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-CG 固体地球科学複合領域・一般

[S-CG54] 地球惑星科学におけるレオロジーと破壊・摩擦の物理

2019年5月28日(火) 10:45 〜 12:15 A09 (東京ベイ幕張ホール)

コンビーナ:田阪 美樹(島根大学)、桑野 修(国立研究開発法人 海洋研究開発機構)、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)、石橋 秀巳(静岡大学理学部地球科学専攻)、座長:桑野 修(国立研究開発法人海洋研究開発機構)、清水 以知子

11:45 〜 12:00

[SCG54-05] 摩擦熔融時におけるチャートの粘性すべり挙動

*本橋 銀太1大橋 聖和2氏家 恒太郎1 (1.筑波大学、2.山口大学)

キーワード:摩擦熔融、チャート、高速摩擦実験

Pelagic chert is one of the major lithology in accretionary complexes. Thus, frictional properties of chert at seismic slip rates are important for understanding of earthquake faulting in subduction zones. Here, we conducted high-velocity friction experiments on chert collected from the Jurassic accretionary complex in central Japan at a slip rate of 1.3 m/s and normal stresses of 5–13 MPa under room humidity conditions. The results show that initial slip weakening was followed by slip strengthening and subsequent second slip weakening toward a steady-state shear strength. Slip strengthening resulted from the formation of a silica-rich melt layer (experimentally generated pseudotachylyte) at lower melting temperatures than expected. The chemical composition of the pseudotachylyte matrix suggests the frictional melting of quartz with a small amount of illite, which may contribute to reduce melting temperatures. The second slip weakening occurred despite an increasing shear strain rate because of the thinning of the melt layer, implying that the viscosity of the melt layer decreased with slip. The estimated temperatures before and after the second slip weakening and microstructural and chemical features of experimentally generated pseudotachylytes suggest that the viscosity decrease during the second slip weakening is not due to a change in the chemical composition of melt layer, but rather a temperature increase in the melt layer.