{"_buckets": {"deposit": "701f9693-3ece-40c6-80ed-08119f488546"}, "_deposit": {"created_by": 1, "id": "400", "owners": [1], "pid": {"revision_id": 0, "type": "depid", "value": "400"}, "status": "published"}, "_oai": {"id": "oai:ir.soken.ac.jp:00000400", "sets": ["11"]}, "author_link": ["8399", "8397", "8398"], "item_1_biblio_info_21": {"attribute_name": "書誌情報（ソート用）", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2001-09-28", "bibliographicIssueDateType": "Issued"}, "bibliographic_titles": [{}]}]}, "item_1_creator_2": {"attribute_name": "著者名", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "関口, 朋彦"}], "nameIdentifiers": [{"nameIdentifier": "8397", "nameIdentifierScheme": "WEKO"}]}]}, "item_1_creator_3": {"attribute_name": "フリガナ", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "セキグチ, トモヒコ"}], "nameIdentifiers": [{"nameIdentifier": "8398", "nameIdentifierScheme": "WEKO"}]}]}, "item_1_date_granted_11": {"attribute_name": "学位授与年月日", "attribute_value_mlt": [{"subitem_dategranted": "2001-09-28"}]}, "item_1_degree_grantor_5": {"attribute_name": "学位授与機関", "attribute_value_mlt": [{"subitem_degreegrantor": [{"subitem_degreegrantor_name": "総合研究大学院大学"}]}]}, "item_1_degree_name_6": {"attribute_name": "学位名", "attribute_value_mlt": [{"subitem_degreename": "博士（学術）"}]}, "item_1_description_1": {"attribute_name": "ID", "attribute_value_mlt": [{"subitem_description": "2001510", "subitem_description_type": "Other"}]}, "item_1_description_12": {"attribute_name": "要旨", "attribute_value_mlt": [{"subitem_description": "       Icy minor bodies in the outer solar system like TNOs (Trans-Neptunian Objects), Centaurs, cometary nuclei and unusual asteroids are thought to be candidates of planetesimal aggregate bodies in the formation theory of the solar system. Therefore, studies of the physical properties of these objects provide clues to the initial conditions for the solar system. However, their physical properties are still poorly known even the most basic parameters like size and albedo because of their extreme faintness. Typical brightness of TNOs in V-band is fainter than 21 magnitude which makes the use of the largest telescopes an indispensable requirement.\n       Observations were carried out to reveal the characteristics of these faint objects using the largest telescopes. Photometric and low dispersion spectroscopic observations of 16 TNOs and 1 Centaurs in optical and near-IR wavelength were performed for the purpose of colour taxonomical study as the first approach. On the contrary to former studies, absolute magnitude of TNOs and Centaurs shows no significant correlation with the (V-I) colour. Our new measurements of their colours showed no clear bi-modality and continuous diversity from solar to reddened colour of their surface. The surface of TNOs and Centaurs can be modified by resurfacing process of the intrinsic cometary activity. Bi-colour lightcurve observations in high spatial resolution mode, together with deep imasing were performed in order to confirm a cometary activity of TNO 1996 TO66. The inhomogeneous (V - R) colour variation of TNO over one rotation was obtained. It supports the existence of TNO\u0027s patchy surface assumption like Pluto\u0027s spotted surface. However, cometary coma was not detected down to 29 mag/sq.arcsec. As a next step toward the physical studies of these objects, the determination method of the most basic parameters, size and albedo, and the observing feasibility for the outer minor bodies are discussed. As a trial case, the MUSES-C spacecraft mission target, NEA 1998 SF36 was analyzed from thermal observations in mid-IR (N-band). The derived radius and albedo of were 178 (+13/-14) m and 0.29 (+0.05/-0.04), respectively.\n       Finally, the capability of adoption to the faint objects such like TNOs and Centaurs are presented with the possible future facilities. ", "subitem_description_type": "Other"}]}, "item_1_description_18": {"attribute_name": "フォーマット", "attribute_value_mlt": [{"subitem_description": "application/pdf", "subitem_description_type": "Other"}]}, "item_1_description_7": {"attribute_name": "学位記番号", "attribute_value_mlt": [{"subitem_description": "総研大甲第552号", "subitem_description_type": "Other"}]}, "item_1_select_14": {"attribute_name": "所蔵", "attribute_value_mlt": [{"subitem_select_item": "有"}]}, "item_1_select_16": {"attribute_name": "複写", "attribute_value_mlt": [{"subitem_select_item": "複写承諾書なし"}]}, "item_1_select_17": {"attribute_name": "公開状況", "attribute_value_mlt": [{"subitem_select_item": "全文公開可"}]}, "item_1_select_8": {"attribute_name": "研究科", "attribute_value_mlt": [{"subitem_select_item": "数物科学研究科"}]}, "item_1_select_9": {"attribute_name": "専攻", "attribute_value_mlt": [{"subitem_select_item": "09 天文科学専攻"}]}, "item_1_text_10": {"attribute_name": "学位授与年度", "attribute_value_mlt": [{"subitem_text_value": "2001"}]}, "item_1_text_20": {"attribute_name": "業務メモ", "attribute_value_mlt": [{"subitem_text_value": "（2018年1月26日）本籍など個人情報の記載がある旧要旨・審査要旨を個人情報のない新しいものに差し替えた。承諾書を確認した。研究科長宛提出書は図書館にはなし。学位規則変更前のため、本文は国会図書館の自動収集対象外（製本納入）なので、著者版フラグはauthorにする。"}]}, "item_1_version_type_23": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_ab4af688f83e57aa", "subitem_version_type": "AM"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "SEKIGUCHI, Tomohiko", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "8399", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2016-02-17"}], "displaytype": "simple", "download_preview_message": "", "file_order": 0, "filename": "甲552_要旨.pdf", "filesize": [{"value": "208.9 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_11", "mimetype": "application/pdf", "size": 208900.0, "url": {"label": "要旨・審査要旨 / Abstract, Screening Result", "url": "https://ir.soken.ac.jp/record/400/files/甲552_要旨.pdf"}, "version_id": "9d0f3109-610a-4fcc-b971-9631981bec19"}, {"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2016-02-17"}], "displaytype": "simple", "download_preview_message": "", "file_order": 1, "filename": "甲552_本文.pdf", "filesize": [{"value": "3.8 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_11", "mimetype": "application/pdf", "size": 3800000.0, "url": {"label": "本文", "url": "https://ir.soken.ac.jp/record/400/files/甲552_本文.pdf"}, "version_id": "7ad92040-d144-42e4-81a2-8500a6e5d7bf"}]}, "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": "thesis", "resourceuri": "http://purl.org/coar/resource_type/c_46ec"}]}, "item_title": "Physical Observations of Icy Minor Bodies in the Outer Solar System", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Physical Observations of Icy Minor Bodies in the Outer Solar System"}, {"subitem_title": "Physical Observations of Icy Minor Bodies in the Outer Solar System", "subitem_title_language": "en"}]}, "item_type_id": "1", "owner": "1", "path": ["11"], "permalink_uri": "https://ir.soken.ac.jp/records/400", "pubdate": {"attribute_name": "公開日", "attribute_value": "2010-02-22"}, "publish_date": "2010-02-22", "publish_status": "0", "recid": "400", "relation": {}, "relation_version_is_last": true, "title": ["Physical Observations of Icy Minor Bodies in the Outer Solar System"], "weko_shared_id": 1}