日本地球惑星科学連合2022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-IT18] GEOPHYSICAL PROPERTIES AND TRANSPORT PROCESSES IN THE DEEP CRUST AND MANTLE

2022年5月31日(火) 11:00 〜 13:00 オンラインポスターZoom会場 (22) (Ch.22)

コンビーナ:Bjorn Mysen(Geophysical Laboratory, Carnegie Inst. Washington)、コンビーナ:大谷 栄治(東北大学大学院理学研究科地学専攻)、高橋 菜緒子(東北大学大学院理学研究科)、コンビーナ:北 佐枝子(建築研究所)、座長:大谷 栄治(東北大学大学院理学研究科地学専攻)


11:00 〜 13:00

[SIT18-P05] Acoustic wave velocities of ferrous-bearing MgSiO3 glass up to 158 GPa with implications for dense silicate melts at the base of the Earth’s mantle

*増野 いづみ1,2、村上 元彦2、北尾 真司3、三井 隆也4、増田 亮5、瀬戸 誠3 (1.岡山大学惑星物質研究所、2.スイス連邦工科大学チューリッヒ校、3.京都大学、4.量子科学技術研究開発機構、5.弘前大学)

キーワード:ケイ酸塩ガラス、下部マントル、部分溶融

We conducted in-situ high-pressure acoustic wave velocity measurements of Fe2+-bearing MgSiO3 glass up to 158 GPa by means of Brillouin scattering spectroscopy in a diamond anvil cell to clarify the effect of iron on the elasticity and structural evolution of silicate melts in the lower mantle. The change in trend of the acoustic wave velocity profile, likely induced by the structural transition of Si-O coordination number from 6 to 6+ proposed in previous studies of silicate glasses, was confirmed to be located at around 129 GPa. Given the iron contents of partial melts derived from a pyrolitic or chondritic mantle, the transition pressure where Si-O coordination number likely becomes higher than 6 would be at around 125-128 GPa, which is well within the lowermost mantle pressure regime. Our data show the substitution of 12 mol% Fe in MgSiO3 glass decreases the VS by ~5.5 %. This study implies that iron considerably affects the buoyancy relations between melts/crystals and the iron-bearing melts at the lowermost mantle will have the higher coordination number than 6.