日本地球惑星科学連合2019年大会

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[E] 口頭発表

セッション記号 S (固体地球科学) » S-GC 固体地球化学

[S-GC40] Volatile Cycles in the Deep Earth - from Subduction Zone to Hot Spot

2019年5月29日(水) 13:45 〜 15:15 A10 (東京ベイ幕張ホール)

コンビーナ:角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、羽生 毅(海洋研究開発機構 地球内部物質循環研究分野)、佐野 有司(東京大学大気海洋研究所海洋地球システム研究系)、Gray E Bebout(Lehigh University)、座長:羽生 毅Gray Bebout(Lehigh University)、佐野 有司角野 浩史

14:30 〜 14:45

[SGC40-03] DH partitioning experiment among high-pressure polymorph of olivine

*佐野 亜沙美1伊藤 正一2井上 徹3野田 昌道3 (1.日本原子力研究開発機構 J-PARCセンター、2.京都大学、3.広島大学)

キーワード:マントル遷移層、オリビン、ワズレアイト、水素同位体

Mantle is known to have homogeneous hydrogen isotope composition with δD = -80 ~ -60 ‰ based on the analysis of MORB and OIB [1, 2]. The reason of the depletion of deuterium compared to the present ocean has been explained by the existence of isolated primordial reservoir in the mantle [1], evolution by the subduction of deuterium-poor hydrous mineral through the geological timescale [3], and addition of cometary water after the formation of ocean [4]. Hydrogen isotope partitioning factor among minerals is a key in these discussions, but little is known under high pressure and high temperature of mantle conditions. In this study we focused on DH partitioning between olivine and wadsleyite, which is a main constituent of upper mantle and mantle transition zone (MTZ). High pressure experiments suggest that wadsleyite and its high pressure polymorph of ringwoodite can contain significant amount of water up to 3.3 wt.% thus MTZ has an ability to keep water up to several times of ocean [5]. Finding of Ringwoodite with 1.4 wt.% H2O in a diamond inclusion also reveals hydrated MTZ at least locally [6].

The partitioning experiment was conducted using Kawai-type multianvil press at GRC, Ehime University. Powder of Mg(OH)2 and Mg(OD)2 was mixed with synthetic olivine so that the starting composition is equivalent to Mg1.8Fe0.2SiO4 + 1.0 wt.% HDO. The sample was sealed in the Au75Pd25 capsule and kept at 1300 °C and around 13 GPa, which is the condition of olivine and wadsleyite coexist. The recovered sample was polished and analyzed by micro-focused X-ray diffractometer, Raman spectroscopy and EPMA. Hydrogen isotope composition was determined using SIMS at Kyoto University.


To test for equilibrium, partitioning experiments are made with changing duration times from 1 h to 72 h. The fractionation factor decreases with increasing of duration time. After keeping for 30 h, 1000lnαOlivine-Wadsleyite seems to reach almost equilibrium around -60 ‰. Assuming that the δD of olivine of upper mantle to -80, the δD of wadsleyite at MTZ become -20 to 0, which is more comparable to the composition of the ocean. The present result shows that the depletion of deuterium of upper mantle can be explained as a result of DH fractionation between upper mantle and MTZ.


[1] Kyser and O’Neil, 1984, Geochim Cosmochim. Acta. [2] Clog et al., 2013, Earth Planet. Sci. Lett. [3] Kurokawa et al., 2018, Earth Planet. Sci. Lett. [4] Kokubu et al., 1961, Geochim. Cosmochim. Acta [5] Smyth et al., 1987, Am. Mineral. [6] Pearson et al., 2014, Nature.