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  4. Synthesis and equation of state of perovskites in the (Mg, Fe)(3)Al2Si3O12 system to 177 GPa
 
research article

Synthesis and equation of state of perovskites in the (Mg, Fe)(3)Al2Si3O12 system to 177 GPa

Dorfman, Susannah M.  
•
Shieh, Sean R.
•
Meng, Yue
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2012
Earth And Planetary Science Letters

Natural and synthetic pyrope-almandine compositions from 38 to 100 mol% almandine (Alm38-Alm100) were studied by synchrotron X-ray diffraction in the laser-heated diamond anvil cell to 177 GPa. Single-phase orthorhombic GdFeO3-type perovskites were synthesized across the entire examined compositional range at deep lower mantle pressures, with higher Fe-contents requiring higher synthesis pressures. The formation of perovskite with Alm100 (Fe3Al2Si3O12) composition at 80 GPa marks the first observation of a silicate perovskite in a Fe end-member. Fe-enrichment broadens and lowers the pressure range of the post-perovskite transition for intermediate compositions such as Alm54, but the more Fe-rich Alm100-composition perovskite remains stable to pressures as high as 149 GPa. Volume compression data for the Alm54 and Alm100 compositions were fit to the Birch-Murnaghan equation of state. The compressibility of perovskites synthesized from compositions along the pyrope-almandine join is not strongly sensitive to Fe-content. The compression curves were smooth over the entire measured range, and no evidence for a volume anomaly associated with a spin transition was observed. (C) 2012 Elsevier B.V. All rights reserved.

  • Details
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Type
research article
DOI
10.1016/j.epsl.2012.09.024
Web of Science ID

WOS:000312621600019

Author(s)
Dorfman, Susannah M.  
Shieh, Sean R.
Meng, Yue
Prakapenka, Vitali B.
Duffy, Thomas S.
Date Issued

2012

Publisher

Elsevier Science Bv

Published in
Earth And Planetary Science Letters
Volume

357

Start page

194

End page

202

Subjects

perovskite

•

post-perovskite

•

lower mantle

•

D '' region

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
EPSL  
Available on Infoscience
March 28, 2013
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/91160
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