STXM-XANES analyses of Murchison meteorite samples captured by aerogel after hypervelocity impacts: A potential implication of organic matter degradation for micrometeoroid collection experiments
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- Yabuta Hikaru
- Department of Earth and Planetary Systems Science, Hiroshima University
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- Hasegawa Sunao
- Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA)
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- Tabata Makoto
- Department of Physics, Chiba University
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- Ito Motoo
- Kochi Institute for Core Sample Research, JAMSTEC
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- Furukawa Yoshihiro
- Department of Earth Science, Tohoku University
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- Nakato Aiko
- Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA)
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- Kilcoyne A. L. David
- Advanced Light Source, Lawrence Berkeley National Laboratory
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- Kobayashi Kensei
- Faculty of Engineering, Yokohama National University
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- Yokobori Shin-ichi
- Department of Applied Life Sciences, Tokyo University of Pharmacy and Life Sciences
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- Imai Eiichi
- Nagaoka University of Technology
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- Kawaguchi Yuko
- Department of Applied Life Sciences, Tokyo University of Pharmacy and Life Sciences
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- Yano Hajime
- Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA)
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- Yamagishi Akihiko
- Department of Applied Life Sciences, Tokyo University of Pharmacy and Life Sciences
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- Okudaira Kyoko
- Research Center for Advanced Information Science and Technology, University of Aizu
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- Kebukawa Yoko
- Faculty of Engineering, Yokohama National University
書誌事項
- 公開日
- 2019
- 資源種別
- journal article
- DOI
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- 10.2343/geochemj.2.0549
- 公開者
- 一般社団法人日本地球化学会
この論文をさがす
説明
<p>The Tanpopo mission is an astrobiology space experiment at the Japanese Experiment Module (JEM) ‘Kibo’ on the International Space Station (ISS). One of the sub-divided themes of the Tanpopo mission is for the intact capture of organic bearing micrometeoroids in low Earth orbit using ultralow density silica aerogel (0.01 g/cm3). In order to evaluate damage to organic matter in micrometeoroids during hyper velocity impacts into the aerogel, Murchison meteorite powdered samples, analogs of organic bearing micrometeoroids, were fired into flight-grade silica aerogel (0.01 g/cm3) using a two-stage light-gas gun with velocities of 4.4 and 5.9 km/s. The recovered Murchison grains were analyzed using scanning transmission X-ray microscopy/X-ray absorption near edge structure (STXM/XANES), transmission electron microscopy (TEM) and nanoscale secondary ion mass spectrometry (NanoSIMS). TEM observation did not show significant modifications of the recovered Murchison grains. Carbon-XANES spectra, however, showed a large depletion of the organic matter after the 5.9 km/s impact, but no such effects nor any significant hydrogen isotopic fractionation were observed after the 4.4 km/s impact.</p>
収録刊行物
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- GEOCHEMICAL JOURNAL
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GEOCHEMICAL JOURNAL 53 (1), 53-67, 2019
一般社団法人日本地球化学会
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詳細情報 詳細情報について
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- CRID
- 1390282763098914944
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- NII論文ID
- 130007593227
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- NII書誌ID
- AA00654975
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- ISSN
- 18805973
- 00167002
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- NDL書誌ID
- 029673111
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- 本文言語コード
- en
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- 資料種別
- journal article
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- データソース種別
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- JaLC
- NDLサーチ
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- CiNii Articles
- KAKEN
- OpenAIRE
- IRDB
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- 抄録ライセンスフラグ
- 使用不可
