日本地球惑星科学連合2022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-IT17] 地球型惑星内部での液体の特性とその役割

2022年5月22日(日) 13:45 〜 15:15 102 (幕張メッセ国際会議場)

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

14:55 〜 15:10

[SIT17-05] Longitudinal wave velocity of sodium aluminosilicate melt at high pressure

*坂巻 竜也1 (1.東北大学大学院理学研究科)

キーワード:longitudinal wave velocity、sodium aluminosilicate melt、high pressure

The longitudinal wave velocity (VP) of sodium aluminosilicate (Na-Al-Silicate: NAS) melt was measured up to 3.7 GPa and 1542 K using the ultrasonic technique combing with synchrotron X-ray diffraction and radiography at BL04B1 of SPring-8. The velocity of NAS melt decreased with pressure up to 3.7 GPa although the NAS glass showed the positive pressure dependence of the velocity.
The VP pressure dependence of NAS melt is completely different from that of diopside melt, which showed a monotonous increase with pressure. The difference in VP pressure dependence results from the degree of the polymerization of the silicate network. NAS melt is polymerized one and the ratio of non-bridging oxygen (NBO) to tetrahedrally cation (T) is 0.5. On the other hand, the NBO/T of diopside melt is 2, which means the melt has depolymerized network. In the case of polymerized melt, the first stage of the pressure-induced structural change is the drastic shrinkage of the void of the network because the cavity of the polymerized network is much larger than that of depolymerized melt. Therefore, the compressibility of the NAS melt is very high at low pressure, and the VP decreases with pressure.
Assuming that the natural composition (e.g., basalt), the NBO/T of the magma generated at the uppermost mantle is about 0.7, which indicates polymerized melt. In this case, the pressure dependence of the velocity may be negative and the high-pressure velocity is smaller than ambient velocity. Thus, the presence of the polymerized melt in the mineral aggregation causes an efficient decrease in the velocity of bulk rock. The velocity anomaly at the shallower region of the Earth’s interior, such as the top of the asthenosphere, can be caused by the existence of a tiny amount of partial melt.