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-IT 地球内部科学・地球惑星テクトニクス

[S-IT21] 核-マントルの相互作用と共進化

2019年5月27日(月) 09:00 〜 10:30 A10 (東京ベイ幕張ホール)

コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、太田 健二(東京工業大学大学院理工学研究科地球惑星科学専攻)、土屋 卓久(愛媛大学地球深部ダイナミクス研究センター)、座長:Anselme Borgeaud土屋 卓久

09:00 〜 09:15

[SIT21-01] The role of stishovite as a deep nitrogen carrier indicated from high-pressure and high-temperature experiments

*福山 鴻1鍵 裕之1井上 徹2,3新名 亨3柿澤 翔3菱田 俊一4佐野 有司5高畑 直人5 (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専攻、3.愛媛大学地球深部ダイナミクス研究センター、4.国立研究開発法人物質・材料研究機構、5.東京大学大気海洋研究所)

キーワード:枯渇した窒素、地球深部窒素循環、プレートテクトニクス、スティショバイト、暗い太陽のパラドクス

Nitrogen occupies about 80% in the Earth's atmosphere and is one of essential elements of life. For these reasons, nitrogen is an important volatile element in various aspects of geoscience, including climates (e.g. Goldblatt et al., 2009; Wordsworth and Pierrehumbert, 2013) and the origin of life. However, we couldn't have still understood details of behavior or cycle of nitrogen in the Earth's interior. For example, it is known that the amount of nitrogen in deep Earth is more depleted than that of other volatile elements (Marty, 2012). This is called "missing" nitrogen and suggested to be caused by nitrogen stored in the upper mantle, the mantle transition zone, and the lower mantle through magma ocean from experimental researches (e.g., Li et al., 2013; Yoshioka et al., 2018). However, only two experiments corresponding to the lower mantle were conducted in the previous study (Yoshioka et al., 2018). In addition, subducting slab have played important role for volatile cycle into the deep Earth.

In this research, in order to investigate how much nitrogen is incorporated into stishovite which can carry nitrogen to the lower mantle, we conducted high-pressure and high-temperature experiments using multi-anvil apparatus installed at Geodynamics Research Center, Ehime University. All experimental pressure conditions were 27 GPa and temperature conditions ranged from 1400 ℃ to 1700 ℃. Fe-FeO buffer was used to control the redox state equal to the lower mantle. Nitrogen in recovered samples were analyzed using NanoSIMS installed at Atmosphere and Ocean Research Institute, The University of Tokyo. Nitrogen implanted standard samples were prepared in order to estimate nitrogen solubility in silicate minerals at National Institute for Materials Science.

A series of experimental results revealed that stishovite can incorporate 39-418 ppm nitrogen which is higher than nitrogen solubility in bridgmanite (5-50 ppm nitrogen solubility reported by Yoshioka et al. (2018)). Stishovite is mainly formed by the transition of nitrogen-rich sedimentary rocks transported to the lower mantle via subducting slabs. Our study suggests that nitrogen would continue to be supplied to the lower mantle via subducting slabs since when the plate tectonics had begun. This implies that "hidden" nitrogen reservoir was formed in the lower mantle approximately 4 billion years ago. Furthermore, this " hidden" nitrogen reservoir may play a role in decreasing high-concentration nitrogen which had enhanced greenhouse effect in the early atmosphere (Goldblatt et al., 2009) to the present nitrogen concentration level. Thus, our experimental results support the young faint Sun paradox explained by high-concentration nitrogen in the early Earth (e.g. Goldblatt et al., 2009; Wordsworth and Pierrehumbert, 2013) and suggest that "missing" nitrogen has been caused by forming a "hidden" nitrogen reservoir in the lower mantle.