WEKO3
アイテム
{"_buckets": {"deposit": "fd95669e-3808-48d2-ad3c-e546eeeb824a"}, "_deposit": {"created_by": 4, "id": "4506", "owners": [4], "pid": {"revision_id": 0, "type": "depid", "value": "4506"}, "status": "published"}, "_oai": {"id": "oai:nipr.repo.nii.ac.jp:00004506", "sets": ["587"]}, "author_link": ["46522", "7886"], "item_1_biblio_info_14": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1990-10", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "26", "bibliographicPageStart": "19", "bibliographicVolumeNumber": "3", "bibliographic_titles": [{"bibliographic_title": "Proceedings of the NIPR Symposium on Antarctic Meteorites"}]}]}, "item_1_creator_8": {"attribute_name": "著者名(英)", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Wang,Ming-Sheng", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "7886", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Lipschutz,Michael E.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "46522", "nameIdentifierScheme": "WEKO"}]}]}, "item_1_description_1": {"attribute_name": "ページ属性", "attribute_value_mlt": [{"subitem_description": "P(論文)", "subitem_description_type": "Other"}]}, "item_1_description_12": {"attribute_name": "抄録(英)", "attribute_value_mlt": [{"subitem_description": "Contents of siderophile Au, Co and Sb, mobile Ag, Bi, Cd, In, Se, Te, Tl and Zn and lithophile Cs, Ga, Rb and U were determined by RNAA in samples of the lunar meteorite (anorthositic breccia) Yamato (Y)-86032. Contents of the 4 lithophiles in matrix (, 75AM) and anorthositic clast (, 101AC) are similar to those in samples of the other 3 lunar meteorites. This is consistent with all these anorthositic breccias being from the lunar highlands. Contents of the other 11 elements indicate a micrometeorite component of 2.5±1.1% (Cl-equivalent) in the parent regolith of Y-86032,75AM. This value is unusual for lunar samples and is virtually identical to the value for the paired samples Y-82192/3 found in the same bare ice region, suggesting that these 3 specimens derive from the same lunar region in the same impact. No micrometeorite component is detectable in Y-86032,101AC. Slight compositional differences between Y-82192/3 and Y-86032 indicate that they did not travel Earthward as a single rock. Allan Hills-81005 and Y-791197 each exhibit characteristic siderophile/mobile element patterns indicating deviation from different parent regions in separate events. Hence, the 5 lunar meteorites studied thus far derive from 3 distinct impacts.", "subitem_description_type": "Other"}]}, "item_1_identifier_registration": {"attribute_name": "ID登録", "attribute_value_mlt": [{"subitem_identifier_reg_text": "10.15094/00004506", "subitem_identifier_reg_type": "JaLC"}]}, "item_1_publisher_22": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "National Institute of Polar Research"}]}, "item_1_source_id_13": {"attribute_name": "雑誌書誌ID", "attribute_value_mlt": [{"subitem_source_identifier": "AA10784627", "subitem_source_identifier_type": "NCID"}]}, "item_1_text_10": {"attribute_name": "著者所属(英)", "attribute_value_mlt": [{"subitem_text_language": "en", "subitem_text_value": "Department of Chemistry, Purdue University/Department of Chemistry, Purdue University"}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "1990-10-01"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "KJ00000036312.pdf", "filesize": [{"value": "1.2 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_6", "mimetype": "application/pdf", "size": 1200000.0, "url": {"label": "KJ00000036312", "url": "https://nipr.repo.nii.ac.jp/record/4506/files/KJ00000036312.pdf"}, "version_id": "21d19b14-d730-44ba-b609-1b23be3ddc79"}]}, "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": "departmental bulletin paper", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Labile trace elements in lunar meteorite Yamato-86032", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Labile trace elements in lunar meteorite Yamato-86032"}]}, "item_type_id": "1", "owner": "4", "path": ["587"], "permalink_uri": "https://doi.org/10.15094/00004506", "pubdate": {"attribute_name": "公開日", "attribute_value": "1990-10-01"}, "publish_date": "1990-10-01", "publish_status": "0", "recid": "4506", "relation": {}, "relation_version_is_last": true, "title": ["Labile trace elements in lunar meteorite Yamato-86032"], "weko_shared_id": 4}
Labile trace elements in lunar meteorite Yamato-86032
https://doi.org/10.15094/00004506
https://doi.org/10.15094/00004506895d9b12-1e7c-46d7-bdda-321fca13c1ba
名前 / ファイル | ライセンス | アクション |
---|---|---|
KJ00000036312 (1.2 MB)
|
Item type | 紀要論文(ELS) / Departmental Bulletin Paper(1) | |||||
---|---|---|---|---|---|---|
公開日 | 1990-10-01 | |||||
タイトル | ||||||
タイトル | Labile trace elements in lunar meteorite Yamato-86032 | |||||
言語 | ||||||
言語 | eng | |||||
資源タイプ | ||||||
資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
資源タイプ | departmental bulletin paper | |||||
ID登録 | ||||||
ID登録 | 10.15094/00004506 | |||||
ID登録タイプ | JaLC | |||||
ページ属性 | ||||||
内容記述タイプ | Other | |||||
内容記述 | P(論文) | |||||
著者名(英) |
Wang,Ming-Sheng
× Wang,Ming-Sheng× Lipschutz,Michael E. |
|||||
著者所属(英) | ||||||
en | ||||||
Department of Chemistry, Purdue University/Department of Chemistry, Purdue University | ||||||
抄録(英) | ||||||
内容記述タイプ | Other | |||||
内容記述 | Contents of siderophile Au, Co and Sb, mobile Ag, Bi, Cd, In, Se, Te, Tl and Zn and lithophile Cs, Ga, Rb and U were determined by RNAA in samples of the lunar meteorite (anorthositic breccia) Yamato (Y)-86032. Contents of the 4 lithophiles in matrix (, 75AM) and anorthositic clast (, 101AC) are similar to those in samples of the other 3 lunar meteorites. This is consistent with all these anorthositic breccias being from the lunar highlands. Contents of the other 11 elements indicate a micrometeorite component of 2.5±1.1% (Cl-equivalent) in the parent regolith of Y-86032,75AM. This value is unusual for lunar samples and is virtually identical to the value for the paired samples Y-82192/3 found in the same bare ice region, suggesting that these 3 specimens derive from the same lunar region in the same impact. No micrometeorite component is detectable in Y-86032,101AC. Slight compositional differences between Y-82192/3 and Y-86032 indicate that they did not travel Earthward as a single rock. Allan Hills-81005 and Y-791197 each exhibit characteristic siderophile/mobile element patterns indicating deviation from different parent regions in separate events. Hence, the 5 lunar meteorites studied thus far derive from 3 distinct impacts. | |||||
雑誌書誌ID | ||||||
収録物識別子タイプ | NCID | |||||
収録物識別子 | AA10784627 | |||||
書誌情報 |
Proceedings of the NIPR Symposium on Antarctic Meteorites 巻 3, p. 19-26, 発行日 1990-10 |
|||||
出版者 | ||||||
出版者 | National Institute of Polar Research |