Mineralogy and noble gas isotopes of micrometeorites collected from Antarctic snow
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- Material Type
- 記事
- Author/Editor
- Ryuji OkazakiTakaaki NoguchiShin-ichi Tsujimoto
- Publication, Distribution, etc.
- Publication Date
- 2015-06-17
- Publication Date (W3CDTF)
- 2015-06-17
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 67(90)
- Volume
- 67(90)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-015-0261-8
- Persistent ID (NDL)
- info:ndljp/pid/9497169
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2015-09-15T20:13:28+09:00
- Date Captured (W3CDTF)
- 2015-08-20
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/9227920
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- We have investigated seven micrometeorites (MMs) from Antarctic snow collected in 2003 and 2010 by means of electron microscopy, X-ray diffraction, micro-Raman spectroscopy, transmission electron microscopy (TEM) observation, and noble-gas isotope analysis. Isotopic ratios of He and Ne indicate that the noble gases in these MMs are mostly of solar wind (SW). Based on the release patterns of SW [4]He, which should reflect the degree of heating during atmospheric entry, the seven MMs were classified into three types including two least heated, three moderately heated, and two severely heated MMs. The heating degrees are well correlated to their mineralogical features determined by TEM observation. One of the least heated MMs is composed of phyllosilicates, whereas the other consists of anhydrous minerals within which solar flare tracks were observed. The two severely heated MMs show clear evidence of atmospheric heating such as partial melt of the uppermost surface layer in one and abundant patches of dendritic magnetite and Si-rich glass within an olivine grain in the other. It is noteworthy that a moderately heated MM composed of a single crystal of olivine has a [3]He/[4]He ratio of 8.44 × 10[−4], which is higher than the SW value of 4.64 × 10[−4], but does not show a cosmogenic [21]Ne signature such as [20]Ne/[21]Ne/[22]Ne = 12.83/0.0284/1. The isotopic compositions of He and Ne in this sample cannot be explained by mixing of a galactic cosmic ray (GCR)-produced component and SW gases. The high [3]He/[4]He ratio without cosmogenic [21]Ne signature likely indicates the presence of a [3]He-enriched component derived from solar energetic particles.
- DOI
- 10.1186/s40623-015-0261-8
- Access Restrictions
- インターネット公開
- Rights (production)
- © 2015 Okazaki et al. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.
- Related Material (URI)
- Is Referenced By
- A history of mild shocks experienced by the regolith particles on hydrated asteroid RyuguNoble gases and nitrogen in samples of asteroid Ryugu record its volatile sources and recent surface evolutionCollection of Antarctic micrometeorites stored in the surface snow near the Dome Fuji StationHayabusa2 Sample Catcher and Container: Metal-Seal System for Vacuum Encapsulation of Returned Samples with Volatiles and Organic Compounds Recovered from C-Type Asteroid Ryugu微小地球外物質の鉱物科学的研究 ～ちいさきものはみなうつくし～Volcanic ash in bare ice south of Sør Rondane Mountains, Antarctica : geochemistry, rock magnetism and nondestructive magnetic detection with SQUID gradiometer
- References
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- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース学術機関リポジトリデータベース雑誌記事索引データベースCrossrefCiNii ArticlesCiNii Articles科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベースCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- Bibliographic ID (NDL)
- 9497169
- NAID
- 120005758189120006800830