{"@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/1361975843214532736.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1038/s41598-019-56139-x"}},{"identifier":{"@type":"URI","@value":"https://www.nature.com/articles/s41598-019-56139-x.pdf"}},{"identifier":{"@type":"URI","@value":"https://www.nature.com/articles/s41598-019-56139-x"}},{"identifier":{"@type":"DOI","@value":"10.48550/arxiv.1912.12056"}},{"identifier":{"@type":"PMID","@value":"31882613"}}],"resourceType":"学術雑誌論文(journal article)","dc:title":[{"@value":"Transport of impact ejecta from Mars to its moons as a means to reveal Martian history"}],"description":[{"type":"abstract","notation":[{"@value":"<jats:title>Abstract</jats:title><jats:p>Throughout the history of the solar system, Mars has experienced continuous asteroidal impacts. These impacts have produced impact-generated Mars ejecta, and a fraction of this debris is delivered to Earth as Martian meteorites. Another fraction of the ejecta is delivered to the moons of Mars, Phobos and Deimos. Here, we studied the amount and condition of recent delivery of impact ejecta from Mars to its moons. Using state-of-the-art numerical approaches, we report, for the first time, that materials delivered from Mars to its moons are physically and chemically different from the Martian meteorites, which are all igneous rocks with a limited range of ages. We show that Mars ejecta mixed in the regolith of its moons potentially covers all its geological eras and consists of all types of rocks, from sedimentary to igneous. A Martian moons sample-return mission will bring such materials back to Earth, and the samples will provide a wealth of “time-resolved” geochemical information about the evolution of Martian surface environments.</jats:p>"}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1420845751137911424","@type":"Researcher","personIdentifier":[{"@type":"KAKEN_RESEARCHERS","@value":"20814693"},{"@type":"NRID","@value":"1000020814693"},{"@type":"NRID","@value":"9000250471169"},{"@type":"NRID","@value":"9000375858663"},{"@type":"RESEARCHMAP","@value":"https://researchmap.jp/ryukih"}],"foaf:name":[{"@value":"Ryuki 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Usui"}]},{"@id":"https://cir.nii.ac.jp/crid/1381975843214532745","@type":"Researcher","foaf:name":[{"@value":"Kazuhisa Fujita"}]}],"publication":{"publicationIdentifier":[{"@type":"EISSN","@value":"20452322"}],"prism:publicationName":[{"@value":"Scientific Reports"}],"dc:publisher":[{"@value":"Springer Science and Business Media LLC"}],"prism:publicationDate":"2019-12-27","prism:volume":"9","prism:number":"1","prism:startingPage":"19833"},"reviewed":"false","dc:rights":["https://creativecommons.org/licenses/by/4.0","https://creativecommons.org/licenses/by/4.0"],"url":[{"@id":"https://www.nature.com/articles/s41598-019-56139-x.pdf"},{"@id":"https://www.nature.com/articles/s41598-019-56139-x"}],"createdAt":"2019-12-27","modifiedAt":"2022-12-17","foaf:topic":[{"@id":"https://cir.nii.ac.jp/all?q=Earth%20and%20Planetary%20Astrophysics%20(astro-ph.EP)","dc:title":"Earth and Planetary Astrophysics (astro-ph.EP)"},{"@id":"https://cir.nii.ac.jp/all?q=FOS:%20Physical%20sciences","dc:title":"FOS: Physical sciences"},{"@id":"https://cir.nii.ac.jp/all?q=Article","dc:title":"Article"},{"@id":"https://cir.nii.ac.jp/all?q=Astrophysics%20-%20Earth%20and%20Planetary%20Astrophysics","dc:title":"Astrophysics - Earth and Planetary Astrophysics"}],"project":[{"@id":"https://cir.nii.ac.jp/crid/1040000781956268416","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H02990"},{"@type":"JGN","@value":"JP17H02990"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17H02990/"}],"notation":[{"@language":"ja","@value":"衝突剥離過程の解明：天体衝突による惑星間物質輸送への応用"},{"@language":"en","@value":"Study on impact spallation: Material transfer between planetary bodies by impacts"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781959762048","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06454"},{"@type":"JGN","@value":"JP17H06454"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-ORGANIZER-17H06454/"}],"notation":[{"@language":"ja","@value":"水惑星学の創成"},{"@language":"en","@value":"Aqua planetology"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781959777024","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06457"},{"@type":"JGN","@value":"JP17H06457"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-17H06457/"}],"notation":[{"@language":"ja","@value":"太陽系天体における水・物質循環のモデリング"},{"@language":"en","@value":"Modeling of water and material circulations in the solar system objects"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000781994474368","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18H04464"},{"@type":"JGN","@value":"JP18H04464"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PUBLICLY-18H04464/"}],"notation":[{"@language":"ja","@value":"室内・数値衝突実験による氷天体衝突時のエネルギー分配・化学反応過程の解明"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782003488000","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"18K13600"},{"@type":"JGN","@value":"JP18K13600"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-18K13600/"}],"notation":[{"@language":"ja","@value":"多様な地球型惑星が持つ衛星系の起源・進化の統一的理解に向けた理論研究"},{"@language":"en","@value":"Towards understanding the formation and evolution of diverse satellite systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782013497472","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19H00715"},{"@type":"JGN","@value":"JP19H00715"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19H00715/"}],"notation":[{"@language":"ja","@value":"隕石および太古代火成岩の親鉄元素同位体分析による地球形成モデルの構築"},{"@language":"en","@value":"Construction of Earth formation model by isotopic analysis of siderophile elements in meteorites and Archean igneous rocks"}]},{"@id":"https://cir.nii.ac.jp/crid/1040000782014029056","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19H01960"},{"@type":"JGN","@value":"JP19H01960"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19H01960/"}],"notation":[{"@language":"ja","@value":"炭酸塩の揮発性元素同位体分析および化学種解析に基づく火星水環境進化の研究"},{"@language":"en","@value":"Speciation and isotope analyses of volatile elements in carbonates for the evolution of surface environment on Mars"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256844051456","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"15KK0153"},{"@type":"JGN","@value":"JP15KK0153"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-15KK0153/"}],"notation":[{"@language":"ja","@value":"火星の海および表層氷の進化史：火星隕石の地球化学的解析からの制約（国際共同研究強化）"},{"@language":"en","@value":"Meteoritic Evidence for the History of Water on Mars: (Fostering Joint International Research)"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256875808256","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"16H04073"},{"@type":"JGN","@value":"JP16H04073"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-16H04073/"}],"notation":[{"@language":"ja","@value":"火星隕石の地球化学的解析に基づく火星の水の散逸史および表層酸化過程の解明"},{"@language":"en","@value":"Geochemical study of Martian meteorites for the evolution of water and paleo-environment on Mars"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256936477440","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17H06459"},{"@type":"JGN","@value":"JP17H06459"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PLANNED-17H06459/"}],"notation":[{"@language":"ja","@value":"水惑星学創成に向けた太陽系探査"},{"@language":"en","@value":"Solar System Exploration for Aqua-planetology"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256937329792","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17J01269"},{"@type":"JGN","@value":"JP17J01269"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17J01269/"}],"notation":[{"@language":"ja","@value":"多様なリング－衛星系の起源・進化の統一的理解に向けた理論研究"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256951459584","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"17K18812"},{"@type":"JGN","@value":"JP17K18812"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-17K18812/"}],"notation":[{"@language":"ja","@value":"衝突雷: 惑星古環境を探る新たな視点"},{"@language":"en","@value":"Impact-induced lightning: A new perspective on the paleoenvironment of planets"}]},{"@id":"https://cir.nii.ac.jp/crid/1040282256990212736","@type":"Project","projectIdentifier":[{"@type":"KAKEN","@value":"19H00726"},{"@type":"JGN","@value":"JP19H00726"},{"@type":"URI","@value":"https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-19H00726/"}],"notation":[{"@language":"ja","@value":"隕石に刻まれた初期太陽系衝突史の復元"},{"@language":"en","@value":"Reconstruction of impact histories in early solar system based on shock metamorphic features in meteorites"}]}],"relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050295181679762176","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A Material-based Panspermia Hypothesis: The Potential of Polymer Gels and Membraneless Droplets"}]},{"@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 system revealed by the 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MARTIAN METEORITES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643744429312","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Searching for life on Mars and its moons"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298754819810560","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Preliminary design of Martian Moons eXploration (MMX)"}]},{"@id":"https://cir.nii.ac.jp/crid/1360302866839995520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Curation protocol of Phobos sample returned by Martian Moons eXploration"}]},{"@id":"https://cir.nii.ac.jp/crid/1360565165902965760","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Formation of Phobos and Deimos via a giant impact"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567185751455616","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"The potential science and engineering value of samples delivered to Earth by Mars sample return"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567189627944704","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"On the Impact Origin of Phobos and Deimos. 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True Polar Wander and Disk Evolution"}]},{"@id":"https://cir.nii.ac.jp/crid/1360568466003847168","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The Importance of Phobos Sample Return for Understanding the Mars-Moon System"}]},{"@id":"https://cir.nii.ac.jp/crid/1360572092734866304","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Modification of the composition and density of Mercury from late accretion"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574094112091776","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"Martian cratering 8: Isochron refinement and the chronology of Mars"}]},{"@id":"https://cir.nii.ac.jp/crid/1360574095196477952","@type":"Article","relationType":["references"],"jpcoar:relatedTitle":[{"@value":"A Habitable Fluvio-Lacustrine Environment at Yellowknife Bay, Gale Crater, 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