日本地球惑星科学連合2019年大会

講演情報

[E] ポスター発表

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-IT20] 地球型惑星内部での液体の特性とその役割

2019年5月26日(日) 15:30 〜 17:00 ポスター会場 (幕張メッセ国際展示場 8ホール)

コンビーナ:坂巻 竜也(東北大学大学院理学研究科)、中島 陽一(熊本大学大学院先導機構)

[SIT20-P05] High-pressure structural investigations for hydrous sodium silicate melts

*大橋 智典1坂巻 竜也1舟越 賢一2村主 樹1市東 力1柴崎 裕樹3鈴木 昭夫1 (1.東北大学大学院理学系研究科、2.総合科学研究機構 中性子科学センター、3.国立研究開発法人 物質・材料研究機構)

キーワード:含水珪酸塩融体、水の影響、非晶質構造、高温高圧

The behaviors of high-pressure silicate melts, which is controlled by their physico-chemical properties, are important to understand the magma activity in the deep Earth. Particularly, the H2O content significantly affects the properties, such as density (e.g., Sakamaki et al., 2006) and viscosity (e.g., Suzuki et al., 2011; Poe et al., 2006). Since such macroscopic properties are known to be largely determined by the microscopic structure, there are considerable interests in revealing how the structure changes with increasing pressure.

Here, structures of hydrous Na2O-8/3SiO2 melts with 5 wt% (NS8/3_H5) and with 9 wt% H2O (NS8/3_H9) were determined under high pressure and temperature by the in-situ X-ray diffraction (XRD). The in-situ XRD study was carried out using a cubic-type multi-anvil apparatus MAX80, which is installed at the AR-NE5C beamline of PF-AR at Tsukuba, Japan. The experimental P-T conditions were about 1.5–3.0 GPa and 550–970 °C, respectively.

The obtained total structure factors, S(Q) of both liquids show that the position of the first sharp diffraction peaks (FSDP) shift to higher-Q with pressure. This positional shift indicates the intermediate-range order structure of present melts become compact. The reduced radial distribution functions, G(r) indicate different pressure evolutions in the average Si-O bond lengths (rSi-O) depending on their water contents. The rSi-O in the NS8/3_H9 melt shows the monotonic decrease with increasing pressure, however, the rSi-O of the NS8/3_H5 melt hardly changes after its contraction below 1.6 GPa. The structure of the NS8/3_H9 melt is assumed to be slightly more depolymerized than the NS8/3_H5 melt at ambient pressure (Zotov and Keppler, 1998). This difference might be due to a phenomenon that the number of strongly hydrogen-bonded SiOH groups, which are favored in sodium silicate glasses and melts (Xue and Kanzaki, 2004), increase more significantly during pressure-induced depolymerization in the NS8/3_H9 melt than in the NS8/3_H5 melt. This raises Si(-NBO)/Si(-BO) (NBO: non-bridging oxygen, BO: bridging oxygen) ratio, and hence, the rSi-O becomes shorter.