{"created":"2023-06-20T15:08:53.866917+00:00","id":38395,"links":{},"metadata":{"_buckets":{"deposit":"5b8ac525-c787-41dd-9b3b-dfb22faa60a9"},"_deposit":{"created_by":1,"id":"38395","owners":[1],"pid":{"revision_id":0,"type":"depid","value":"38395"},"status":"published"},"_oai":{"id":"oai:jaxa.repo.nii.ac.jp:00038395","sets":["1887:1891"]},"author_link":["433172","433168","433170","433171","433169","433167"],"item_5_biblio_info_10":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"1995-12","bibliographicIssueDateType":"Issued"},"bibliographicPageEnd":"109","bibliographicPageStart":"106","bibliographic_titles":[{"bibliographic_title":"第28回月・惑星シンポジウム"},{"bibliographic_title":"Proceedings of the 28th ISAS Lunar and Planetary Symposium","bibliographic_titleLang":"en"}]}]},"item_5_description_17":{"attribute_name":"抄録（英）","attribute_value_mlt":[{"subitem_description":"We investigate analytically the runaway growth of a protoplanet taking into account the disruption of planetesimals, which is made by the high velocity collision between planetesimals. As for the mass distribution of collisional fragments, we adopt a simple model proposed by Dohnanyi (1969). Calculations show that the growth of a protoplanet is accelerated by a factor of 2.5 by the help of the disruption of planetesimals compared with the case of no disruption.","subitem_description_type":"Other"}]},"item_5_description_32":{"attribute_name":"資料番号","attribute_value_mlt":[{"subitem_description":"資料番号: AA0063352028","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":"東京工業大学 理学部　地球惑星科学科"},{"subitem_text_value":"東京工業大学 理学部　地球惑星科学科"},{"subitem_text_value":"東京工業大学 理学部　地球惑星科学科"}]},"item_5_text_7":{"attribute_name":"著者所属（英）","attribute_value_mlt":[{"subitem_text_language":"en","subitem_text_value":"Tokyo Institute of Technology Department of Earth and Planetary Sciences, Faculty of Science"},{"subitem_text_language":"en","subitem_text_value":"Tokyo Institute of Technology Department of Earth and Planetary Sciences, Faculty of Science"},{"subitem_text_language":"en","subitem_text_value":"Tokyo Institute of Technology Department of Earth and Planetary Sciences, Faculty 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":"稲葉, 知士"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"田中, 秀和"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"中澤, 清"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Inaba, Satoshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Tanaka, Hidekazu","creatorNameLang":"en"}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Nakazawa, Kiyoshi","creatorNameLang":"en"}],"nameIdentifiers":[{}]}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"惑星集積","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星集積","subitem_subject_scheme":"Other"},{"subitem_subject":"小惑星衝突","subitem_subject_scheme":"Other"},{"subitem_subject":"微惑星","subitem_subject_scheme":"Other"},{"subitem_subject":"破砕","subitem_subject_scheme":"Other"},{"subitem_subject":"質量分布","subitem_subject_scheme":"Other"},{"subitem_subject":"惑星進化","subitem_subject_scheme":"Other"},{"subitem_subject":"太陽重力","subitem_subject_scheme":"Other"},{"subitem_subject":"加速度","subitem_subject_scheme":"Other"},{"subitem_subject":"超高速衝突","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary accretion","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary accretion","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"asteroid collision","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetesimal","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"fragmentation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"mass distribution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"planetary evolution","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"solar gravitation","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"acceleration","subitem_subject_language":"en","subitem_subject_scheme":"Other"},{"subitem_subject":"hypervelocity impact","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 acceleration of the runaway growth due to collisional disruption","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The acceleration of the runaway growth due to collisional disruption","subitem_title_language":"en"}]},"item_type_id":"5","owner":"1","path":["1891"],"pubdate":{"attribute_name":"公開日","attribute_value":"2015-03-26"},"publish_date":"2015-03-26","publish_status":"0","recid":"38395","relation_version_is_last":true,"title":["The acceleration of the runaway growth due to collisional disruption"],"weko_creator_id":"1","weko_shared_id":-1},"updated":"2023-06-20T22:41:20.984522+00:00"}