日本地球惑星科学連合2019年大会

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[J] 口頭発表

セッション記号 S (固体地球科学) » S-SS 地震学

[S-SS14] 地震発生の物理・断層のレオロジー

2019年5月29日(水) 09:00 〜 10:30 A05 (東京ベイ幕張ホール)

コンビーナ:岡崎 啓史(海洋研究開発機構)、向吉 秀樹(島根大学大学院総合理工学研究科地球資源環境学領域)、野田 博之(京都大学防災研究所)、吉田 圭佑(東北大学理学研究科附属地震噴火予知研究観測センター)、座長:向吉 秀樹金木 俊也(大阪大学)

09:00 〜 09:15

[SSS14-07] Effect of slickenside on the crustal strength

*安東 淳一1長岡 昂吉1富岡 尚敬2鍵 裕之3ダス カウシク1 (1.広島大学大学院理学研究科地球惑星システム学専攻、2.海洋研究開発機構高知コア研究所、3.東京大学大学院理学系研究科附属地殻化学実験施設)

キーワード:鏡肌、ナノサイズ粒子、剪断実験、断層強度

Slickenside is a glossy and smoothly surface developed on the fault slip plane. Although the slickenside is a common and well-known microstructure, its microstructural characterization and effect on the fault behaviour have not fully studied so far. To understand these points, we characterized the microstructures of natural samples and conducted the frictional experiments. The recovery samples from the experiments were also characterized.

Samples and experiment: The natural samples we characterized were slickensides found on the following rocks collected from several localities. 4-Cherts, 3-Limestones, 1-Amphibolite, 1-Serpentinite, 1-Chromitite, 1-Sandstone, 2-Mudstones, 1-Coaly mudstone and 1-Tuff breccia. The frictional experiments were conducted using limestone and gabbro blocks, and calcite powder with 45 to 75 μm in grain size, with a biaxial friction apparatus. The experimental conditions were 3 - 80 MPa of normal stress, 0.1 m/s and 30 μm/s of slip velocity. The characterization methods of samples were optical microscopy, SEM, TEM, AFM and XANES measurements.
Results and conclusion: The present characterization of natural samples demonstrates that the slickenside is composed of nano-size grains, whose aspect ratio (h/d) of height (h) and diameter (d) is constant at about 0.02 – 0.05 for each sample. These nano-size grains can be identified as same minerals, not amorphous, composed of the parent rocks with some minor exceptions. This fact indicates that the nano-size grains were created during fault slip only by grinding of parent rocks without any reaction including the heating-induced reaction. Therefore, our first conclusion is that the slickenside is a product of aseismic faulting. The slickensides were created by all frictional experiments. The characteristics of these slickensides are same as those of natural samples described above. The interesting results are that the aspect ratio (h/d) of nano-size grains is constant for each experiment and tends to decrease with increasing normal stress from ca. 0.23 to ca. 0.07. The h/d values of nano-size grains composed of natural samples are much smaller than those of the recovered samples, which suggests that the studied natural slickensides were created by faulting at the higher normal stress conditions than at least 80 MPa, and preserved during exhumation from original depth to earth’s surface. This consideration indicates that the fault having slickenside exists at depth corresponding to at least 80 MPa normal stress, ca. 3 km and more. The experimental results using limestone block having pre-existing mirror polished slip plane show that the static and dynamic friction coefficients are very low, ca. 0.3 and 0.2, respectively. In general, it is believed that the frictional sliding on pre-existing fault governs the crustal strength. Therefore, our second conclusion is that the slip behaviour of fault having slickenside might governs the crustal strength. However, the experiments using gabbro block did not show the low static and dynamic friction coefficients. Hence the further detail experiments using simulated slickenside are needed to understand the crustal strength.