{"@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/1362262943634654464.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/j.icarus.2006.12.014"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S0019103506004532?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:S0019103506004532?httpAccept=text/plain"}}],"dc:title":[{"@value":"The effect of YORP on Itokawa"}],"description":[{"notation":[{"@value":"Abstract   The effect of solar radiation on the near-term rotation rate of Asteroid Itokawa via the YORP effect is predicted using the detailed shape model, rotation pole, mass estimate, and optical properties derived from the Hayabusa mission to Itokawa. Based on these estimates Itokawa is decelerating at a rate which will halve its rotation rate in only 50–90 thousand years, a large deceleration that should be detectable in a future appartion. The implications of such a large deceleration for Itokawa's past history are discussed and related to possible seismic shaking."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1380567183441293584","@type":"Researcher","foaf:name":[{"@value":"D.J. Scheeres"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943634654469","@type":"Researcher","foaf:name":[{"@value":"M. Abe"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943634654464","@type":"Researcher","foaf:name":[{"@value":"M. Yoshikawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943634654468","@type":"Researcher","foaf:name":[{"@value":"R. Nakamura"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943634654465","@type":"Researcher","foaf:name":[{"@value":"R.W. Gaskell"}]},{"@id":"https://cir.nii.ac.jp/crid/1382262943634654467","@type":"Researcher","foaf:name":[{"@value":"P.A. Abell"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00191035"}],"prism:publicationName":[{"@value":"Icarus"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"2007-06","prism:volume":"188","prism:number":"2","prism:startingPage":"425","prism:endingPage":"429"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:S0019103506004532?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:S0019103506004532?httpAccept=text/plain"}],"createdAt":"2007-01-09","modifiedAt":"2019-01-10","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050845763137845120","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Thermal and impact histories of 25143 Itokawa recorded in Hayabusa particles"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002215949612288","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Cratering efficiency on coarse-grain targets: Implications for the dynamical evolution of asteroid 25143 Itokawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1360294643725333888","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"YORP Effect on Asteroid 162173 Ryugu: Implications for the Dynamical History"}]},{"@id":"https://cir.nii.ac.jp/crid/1360849942173103872","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Density distribution of asteroid 25143 Itokawa based on smooth terrain shape"}]},{"@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"}]},{"@id":"https://cir.nii.ac.jp/crid/2120870839319803776","@type":"OtherWorks","resourceType":"学術雑誌論文(journal article)","relationType":["isIdenticalTo"],"jpcoar:relatedTitle":[{"@language":"en","@value":"The effect of YORP on Itokawa"}]}],"dataSourceIdentifier":[{"@type":"CROSSREF","@value":"10.1016/j.icarus.2006.12.014"},{"@type":"OPENAIRE","@value":"doi_dedup___::88efc6e54ece540a9a60301c7ac4ce5e"},{"@type":"IRDB","@value":"oai:irdb.nii.ac.jp:01332:0004471310_isIdenticalTo_DOI_S28BQgXKS4HYl4wByCYcdmSctZx"},{"@type":"CROSSREF","@value":"10.1016/j.icarus.2017.09.004_references_DOI_J6AyGbjz7fkfLa2vOPHYhJu8PN6"},{"@type":"CROSSREF","@value":"10.1029/2021je006863_references_DOI_J6AyGbjz7fkfLa2vOPHYhJu8PN6"},{"@type":"CROSSREF","@value":"10.1038/s41598-018-30192-4_references_DOI_J6AyGbjz7fkfLa2vOPHYhJu8PN6"},{"@type":"CROSSREF","@value":"10.1016/j.pss.2019.05.002_references_DOI_J6AyGbjz7fkfLa2vOPHYhJu8PN6"},{"@type":"CROSSREF","@value":"10.1186/s40623-015-0185-3_references_DOI_J6AyGbjz7fkfLa2vOPHYhJu8PN6"}]}