Ferric iron and aluminum partitioning between MgSiO3- and CaSiO3-perovskites under oxidizing conditions

  • NISHIO-HAMANE Daisuke
    Division of Earth and Planetary Sciences, Graduate School of Science, Hokkaido University
  • SETO Yusuke
    Division of Earth and Planetary Sciences, Graduate School of Science, Hokkaido University
  • NAGAI Takaya
    Division of Earth and Planetary Sciences, Graduate School of Science, Hokkaido University
  • FUJINO Kiyoshi
    Division of Earth and Planetary Sciences, Graduate School of Science, Hokkaido University

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Ferric iron and aluminum partitioning between MgSiO3-dominant perovskite (Mg-Pv) and CaSiO3-dominant perovskite (Ca-Pv) was investigated at 27-100 GPa and 1600-2500 K under oxidizing conditions using a starting composition of 0.85CaMgSi2O6 + 0.15Fe3+AlO3 employing a combined laser-heated diamond anvil cell, synchrotron radiation, and analytical transmission electron microscopy. The product phases were Mg-Pv, Ca-Pv, and a small amount of stishovite at pressures below 30 GPa, while a two-phase assemblage of Mg-Pv and Ca-Pv was identified at pressures above 30 GPa. The appearance of stishovite below 30 GPa indicates the partial formation of an oxygen-deficient perovskite from 2ASiO3 + Fe3+AlO3 = 2AFe3+0.5Al0.5O2.5 (oxygen-deficient perovskite) + 2SiO2 (stishovite), where A = Mg or Ca. The composition of Mg-Pv and Ca-Pv show that ferric iron and aluminum were predominantly incorporated into Mg-Pv under oxidizing conditions, indicating that Mg-Pv is the dominant host phase for ferric iron and aluminum even under highly oxidizing lower mantle conditions.

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詳細情報 詳細情報について

  • CRID
    1390282681523617920
  • NII論文ID
    10019908432
  • NII書誌ID
    AA11460926
  • DOI
    10.2465/jmps.061103
  • ISSN
    13493825
    13456296
  • 本文言語コード
    en
  • データソース種別
    • JaLC
    • Crossref
    • CiNii Articles
  • 抄録ライセンスフラグ
    使用不可

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