{"@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/1361981471405735296.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/j.icarus.2005.08.015"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S0019103505003210?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S0019103505003210?httpAccept=text/plain"}}],"dc:title":[{"@value":"Binary near-Earth asteroid formation: Rubble pile model of tidal disruptions"}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381981471405735296","@type":"Researcher","foaf:name":[{"@value":"K WALSH"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471405735297","@type":"Researcher","foaf:name":[{"@value":"D RICHARDSON"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00191035"}],"prism:publicationName":[{"@value":"Icarus"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"2006-01","prism:volume":"180","prism:number":"1","prism:startingPage":"201","prism:endingPage":"216"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:S0019103505003210?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:S0019103505003210?httpAccept=text/plain"}],"createdAt":"2005-10-28","modifiedAt":"2019-01-21","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1360285707160940800","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Photometric observations of 107P/Wilson–Harrington"}]},{"@id":"https://cir.nii.ac.jp/crid/1360286990754069888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Small Solar System Bodies as granular media"}]},{"@id":"https://cir.nii.ac.jp/crid/1360298755615664000","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The ESA Hera Mission: Detailed Characterization of the DART Impact Outcome and of the Binary Asteroid (65803) Didymos"}]},{"@id":"https://cir.nii.ac.jp/crid/1360567182137932544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Collisional elongation: Possible origin of extremely elongated shape of 1I/‘Oumuamua"}]},{"@id":"https://cir.nii.ac.jp/crid/1360857593698667648","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"SPH simulations for shape deformation of rubble-pile asteroids through spinup: The challenge for making top-shaped asteroids Ryugu and Bennu"}]},{"@id":"https://cir.nii.ac.jp/crid/1360865815701393408","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Photometry and Polarimetry of 2010 XC<sub>15</sub>: Observational Confirmation of E-type Near-Earth Asteroid Pair"}]},{"@id":"https://cir.nii.ac.jp/crid/1360869856049783808","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Gravitational disturbance on asteroidal ring systems by close encounter with a small object"}]},{"@id":"https://cir.nii.ac.jp/crid/2050870367116820864","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Towards understanding the dynamical evolution of asteroid 25143 Itokawa : constraints from sample analysis"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1016/j.icarus.2005.08.015"},{"@type":"CROSSREF","@value":"10.1007/s00159-019-0117-5_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2019.03.014_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.3847/psj/ac6f52_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.1186/s40623-015-0185-3_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2021.114505_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.3847/1538-4357/ace88f_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2024.116153_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2011.06.044_references_DOI_8HZTd65piDuSsQYtfriYDmhxqfJ"}]}