Ferromagnesian postperovskite silicates in the D" layer of the Earth

被引:131
作者
Mao, WL
Shen, GY
Prakapenka, VB
Meng, Y
Campbell, AJ
Heinz, DL
Shu, JF
Hemley, RJ
Mao, HK
机构
[1] Univ Chicago, Dept Geophys Sci, Chicago, IL 60637 USA
[2] Carnegie Inst Sci, Geophys Lab, Washington, DC 20015 USA
[3] Univ Chicago, Consortium Adv Radiat Sources, Chicago, IL 60637 USA
[4] Univ Chicago, James Franck Inst, Chicago, IL 60637 USA
[5] Argonne Natl Lab, High Pressure Collaborat Access Team, Argonne, IL 60439 USA
关键词
D O I
10.1073/pnas.0407135101
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Natural olivine with 12 mol % Fe2SiO4 and synthetic orthopyroxenes with 20% and 40% FeSiO3 were studied beyond the pressure-temperature conditions of the core-mantle boundary. All samples were found to convert entirely or partially into the CaIrO3 postperovskite structure, which was recently reported for pure MgSiO3. The incorporation of Fe greatly reduces the pressure needed for the transition and establishes the new phase as the major component of the D" layer. With the liquid core as an unlimited reservoir of iron, core-mantle reactions could further enrich the iron content in this phase and explain the intriguing seismic signatures observed in the D" layer.
引用
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页码:15867 / 15869
页数:3
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