{"created":"2023-06-20T14:52:21.668268+00:00","id":20502,"links":{},"metadata":{"_buckets":{"deposit":"10865197-3f4d-49b6-9f39-b3767b8f947e"},"_deposit":{"created_by":1,"id":"20502","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"20502"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00020502","sets":["1543:1778:1790","1887:1891"]},"author_link":["195839","195838","195835","195836","195837","195840"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2006-08-07","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"157","bibliographicPageStart":"154","bibliographic_titles":[{"bibliographic_title":"第39回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 39th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"Solar system has experienced planetary migration in its formation stage. Especially, Neptune has an evidence of outward migration in the 3:2 mean motion resonance in the Kuiper belt objects. In the point of view of planetary formation theory, outer ice giant planet needs planetary migration to shortening its growth time. Several simulations about planetary migration has done, and some results indicate that planet can migrate outward when disk has enough mass, but there are few works to understand the basic mechanism. In our work, we would like to focus attention on the mass flux that step over the planet to formulate the planetary migration. That kind of mass flux works as a fuel of migration.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063505040","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":"名古屋大学 大学院環境学研究科"},{"subitem_text_value":"名古屋大学 大学院環境学研究科"},{"subitem_text_value":"名古屋大学 大学院環境学研究科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Nagoya University Graduate School of Environmental Studies"},{"subitem_text_language":"en","subitem_text_value":"Nagoya University Graduate School of Environmental Studies"},{"subitem_text_language":"en","subitem_text_value":"Nagoya University Graduate School of Environmental Studies"}]},"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":"高橋, 啓介"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"小林, 浩"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"渡邊, 誠一郎"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Takahashi, Keisuke","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Kobayashi, Hiroshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Watanabe, Seiichiro","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"惑星進化","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星移動","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽系進化","subitem_subject_scheme":"Other"},{"subitem_subject":"海王星","subitem_subject_scheme":"Other"},{"subitem_subject":"角運動量","subitem_subject_scheme":"Other"},{"subitem_subject":"原始惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"原始惑星系円盤","subitem_subject_scheme":"Other"},{"subitem_subject":"運動量輸送","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星重力","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary migration","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar system","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar system evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"Neptune","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"angular momentum","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"protoplanet","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"protoplanetary disk","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"momentum transfer","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary gravitation","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":"Formulation of planetary migration","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"Formulation of planetary migration","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1790","1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"20502","relation_version_is_last":true,"title":["Formulation of planetary migration"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-21T03:49:22.661846+00:00"}