日本地球惑星科学連合2016年大会

講演情報

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-CG57] 流体と沈み込み帯のダイナミクス

2016年5月24日(火) 17:15 〜 18:30 ポスター会場 (国際展示場 6ホール)

コンビーナ:*片山 郁夫(広島大学大学院理学研究科地球惑星システム学専攻)、岡本 敦(東北大学大学院環境科学研究科)、川本 竜彦(京都大学大学院理学研究科附属地球熱学研究施設)、中島 淳一(東京工業大学大学院理工学研究科地球惑星科学専攻)

17:15 〜 18:30

[SCG57-P04] 前弧かんらん岩の加水反応速度に対する実験的制約:有馬型熱水の湧出条件への応用

*中谷 貴之1中村 美千彦1 (1.東北大学大学院理学研究科地学専攻地球惑星物質科学科)

キーワード:加水反応、スラブ流体、蛇紋石、前弧マントル

In order to palce a constraint on the water circulation in subduction zones, hydration rates of peridotites have been investigated experimentally in fore-arc mantle conditions. Experiments were conducted at 400–580°C and 1.3 and 1.8 GPa, where antigorite was expected to form as a stable serpentine phase. Crushed powders of olivine ± orthopyroxene and orthopyroxene + clinopyroxene were reacted with 15 wt% distilled water for 4–19 days. The synthesized serpentine was lizardite in all experimental conditions except that of 1.8 GPa and 580°C in the olivine + orthopyroxene system, in which antigorite was formed. In the olivine + orthopyroxene system, the reactions were interface-controlled except for the reaction at 400°C, which was diffusion-controlled. Corresponding reaction rates were 7.0 × 10-12–1.5 × 10-11 m·s-1 at 500–580°C and 7.5 × 10-16 m2·s-1 at 400°C for the interface- and diffusion-controlled reactions, respectively. Based on a simple reaction-transport model with these hydration rates, we infer that leakage of the slab-derived fluid from an water-unsaturated fore-arc mantle is allowed only when focused flow occurs with a spacing larger than 77–229 km in hot subduction zones like Nankai and Cascadia, whereas the necessary spacing is just 2.3–4.6 m in intermediate-temperature subduction zones like Kyushu and Costa Rica. These calculations suggest that fluid leakage in hot subduction zones may occur after the fore-arc mantle is totally hydrated, while in intermediate-temperature subduction zones, leakage through a water-unsaturated fore-arc mantle may be facilitated.