Hayabusa analogue sample analysis using synchrotron imaging

• Material Type: 文書・図像類
• Title: Hayabusa analogue sample analysis using synchrotron imaging
• Author/Editor: 土山, 明; 上杉, 健太朗; 中野, 司; Tsuchiyama, Akira; Uesugi, Kentaro; Nakano, Tsukasa
• Author Heading: 土山, 明; 上杉, 健太朗; 中野, 司; Tsuchiyama, Akira; Uesugi, Kentaro; Nakano, Tsukasa
• Publication, Distribution, etc.: 宇宙航空研究開発機構
• Publication Date: 2006-03-31
• Publication Date (W3CDTF): 2006-03-31
• Periodical title: 宇宙航空研究開発機構特別資料 = JAXA Special Publication: The Second Open Competition for the Hayabusa Asteroidal Sample Preliminary Examination Team (HASPET)
• No. or year of volume/issue: JAXA-SP-05-021E
• Volume: JAXA-SP-05-021E
• Pages: 102-145
• ISSN (Periodical Title): ISSN : 1349-113X
• Text Language Code: eng
• Subject Heading: 日本の宇宙計画; はやぶさ; MUSES-C; 小惑星探査機; イトカワ; 計算機トモグラフィー; シンクロトロン放射; 非破壊試験; レゴリス; HASPET; 耐火物; 鉱物学; Japanese space program; Hayabusa; Asteroid Sample-return Spacecraft; Itokawa; computed tomography; synchrotron radiation; nondestructive test; regolith; refractory material; mineralogy
• Target Audience: 一般
• Note (General): Densities of Hayabusa analog samples were measured without contamination using synchrotron X-ray microtomography at BL20XU of SPring-8 and an ultra-microbalance. The density of sample 2-1A is 6.37 +/- 0.02 g/cc. The density of sample 2-1B were scattered (5.05-7.18 g/cc). This may caused by volume estimation problem in the microtomography due to the presence of a large amount of highly absorbed materials (probably Fe-Ni metal) and less absorbed materials (probably silicates). Increment of the number of projection in the tomographic imaging will solve the problem. Three-dimensional grain size distribution of sample 2-1A was obtained by identification of individual grains in the 3-D CT (Computer-aided Tomography) images. This will give the basic physical properties of regolith, which may be present on Itokawa's surface. Several phases were recognized in the 3-D CT images using CT value histograms of the images, and their 3-D distribution maps were obtained with the spatial resolution of down to about 0.5 micrometer. This will helpful for planning later destructive analyses. The density, phase estimation (probably plagioclase, Fe-Mg silicates, troilite, kamacite and taenite in sample 2-1A and Fe-Mg silicates, kamacite and taenite in sample 2-1B if meteorites are assumed) and their modes and textures suggest possibility of an ordinary chondrite (LL (Low iron, Low metal) is favorable) with high petrologic type for sample 2-1A and a stony iron for sample 2-1B although the conclusion cannot be made definitely from the CT images alone. Subtraction microradiography was also applied to sample 2-1A to search Zr-bearing minerals effectively for the Pb-Pb dating. Any Zr-bearing minerals were not observed within the spatial resolution of about a few micrometer, but zircon grains added in sample 2-1A were easily recognized by this method.; 資料番号: AA0063920004; レポート番号: JAXA-SP-05-021E
• Source: https://jaxa.repo.nii.ac.jp/?action=repository_action_common_download&item_id=6108&item_no=1&attribute_id=31&file_no=1
• Access Restrictions: 限定公開
• Data Provider (Database): 国立情報学研究所 : 学術機関リポジトリデータベース（IRDB）（機関リポジトリ）; https://irdb.nii.ac.jp
• Original Data Provider (Database): 宇宙航空研究開発機構 : 宇宙航空研究開発機構リポジトリ