日本地球惑星科学連合2016年大会

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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-IT06] Interaction and Coevolution of the Core and Mantle

2016年5月23日(月) 09:00 〜 10:30 304 (3F)

コンビーナ:*田中 聡(海洋研究開発機構 地球深部ダイナミクス研究分野)、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:入舩 徹男(愛媛大学地球深部ダイナミクス研究センター)、鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)

09:45 〜 10:00

[SIT06-04] Reaction between olivine and nitrogen at high pressure and high temperature

*鍵 裕之1久保 俊智1星野 由紀子1八木 健彦1篠崎 彩子2大藤 弘明4中野 智志5中尾 愛子6岡田 卓3 (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.名古屋大学大学院環境学研究科、3.東京大学物性研究所、4.愛媛大学地球深部ダイナミクス研究センター、5.物質材料研究機構、6.理化学研究所)

キーワード:nitrogen, mantle, olivine

Volatiles represented by hydrogen greatly affect deep-earth dynamics. Behavior of volatiles will contribute to understandings of budget of light elements, evolution of the earth, geodynamics and so on. Among volatile components, behavior of nitrogen in the deep earth is still unclear. Nitrogen is a main constituent of atmosphere and also exists in the crust by substituting potassium ions in silicate minerals. Chondrite-normalized nitrogen concentration of the bulk earth is one order of magnitude lower than those other volatiles such as He, Ne, Ar, H2O and so on. There could be a hidden nitrogen reservoir in the deep earth. We are going to test a possibility of a hidden nitrogen reservoir from high pressure and high temperature experiments.
San Carlos olivine or synthetic forsterite were loaded as a starting material in a diamond anvil cell with nitrogen in liquid state or compressed gas (180 MPa). After applying pressure at 5 GPa, a sample was heated using CO2 laser or fiber laser. X-ray diffraction patterns, SEM-EDS images, XPS spectra were obtained on the recovered samples.
XRD measurements on the recovered samples revealed the formation of enstatite (MgSiO3) suggesting the decomposition of Mg2SiO4 into MgSiO3 and MgO. This reaction is contrastive to the reaction occurring in H2 fluid (Shinozaki et al., 2013), Mg2SiO4 decomposed into SiO2 and MgO. Moreover, EDS mapping observations revealed that there are some Mg-rich (Si-depleted) spots.
XPS spectra shown in Fig. 1 revealed that nitrogen was detected from an olivine sample recovered from 5 GPa and 1700 K. Before Ar-sputtering, species assignable to NH4+ is dominant. Presumably, the sample surface is covered with adsorbed molecules. After Ar-sputtering, a broad band attributable to intrinsic nitrogen reacted with the mineral was observed. The present results suggest the formation of nitride species (N3-) in a mantle-derived silicate mineral. This study proposes nitride as a hidden nitrogen reservoir in the deep mantle.