6qpdtMcS4TspZ"},{"@type":"CROSSREF","@value":"10.1186/s40645-016-0099-0_references_DOI_MNbWhEzgSH8pwa6qpdtMcS4TspZ"},{"@type":"CROSSREF","@value":"10.2343/geochemj.2.0416_references_DOI_MNbWhEzgSH8pwa6qpdtMcS4TspZ"}]}