{"created":"2023-06-20T14:52:27.303951+00:00","id":20595,"links":{},"metadata":{"_buckets":{"deposit":"4049a498-c054-4ba6-b983-4bd847f1f442"},"_deposit":{"created_by":1,"id":"20595","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20595"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020595","sets":["1543:1778:1792","1887:1891"]},"author_link":["196446","196448","196444","196447","196445","196443"],"item_5_alternative_title_1":{"attribute_name":"その他のタイトル","attribute_value_mlt":[{"subitem_alternative_title":"木星のサブネビュラにおけるダストの衝突成長に対する不完全固着の影響"}]},"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2004-02","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"68","bibliographicPageStart":"65","bibliographic_titles":[{"bibliographic_title":"第37回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 37th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"The Galilean satellites are considered to have been formed in the Jovian subnebula, which was produced during the gas capture of proto-Jupiter, according to the similar scenario to the planet formation in the solar nebula. However, it is not well understood whether or not all of elementary steps of the satellite formation are described by the scaled-down planet formation processes because the subnebula is so different from the solar nebula in temperature, density, time scale, and so on. In this study, concerned is the collisional growth of dust, the first stage of the satellite formation. During the growth due to mutual collisions, the dust particles fall toward Jupiter due to gas drag. Falling velocity strongly depends on the size of dust particles, and the particles with radius of 10(exp -2) to 1 m fall fastest. For a minimum mass Jovian subnebula model (Mosqueira and Estrada, 2003), the maximum falling velocity is about 120 m/s at the present orbit of Ganymede. At this velocity, a dust particle would reach Jupiter in three months. To form satellitesimals, it is necessary that the time scale of dust growth through this dangerous size range is shorter than that of falling. The time scale of collisional growth is estimated by performing a numerical computation taking it into account that dust particles can not stick when they collide in a very high velocity. Given is 10 m/s as the critical velocity for sticking (Dominik and Tielens, 1996). As a result, obtained is about one month as a minimum growth time. This indicates that the formation of satellitesimals is difficult without considering the effect of the formation of dust concentrated region or (and) the mechanism to increase the critical velocity to form satellitesimals.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0047898017","subitem_description_type":"Other"}]},"item_5_publisher_8":{"attribute_name":"出版者","attribute_value_mlt":[{"subitem_publisher":"宇宙航空研究開発機構宇宙科学研究本部"}]},"item_5_publisher_9":{"attribute_name":"出版者（英）","attribute_value_mlt":[{"subitem_publisher":"Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)"}]},"item_5_text_6":{"attribute_name":"著者所属","attribute_value_mlt":[{"subitem_text_value":"北海道大学 大学院理学研究科"},{"subitem_text_value":"インテック"},{"subitem_text_value":"北海道大学 大学院理学研究科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Hokkaido University Graduate School of Science"},{"subitem_text_language":"en","subitem_text_value":"INTEC Inc."},{"subitem_text_language":"en","subitem_text_value":"Hokkaido University Graduate School of Science"}]},"item_access_right":{"attribute_name":"アクセス権","attribute_value_mlt":[{"subitem_access_right":"metadata only access","subitem_access_right_uri":"http://purl.org/coar/access_right/c_14cb"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorNames":[{"creatorName":"福井, 隆"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"島沢, 竜平"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"倉本, 圭"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Fukui, Takashi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Shimazawa, Ryuhei","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kuramoto, Kiyoshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"衝突成長","subitem_subject_scheme":"Other"},{"subitem_subject":"衛星形成","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽星雲","subitem_subject_scheme":"Other"},{"subitem_subject":"木星","subitem_subject_scheme":"Other"},{"subitem_subject":"気体密度","subitem_subject_scheme":"Other"},{"subitem_subject":"質量密度","subitem_subject_scheme":"Other"},{"subitem_subject":"数値解析","subitem_subject_scheme":"Other"},{"subitem_subject":"模型","subitem_subject_scheme":"Other"},{"subitem_subject":"collisional growth","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"satellite formation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar nebula","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Jupiter","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"gas density","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"mass density","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"numerical analysis","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"model","subitem_subject_language":"en","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"conference paper","resourceuri":"http://purl.org/coar/resource_type/c_5794"}]},"item_title":"The effect of imperfect sticking on the collisional growth of dust in the Jovian subnebula","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The effect of imperfect sticking on the collisional growth of dust in the Jovian subnebula","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1792","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20595","relation_version_is_last":true,"title":["The effect of imperfect sticking on the collisional growth of dust in the Jovian subnebula"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:48:03.054897+00:00"}