Japan Geoscience Union Meeting 2022

Presentation information

[E] Poster

S (Solid Earth Sciences ) » S-IT Science of the Earth's Interior & Techtonophysics

[S-IT19] Deep Earth Sciences

Mon. May 30, 2022 11:00 AM - 1:00 PM Online Poster Zoom Room (22) (Ch.22)

convener:Kenji Ohta(Department of Earth and Planetary Sciences, Tokyo Institute of Technology), convener:Kenji Kawai(Department of Earth and Planetary Science, School of Science, University of Tokyo), Tsuyoshi Iizuka(University of Tokyo), convener:Jun Tsuchiya(Geodynamics Research Center, Ehime University), Chairperson:Kenji Ohta(Department of Earth and Planetary Sciences, Tokyo Institute of Technology), Jun Tsuchiya(Geodynamics Research Center, Ehime University), Tsuyoshi Iizuka(University of Tokyo), Kenji Kawai(Department of Earth and Planetary Science, School of Science, University of Tokyo)

11:00 AM - 1:00 PM

[SIT19-P05] Amorphization kinetics of bridgmanite at high temperatures

*Masayuki Nishi1, Akihiro Kaneko2, Hiroshi Ohgidani2, Haruhiko Dekura2, Sho Kakizawa3, Shogo Kawaguchi3, Shintaro Kobayashi3, Tatsuhiro Sakaiya1, Tadashi Kondo1 (1.Department of Earth and Space Science, Osaka University, 2.Geodynamics Research Center, Ehime Univerisity, 3.Japan Synchrotron Radiation Research Institute (JASRI))

Keywords:bridgmanite, meteorite, amorphization

High-pressure minerals found in shocked meteorites provide pressure–temperature–time information that can be used to constrain the impact histories of their parent bodies. The occurrence of bridgmanite in shocked meteorites suggests that the peak pressure during the impact process reaches at least ~23 GPa at which bridgmanite is thermodynamically stable. Although most high-pressure phases (e.g., coesite, stishovite, pyrope, ringwoodite, and akimotoite) are kinetically stable below ~800 K at ambient pressure, bridgmanite is amorphized at temperatures above ~400 K. Considering that post-shock temperatures above 400 K are maintained for a long duration in the L6 chondrite, the presence of natural bridgmanite in our environments is unexpected. Despite its importance in the shock histories of meteorites and mantle mineralogy, it remains unclear how bridgmanite is preserved.
To gain insights into the enigmatic existence of bridgmanite in shocked meteorite, we carried out time-resolved high-temperature XRD measurements on synthetic bridgmanite with a composition of MgSiO3 at the synchrotron radiation facilities of SPring-8 (BL02B2). Our results show that the significant volume expansion due to the amorphization induces static stress that can reach up to ~0.5 GPa, which prevents the progress of the amorphization. This time-insensitive amorphization kinetics may have enabled the preservation of bridgmanite in the shocked meteorite that fell on Earth. Also, because natural bridgmanite grains can be distinguished from amorphous ones in the backscattered electron image, the amorphous/crystal fraction can be used to estimate the remnant post-shock temperature. Accordingly, if 10% of bridgmanite remains crystalline, the post-shock temperature conditions can be estimated to be ~600 K, irrespective of the time duration.