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ID 60715
フルテキストURL
fulltext.pdf 1.13 MB
著者
Xie, Longjian Institute for Planetary Materials, Okayama University
Yoneda, Akira Institute for Planetary Materials, Okayama University
Yamazaki, Daisuke Institute for Planetary Materials, Okayama University
Manthilake, Geeth Laboratoire Magmas et Volcans, Université Clermont Auvergne, CNRS, IRD, OPGC
Higo, Yuji Japan Synchrotron Radiation Research Institute
Tange, Yoshinori Japan Synchrotron Radiation Research Institute
Guignot, Nicolas Synchrotron SOLEIL
King, Andrew Synchrotron SOLEIL
Scheel, Mario Synchrotron SOLEIL
Andrault, Denis Laboratoire Magmas et Volcans, Université Clermont Auvergne, CNRS, IRD, OPGC
抄録
Thermochemical heterogeneities detected today in the Earth's mantle could arise from ongoing partial melting in different mantle regions. A major open question, however, is the level of chemical stratification inherited from an early magma-ocean (MO) solidification. Here we show that the MO crystallized homogeneously in the deep mantle, but with chemical fractionation at depths around 1000 km and in the upper mantle. Our arguments are based on accurate measurements of the viscosity of melts with forsterite, enstatite and diopside compositions up to similar to 30 GPa and more than 3000 K at synchrotron X-ray facilities. Fractional solidification would induce the formation of a bridgmanite-enriched layer at similar to 1000 km depth. This layer may have resisted to mantle mixing by convection and cause the reported viscosity peak and anomalous dynamic impedance. On the other hand, fractional solidification in the upper mantle would have favored the formation of the first crust.
発行日
2020-01-28
出版物タイトル
Nature Communications
11巻
1号
出版者
Nature Research
開始ページ
4387
ISSN
2041-1723
NCID
AA12645905
資料タイプ
学術雑誌論文
言語
英語
OAI-PMH Set
岡山大学
著作権者
© The Author(s) 2020
論文のバージョン
publisher
PubMed ID
DOI
Web of Science KeyUT
関連URL
isVersionOf https://doi.org/10.1038/s41467-019-14071-8
ライセンス
http://creativecommons.org/ licenses/by/4.0/
助成機関名
日本学術振興会
助成番号
DC2-JP17J10966