日本地球惑星科学連合2023年大会

講演情報

[J] オンラインポスター発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG50] 地球惑星科学におけるレオロジーと破壊・摩擦の物理

2023年5月25日(木) 10:45 〜 12:15 オンラインポスターZoom会場 (19) (オンラインポスター)

コンビーナ:田阪 美樹(静岡大学 )、東 真太郎(東京工業大学 理学院 地球惑星科学系)、清水 以知子(京都大学大学院理学研究科地球惑星科学専攻)、桑野 修(国立研究開発法人 海洋研究開発機構)

現地ポスター発表開催日時 (2023/5/24 17:15-18:45)

10:45 〜 12:15

[SCG50-P07] Ductile fractures evolved from creep cavitation in the down-dip extension of seismogenic fault domains

*Thomas Jing Yi Yeo1,2Norio Shigematsu2Simon Richard Wallis1 (1.Department of Earth and Planetary Science, Graduate School of Science, Tokyo University 、2.Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology, AIST )


キーワード:Electron backscattered diffraction, creep cavitation, fractures, microstructures

Ductile fracture is a phenomenon where severe ductile deformation results in the failure of metals, alloys and rocks at elevated temperatures and has been proposed as an important mechanism to account for tectonic tremors or slow slip in the down-dip extension of the seismogenic faults. We are now studying the possibility that ductile fracture on the micro scale can evolve into large-scale geological structures and to the potential to account for the geophysically observed earthquake-related phenomena using samples of Ryoke myloinites along the Median Tectonic Line in SW Japan. It has been shown that ductile fracture in metals begins with the development of grain-scale cavities which then grow and coalesce (Ashby et al., 1979). To examine how this process affects mylonites, we examined the evolution of micro-voids with increasing ductile strain and in particular their relationship to fractures.

Microstructures of the mylonite samples were analysed using a combination of scanning electron microscope imaging and electron backscattered diffraction (EBSD). Previous work has shown that the samples were deformed at around 350 °C with varying degrees of mylonitisation (or strain) and that the mylonites are locally associated with a crushed zone. Ductile strain was quantified based on the quartz recrystallised fraction, revealed by applying the Gaussian mixture model to electron backscattered diffraction data (Yeo et al, 2023). Creep cavitation can be recognised through the presence of micro-voids, many of which are now filled with secondary precipitated minerals, and documenting these voids can reveal the relationship between cavity density and ductile strain. Current observations show that the number of micro-voids increase as the ductile strain increases towards the crushed zone. These spatial relationships suggest that growth and linking of micro-voids developed during mylonitic deformation may lead to the development of large fractures and rock failure.