日本地球惑星科学連合2014年大会

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セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT38_30PM1] 地球構成物質のレオロジーと物質移動

2014年4月30日(水) 14:15 〜 16:00 511 (5F)

コンビーナ:*大内 智博(愛媛大学地球深部ダイナミクス研究センター)、桑野 修(独立行政法人海洋研究開発機構)、清水 以知子(東京大学大学院理学系研究科地球惑星科学専攻)、座長:辻野 典秀(岡山大学・地球物質科学研究センター)

15:30 〜 15:45

[SIT38-P10_PG] 23GPaまでのCa-Pv及びMg-Pvのその場応力歪測定に関する予備的実験

ポスター講演3分口頭発表枠

*辻野 典秀1山崎 大輔1芳野 極1櫻井 萌2西原 遊3肥後 祐司4 (1.岡山大学・地球物質科学研究センター、2.東京工業大学・地球惑星科学専攻、3.愛媛大学地球深部ダイナミクス研究センター、4.(財)高輝度光科学研究センター)

キーワード:その場観察実験, 変形実験, 応力, 歪, ペロブスカイト, 下部マントル

In order to discuss mantle dynamics in the Earth's interior, knowledge of viscosity of the Earth's lower mantle, which is the highest of the whole mantle, is important. Viscosity models of the Earth's lower mantle were reported by geophysical observations. However, observation values of viscosity have large variety (2~3 order magnitude). Although determination of viscosity of lower mantle minerals by high pressure experiments is needed to understand mantle dynamics, stress-strain relationship for MgSiO3-perovskite (Mg-Pv) and CaSiO3-perovskite (Ca-Pv), which are principal minerals of the Earth's lower mantle, are not reported due to difficulty of high pressure deformation experiments. In this study, we tried in-situ stress-strain measurements of Ca-Pv and Mg-Pv up to 23.0 GPa.
In-situ uniaxial deformation experiments were conducted using a deformation DIA apparatus (SPEED-Mk.II) as Kawai-type apparatus at SPring-8 BL04B1. Experimental conditions of Ca-Pv and Mg-Pv are 13.8 GPa, 1473 K and 23.0 GPa, 1273 K, respectively. cBN anvils, which was transparent material against X-ray, was used along X-ray path. Two-dimensional X-ray diffraction patterns were taken for 120-180 s using CCD detector. To calculate the stress magnitude from the X-ray diffraction data, we used a model of stress-lattice strain relationship (Singh et al. 1998),
dhkl(ψ)= d0hkl [1+(1-3cos2ψ) σ/6 Ghkl] (1)
where dhkl is the d-spacing measured as a function of azimuth angle ψ, d0hkl is the d-spacing under the hydrostatic pressure, Ghkl is the appropriate shear modulus for a given hkl, and σ is the uniaxial stress. Pressure and stress were estimated using Ca-Pv (110) (200) and Au (111) diffraction in Pressure marker (Au : Fo = 1 : 2 volume ratio) at deformation experiments of Ca-Pv and Mg-Pv, respectively. An X-ray radiograph of the strain markers was taken using an imaging system composed of a YAG crystal and a CCD camera with an exposure time of 60 s.
Uniaxial stress of Ca-Pv at 13.8 GPa, 1473 K and ~1.2×10-5 /s and Mg-Pv at 23.0 GPa, 1273 K and ~1.5×10-5 /s were estimated as ~2GPa and ~0.25 GPa , respectively. Stress of Mg-Pv was significantly smaller than that of Ca-Pv though temperature condition of Mg-Pv was lower than that of Ca-Pv. This fact is doubtful. This reason is thought that stress estimated by Au was much smaller than that of Mg-Pv because of framework made by Ringeoodite, which was polymorphic phase of Fo in pressure marker.