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- Lionel G. Vacher
- Department of Physics, Washington University in St. Louis, St. Louis, MO, USA
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- Wataru Fujiya
- Faculty of Science, Ibaraki University, 2-1-1 Bunkyo, Mito, 310-8512 Ibaraki, Japan
書誌事項
- 公開日
- 2022-06-01
- 資源種別
- journal article
- DOI
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- 10.2138/gselements.18.3.175
- 公開者
- Mineralogical Society of America
この論文をさがす
説明
<jats:p>Water played a critical role in the evolution of rocky material and planetesimals in the early Solar System. Many primitive asteroids (the sources of chondrites) accreted a significant amount of water ice and were affected by aqueous alteration and/or fluid-assisted metamorphism. These secondary parent body processes have strongly modified the primary mineralogy of chondrites in favor of a wide diversity of secondary phases that formed by interaction with water. The mineralogical and isotopic characterization of these secondary phases in chondrites and returned samples from hydrous asteroids Ryugu and Bennu can help us reconstruct the dynamical evolution of water in the early Solar System and understand the timing and mechanisms of aqueous alteration on hydrous asteroids.</jats:p>
収録刊行物
-
- Elements
-
Elements 18 (3), 175-180, 2022-06-01
Mineralogical Society of America
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詳細情報 詳細情報について
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- CRID
- 1360021390584189056
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- ISSN
- 18115217
- 18115209
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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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- Crossref
- KAKEN
- OpenAIRE
