日本地球惑星科学連合2023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-IT16] 地球深部科学

2023年5月25日(木) 13:45 〜 15:15 302 (幕張メッセ国際会議場)

コンビーナ:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、太田 健二(東京工業大学理学院地球惑星科学系)、河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、座長:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)

13:45 〜 14:00

[SIT16-06] Transformational faulting in metastable Mn2GeO4 olivine: implications for physical mechanisms of deep-focus earthquakes

Feng Shi2,1、*Yanbin Wang1、Timothy Officer1、Tony Yu1、Lupei Zhu3 (1.Center for Advanced Radiation Sources, The University of Chicago、2.State Key Laboratory of Geological Processes and Mineral Resources, School of Earth Sciences, China University of Geosciences, Wuhan, Hubei, China、3.Department of Earth and Atmospheric Sciences, Saint Louis University)

キーワード:intraslab seismicity, deep-focus earthquakes, laboratory earthquake simulation , Acoustic emission, synchrotron , high pressure

The transformational faulting hypothesis postulates that metastable olivine in cold subducting slabs transforms to wadsleyite (a spinelloid) and/or ringwoodite (a spinel) below ~300 km depth, forming localized shear zones leading to deep-focus earthquakes [1]. Detailed physical mechanisms of this hypothesis are still under debate [2, 3]. Several experimental studies have been conducted on an analog olivine Mg2GeO4, which transforms directly to the spinel structure, like ringwoodite. In this study, we examine another analog olivine, Mn2GeO4, which transforms to beta-Mn2GeO4 (a spinelloid isostructural to wadsleyite) at high pressure [4]. Controlled deformation experiments (strain rates from 3x10-5 to 8x10-5 s-1) were conducted on metastable Mn2GeO4 olivine within the beta-Mn2GeO4 stability field (~4-5 GPa and 673 – 1323 K) with acoustic emission (AE) monitoring. Based on the experimental data, the mechanical behavior of metastable Mn2GeO4 olivine is divided into three regimes, depending primarily on temperature. Below ~750 K, olivine is strong but ductile, with no AEs emitted up to ~30% strain. Above ~1150 K, Mn2GeO4 olivine is weak and ductile, with no AEs detected. Only between 750 and 1150 K does metastable Mn2GeO4 olivine behave in a brittle manner, emitting numerous AEs, associated with large stress drops. Scanning and transmission electron microscopy (SEM and TEM) on recovered samples show that all brittle samples contain macroscopic faults. SEM shows that beta-Mn2GeO4 forms primarily sub-parallel long and narrow bands (thickness on the order of 100 nm) cutting through individual olivine grains. Some of the extremely thin shear bands are indicated in Fig. (a) by white arrows. The appearance and topology of these bands are very similar to the nano-shear bands (NSBs) reported in faulted metastable Mg2GeO4 olivine after transformational faulting [2, 3]. Electron back-scattered diffraction (EBSD) reveals that these NSBs are primarily located within the boundaries of olivine kink bands [Fig. (b); same area as in Fig. (a)]. Kink bands have been peviously reporrted in olivines of various compositions (silicates, germanates, etc.) when deformed by low-temperature plasticity [5, 6]. Interestingly, in our Mn2GeO4 sample deformed at similar temperature condition but within the olivine stability field, virtually no kink bands are present. The observed kink bands thus appear to be related to the metastability of olivine and triggered by existing defects or nuclei of beta-Mn2GeO4 within olivine grains. The highly localized spatial distribution of KBBs explains the narrowness of the NSBs. Aided by local temperature increase due to the exothermic nature of the phase transformation, these NSBs propagate and self-organize with increasing deformation, leading to macroscopic failure. Such a micro-mechanism is likely to occur in metastable olivine in subducting slabs below ~300 km depth.
References cited
[1] Green, H. W. and Burnley, P. C., Nature, 341:733-737, 1989.
[2] Riggs, E. M., and Green, H. W., Journal of Geophysical Research-Solid Earth, 110:B03202, 2005.
[3] Wang, Y., Zhu, L., Shi, F., Schubnel, A., et al., Science Advances, 3:e1601896, 2017.
[4] Morimoto, N., Akimoto, S., Koto, K., and Tokonami, M., Physics of the Earth and Planetary Interiors, 3:161-165, 1970.
[5] Raleigh, C. B., Journal of Geophysical Research, 73:5391-5406, 1968.
[6] Burnley, P. C., Cline, C. J., II, and Drue, A., American Mineralogist, 98:927-931, 2013.