日本地球惑星科学連合2018年大会

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[EE] 口頭発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT19] Mineral-melt-fluid interaction and COHN volatile speciation in Earth and planetary

2018年5月20日(日) 10:45 〜 12:15 201B (幕張メッセ国際会議場 2F)

コンビーナ:Mysen Bjorn(Geophysical Laboratory, Carnegie Inst. Washington)、大谷 栄治(東北大学大学院理学研究科地学専攻)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、座長:大谷 栄治(東北大学)

11:00 〜 11:15

[SIT19-08] Incorporation of nitrogen into the lower-mantle minerals under high pressure and high temperature
-Transportation and storage of nitrogen in the deep earth-

*福山 鴻1鍵 裕之1井上 徹2,3新名 亨3柿澤 翔3高畑 直人4佐野 有司4 (1.東京大学大学院理学系研究科附属地殻化学実験施設、2.広島大学大学院理学研究科地球惑星システム学講座、3.愛媛大学地球深部ダイナミクス研究センター、4.東京大学大気海洋研究所)

キーワード:枯渇した窒素、下部マントル、酸化還元状態、スティショバイト、暗い太陽のパラドクス、マルチアンビル高圧発生装置

Nitrogen occupies about 80% of the Earth 's atmosphere and is an essential element of life. Moreover, it is suggested that nitrogen had an impact on the climate in the early Earth (e.g. Goldblatt et al., 2009; Wordsworth and Pierrehumbert, 2013). From these backgrounds, nitrogen is a very important volatile element in discussing the early Earth evolution process and origin of the life. However, we still cannot fully understand the behavior of nitrogen in the deep Earth. For example, nitrogen is depleted compared to other volatile elements in deep mantle (Marty et al., 2012). This is so-called "Missing" nitrogen and it is an important subject in earth science.
In this study, we compared nitrogen incorporation into lower-mantle minerals (bridgmanite, periclase and stishovite) by high-temperature high-pressure experiment using multi-anvil apparatus installed at Geodynamics Research Center, Ehime University under the conditions of 27 GPa and 1600 ℃-1900 ℃. In these experiments, we used Fe-FeO buffer in order to reproduce the redox state of the lower mantle. Two types of starting materials: a powder mixture of SiO2 (quartz) and MgO and a powder mixture of SiO2, MgO, Al2O3 and Mg(OH)2 were used for starting materials. Nitrogen in recovered samples was analyzed using NanoSIMS installed at Atmosphere and Ocean Research Institute.
A series of experimental results revealed that stishovite and periclase can incorporate more nitrogen than bridgmanite. This suggests that periclase, the major mineral in the lower mantle, may be a nitrogen reservoir. Furthermore, the results suggest that stishovite, which is formed by the transition of the SiO2-rich oceanic crustal sedimentary rocks transported to the lower mantle via subducting slabs, can incorporate more nitrogen than bridgmanite (20 ppm nitrogen solubility reported by Yoshioka et al. (2016)). Our study suggests that nitrogen would continue to be supplied to the lower mantle via subducting slabs since approximate 4 billion years ago when the plate tectonics had begun, forming a “Hidden” nitrogen reservoir in the lower mantle. Furthermore, this “Hidden” nitrogen reservoir may play a role in decreasing high-concentration nitrogen which enhanced greenhouse effect in the early atmosphere (Goldblatt et al., 2009) to the present nitrogen concentration level.