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  1. B200 工学部/工学研究科
  2. B200a 雑誌掲載論文
  3. 学術雑誌

Spin crossover and iron-rich silicate melt in the Earth’s deep mantle

http://hdl.handle.net/2237/20801
http://hdl.handle.net/2237/20801
6b09081d-5231-4906-b07c-898af9bd8d8a
名前 / ファイル ライセンス アクション
Nature_2011.pdf Nature_2011.pdf (6.5 MB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2014-11-18
タイトル
タイトル Spin crossover and iron-rich silicate melt in the Earth’s deep mantle
言語 en
著者 Nomura, Ryuichi

× Nomura, Ryuichi

WEKO 54534

en Nomura, Ryuichi

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Ozawa, Haruka

× Ozawa, Haruka

WEKO 54535

en Ozawa, Haruka

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Tateno, Shigehiko

× Tateno, Shigehiko

WEKO 54536

en Tateno, Shigehiko

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Hirose, Kei

× Hirose, Kei

WEKO 54537

en Hirose, Kei

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Hernlund, John

× Hernlund, John

WEKO 54538

en Hernlund, John

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Muto, Shunsuke

× Muto, Shunsuke

WEKO 54539

en Muto, Shunsuke

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Ishii, Hirofumi

× Ishii, Hirofumi

WEKO 54540

en Ishii, Hirofumi

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Hiraoka, Nozomu

× Hiraoka, Nozomu

WEKO 54541

en Hiraoka, Nozomu

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アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
キーワード
主題Scheme Other
主題 Earth science
抄録
内容記述 A melt has greater volume than a silicate solid of the same composition. But this difference diminishes at high pressure, and the possibility that a melt sufficiently enriched in the heavy element iron might then become more dense than solids at the pressures in the interior of the Earth (and other terrestrial bodies) has long been a source of considerable speculation1, 2. The occurrence of such dense silicate melts in the Earth's lowermost mantle would carry important consequences for its physical and chemical evolution and could provide a unifying model for explaining a variety of observed features in the core–mantle boundary region3. Recent theoretical calculations4 combined with estimates of iron partitioning between (Mg,Fe)SiO3 perovskite and melt at shallower mantle conditions5, 6, 7 suggest that melt is more dense than solids at pressures in the Earth's deepest mantle, consistent with analysis of shockwave experiments8. Here we extend measurements of iron partitioning over the entire mantle pressure range, and find a precipitous change at pressures greater than ~76 GPa, resulting in strong iron enrichment in melts. Additional X-ray emission spectroscopy measurements on (Mg0.95Fe0.05)SiO3 glass indicate a spin collapse around 70 GPa, suggesting that the observed change in iron partitioning could be explained by a spin crossover of iron (from high-spin to low-spin) in silicate melt. These results imply that (Mg,Fe)SiO3 liquid becomes more dense than coexisting solid at ~1,800 km depth in the lower mantle. Soon after the Earth's formation, the heat dissipated by accretion and internal differentiation could have produced a dense melt layer up to ~1,000 km in thickness underneath the solid mantle. We also infer that (Mg,Fe)SiO3 perovskite is on the liquidus at deep mantle conditions, and predict that fractional crystallization of dense magma would have evolved towards an iron-rich and silicon-poor composition, consistent with seismic inferences of structures in the core–mantle boundary region.
言語 en
内容記述タイプ Abstract
出版者
言語 en
出版者 nature publishing group
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ AM
出版タイプResource http://purl.org/coar/version/c_ab4af688f83e57aa
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1038/nature09940
ISSN
収録物識別子タイプ PISSN
収録物識別子 0028-0836
書誌情報 en : Nature

巻 473, p. 199-202, 発行日 2011-05
著者版フラグ
値 author
URI
識別子 http://dx.doi.org/10.1038/nature09940
識別子タイプ DOI
URI
識別子 http://hdl.handle.net/2237/20801
識別子タイプ HDL
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