TY - JOUR
T1 - A new high-pressure form of mg 2 sio 4 highlighting diffusionless phase transitions of olivine
AU - Tomioka, Naotaka
AU - Okuchi, Takuo
N1 - Funding Information:
The authors acknowledge M. Ito and Y. Kodama for their technical assistance and anonymous reviewers and Tsuyoshi Ishikawa for their constructive comments. This work was supported by a Grant-in-Aid for Scientific Research (No. 15H03750 to N. T.) and the Strategic Fund for Strengthening Leading-Edge Research and Development provided by the Japan Society for the Promotion of Science (to the Japan Agency for Marine-Earth Science and Technology).
Publisher Copyright:
© The Author(s) 2017.
PY - 2017
Y1 - 2017
N2 - High-pressure polymorphism of olivine (α-phase of Mg 2 SiO 4 ) is of particular interest for geophysicists aiming to understand the structure and dynamics of the Earth’s interior because of olivine’s prominent abundance in the upper mantle. Therefore, natural and synthetic olivine polymorphs have been actively studied in the past half century. Here, we report a new high-pressure polymorph, the ε*-phase, which was discovered in a heavily shocked meteorite. It occurs as nanoscale lamellae and has a topotaxial relationship with the host ringwoodite (γ-phase of Mg 2 SiO 4 ). Olivine in the host rock entrapped in a shock-induced melt vein initially transformed into polycrystalline ringwoodite through a nucleation and growth mechanism. The ringwoodite grains then coherently converted into the ε*-phase by shear transformation during subsequent pressure release. This intermediate metastable phase can be formed by all Mg 2 SiO 4 polymorphs via a shear transformation mechanism. Here, we propose high-pressure transformations of olivine that are enhanced by diffusionless processes, not only in shocked meteorites but also in thick and cold lithosphere subducting into the deep Earth.
AB - High-pressure polymorphism of olivine (α-phase of Mg 2 SiO 4 ) is of particular interest for geophysicists aiming to understand the structure and dynamics of the Earth’s interior because of olivine’s prominent abundance in the upper mantle. Therefore, natural and synthetic olivine polymorphs have been actively studied in the past half century. Here, we report a new high-pressure polymorph, the ε*-phase, which was discovered in a heavily shocked meteorite. It occurs as nanoscale lamellae and has a topotaxial relationship with the host ringwoodite (γ-phase of Mg 2 SiO 4 ). Olivine in the host rock entrapped in a shock-induced melt vein initially transformed into polycrystalline ringwoodite through a nucleation and growth mechanism. The ringwoodite grains then coherently converted into the ε*-phase by shear transformation during subsequent pressure release. This intermediate metastable phase can be formed by all Mg 2 SiO 4 polymorphs via a shear transformation mechanism. Here, we propose high-pressure transformations of olivine that are enhanced by diffusionless processes, not only in shocked meteorites but also in thick and cold lithosphere subducting into the deep Earth.
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U2 - 10.1038/s41598-017-17698-z
DO - 10.1038/s41598-017-17698-z
M3 - Article
C2 - 29229951
AN - SCOPUS:85047923837
SN - 2045-2322
VL - 7
JO - Scientific Reports
JF - Scientific Reports
IS - 1
M1 - 17351
ER -