{"@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/1362262943348495232.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/j.icarus.2018.04.008"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S0019103517308424?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S0019103517308424?httpAccept=text/plain"}}],"dc:title":[{"@value":"Mars’ growth stunted by an early giant planet instability"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1382262943348495234","@type":"Researcher","foaf:name":[{"@value":"Matthew S. Clement"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943348495232","@type":"Researcher","foaf:name":[{"@value":"Nathan A. Kaib"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943348495235","@type":"Researcher","foaf:name":[{"@value":"Sean N. Raymond"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943348495233","@type":"Researcher","foaf:name":[{"@value":"Kevin J. Walsh"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00191035"}],"prism:publicationName":[{"@value":"Icarus"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"2018-09","prism:volume":"311","prism:startingPage":"340","prism:endingPage":"356"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/","https://www.elsevier.com/legal/tdmrep-license","http://www.elsevier.com/open-access/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:S0019103517308424?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:S0019103517308424?httpAccept=text/plain"}],"createdAt":"2018-04-20","modifiedAt":"2025-11-03","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360009142782519808","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Escape and Accretion by Cratering Impacts: Formulation of Scaling Relations for High-speed Ejecta"}]},{"@id":"https://cir.nii.ac.jp/crid/1360025430625188480","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Collisional erosion of mantle silicate during accretion can set the elevated Fe/Mg ratio of Earth"}]},{"@id":"https://cir.nii.ac.jp/crid/1360290617563405568","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Growing Mars fast: High-resolution GPU simulations of embryo formation"}]},{"@id":"https://cir.nii.ac.jp/crid/1360572092541461120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Mars’ Formation Can Constrain the Primordial Orbits of the Gas Giants"}]},{"@id":"https://cir.nii.ac.jp/crid/1360576118723137152","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Erosion and Accretion by Cratering Impacts on Rocky and Icy Bodies"}]},{"@id":"https://cir.nii.ac.jp/crid/1360580232139218944","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"A rich population of free-floating planets in the Upper Scorpius young stellar association"}]},{"@id":"https://cir.nii.ac.jp/crid/1361412890933863168","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Transforming Dust to Planets"}]},{"@id":"https://cir.nii.ac.jp/crid/1361413119380635520","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Constraining the Formation of the Four Terrestrial Planets in the Solar System"}]},{"@id":"https://cir.nii.ac.jp/crid/2051151842060090624","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Martian moons exploration MMX : sample return mission to Phobos elucidating formation processes of habitable planets"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1016/j.icarus.2018.04.008"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ab9897_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2024.116385_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2021.114305_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.3847/2041-8213/abed56_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/abf6d8_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.1038/s41550-021-01513-x_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.1186/s40623-021-01545-7_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.1007/s11214-018-0533-2_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ab3b0a_references_DOI_8tZHAYNiDbjmT3x5LHiXehfv5P2"}]}