Stability of perovskite (MgSiO3) in the Earth's mantle

被引:81
作者
Saxena, SK
Dubrovinsky, LS
Lazor, P
Cerenius, Y
Haggkvist, P
Hanfland, M
Hu, JZ
机构
[1] EUROPEAN SYNCHROTRON RADIAT FACIL,F-38043 GRENOBLE,FRANCE
[2] CARNEGIE INST WASHINGTON,GEOPHYS LAB,CTR HIGH PRESSURE RES,WASHINGTON,DC 20015
关键词
D O I
10.1126/science.274.5291.1357
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
Available thermodynamic data and seismic models favor perovskite (MgSiO3) as the stable phase in the mantle. MgSiO3 was heated at temperatures from 1900 to 3200 kelvin with a Nd-YAG laser in diamond-anvil cells to study the phase relations at pressures from 45 to 100 gigapascals. The quenched products were studied with synchrotron x-ray radiation. The results show that MgSiO3 broke down to a mixture of MgO (periclase) and SiO2 (stishovite or an unquenchable polymorph) at pressures from 58 to 85 gigapascals. These results imply that perovskite may not be stable in the lower mantle and that it might be necessary to reconsider the compositional and density models of the mantle.
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页码:1357 / 1359
页数:3
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