{"@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/1361981471038435456.json","@type":"Article","productIdentifier":[{"identifier":{"@type":"DOI","@value":"10.1016/0019-1035(86)90121-1"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:0019103586901211?httpAccept=text/xml"}},{"identifier":{"@type":"URI","@value":"https://api.elsevier.com/content/article/PII:0019103586901211?httpAccept=text/plain"}},{"identifier":{"@type":"NAID","@value":"30022300804"}}],"dc:title":[{"@value":"Settling and growth of dust particles in a laminar phase of a low-mass solar nebula"}],"description":[{"notation":[{"@value":"Abstract   It is considered that some vertical convection as well as possible turbulence in an early phase of solar nebula soon terminates owing to diminution of the temperature dependence of dust opacity due to rapid growth of dust particles. We reexamine settling and growth of dust particles in the subsequent laminar phase of the solar nebula in detail, treating a dust layer as a two-component fluid composed of the dust and the gas. We obtain analytic expressions for the settling path, the growing size, and the settling time. The settling process is divided into two phases, i.e., an early gas-dominant phase and a later dust-dominant phase. So far, only the former phase, where the particle path finally turns from vertical to radial, has been investigated. In the latter phase, dust particles drag the gas, rather than the gas does dust particles. Consequently, the particle path turns from radial to vertical. Dust particles grow most appreciably and rapidly in a radially sweeping phase. The final radii of dust particles at the onset of gravitational instability of the dust layer are 20, 5.9, and 0.60 cm in the Earth's, Jupiter's, and Neptune's zones, respectively. These values are much smaller than those obtained previously by S.J. Weidenschilling [1980, Icarus44, 172–189] and Y. Nakagawa et al. [1981, Icarus45, 517–528]. The total settling times are 1.9 × 103, 4.6 × 103, and 2.8 × 104 years in the above-mentioned three zones, respectively. These are somewhat smaller than those obtained by the previous studies. Most of the settling time is spent in the early vertically settling phase."}]}],"creator":[{"@id":"https://cir.nii.ac.jp/crid/1381981471038435456","@type":"Researcher","foaf:name":[{"@value":"Yoshitsugu Nakagawa"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471038435457","@type":"Researcher","foaf:name":[{"@value":"Minoru Sekiya"}]},{"@id":"https://cir.nii.ac.jp/crid/1381981471038435458","@type":"Researcher","foaf:name":[{"@value":"Chushiro Hayashi"}]}],"publication":{"publicationIdentifier":[{"@type":"PISSN","@value":"00191035"}],"prism:publicationName":[{"@value":"Icarus"}],"dc:publisher":[{"@value":"Elsevier BV"}],"prism:publicationDate":"1986-09","prism:volume":"67","prism:number":"3","prism:startingPage":"375","prism:endingPage":"390"},"reviewed":"false","dc:rights":["https://www.elsevier.com/tdm/userlicense/1.0/"],"url":[{"@id":"https://api.elsevier.com/content/article/PII:0019103586901211?httpAccept=text/xml"},{"@id":"https://api.elsevier.com/content/article/PII:0019103586901211?httpAccept=text/plain"}],"createdAt":"2002-11-11","modifiedAt":"2019-04-03","relatedProduct":[{"@id":"https://cir.nii.ac.jp/crid/1050855035390431360","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@language":"en","@value":"Coagulation Instability in Protoplanetary Disks: A Novel Mechanism Connecting Collisional Growth and Hydrodynamical Clumping of Dust Particles"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216960364544","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Dust and gas density evolution at a radial pressure bump in protoplanetary disks"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216960403968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"The radial dependence of pebble accretion rates: A source of diversity in planetary systems"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002216960485376","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Evolution of protoplanetary discs with magnetically driven disc winds"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002217425099264","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"ACCRETION OF SOLID MATERIALS ONTO CIRCUMPLANETARY DISKS FROM PROTOPLANETARY DISKS"}]},{"@id":"https://cir.nii.ac.jp/crid/1360002220783783680","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"DUST DYNAMICS IN PROTOPLANETARY DISK WINDS DRIVEN BY MAGNETOROTATIONAL TURBULENCE: A MECHANISM FOR FLOATING DUST GRAINS WITH CHARACTERISTIC SIZES"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004232174050944","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"Single planet formation regime in the high-ionization environment: Possible origin of hot Jupiters and super-Earths"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004232399121920","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"United theory of planet formation (i): Tandem regime"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004234380612608","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"INDUCED TURBULENCE AND THE DENSITY STRUCTURE OF THE DUST LAYER IN A PROTOPLANETARY DISK"}]},{"@id":"https://cir.nii.ac.jp/crid/1360004234382419968","@type":"Article","resourceType":"学術雑誌論文(journal article)","relationType":["isReferencedBy"],"jpcoar:relatedTitle":[{"@value":"EFFECTS OF DUST GROWTH AND SETTLING ON THE IONIZATION BY RADIONUCLIDES. 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