日本地球惑星科学連合2025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-IT20] 地球深部科学

2025年5月29日(木) 09:00 〜 10:30 105 (幕張メッセ国際会議場)

コンビーナ:石井 貴之(岡山大学惑星物質研究所)、飯塚 理子(早稲田大学教育学部理学科地球科学専修)、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)、土屋 旬(大阪大学理学研究科宇宙地球科学専攻)、座長:飯塚 理子(早稲田大学教育学部理学科地球科学専修)、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)、石井 貴之(岡山大学惑星物質研究所)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)


09:30 〜 09:45

[SIT20-15] Water Incorporation in the Mantle Transition Zone During Magma Ocean Crystallization

*Longjian Xie1,2,3,4、Michael Walter2Tomoo Katsura3、Fang Xu5、Jianhua Wang2、Yingwei Fei2 (1.Center for High Pressure Science & Technology Advanced Research, Shanghai, 201203, P.R. China、2.Earth & Planets Laboratory, Carnegie Science, Washington DC 20015, USA、3.Bayerisches Geoinstitut, University of Bayreuth, Bayreuth, 95440, Germany.、4.Department of Earth Sciences, University College London, London WC1E6BS, UK.、5.School of Earth Sciences, Zhejiang University, Hangzhou 310058, China)

キーワード:water, mantle transition zone, liquidus phase relations, magma ocean

The mantle transition zone (MTZ) is known for its high water storage capacity and has been proposed to be hydrous (Ohtani, 2021). While slab dehydration is a well-studied mechanism for hydrating the MTZ, with water originating from the surface ocean (Kuritani et al., 2011; Richard et al., 2006), primary water in the deep mantle (Hallis et al., 2015) suggests an alternative source. Residual melt from a deep magma ocean is a potential candidate for this primary water. To investigate the evolution of hydrous magma ocean melts at the boundary between the MTZ and the top of the lower mantle, we determined liquidus phase relations in the MgO-FeO-CaO-Al2O3-SiO2-H2O system at 24 GPa. Our results show that the bridgmanite (brg) + stishovite (st) + melt and bridgmanite (brg) + ferropericlase (fp) + melt boundary curves shift toward Mg-rich melt compositions with decreasing temperature and extend to extremely high H2O contents (~80 mol% H2O). Density calculations reveal that melts along these boundary curves are neutrally buoyant relative to upper lower mantle and MTZ minerals at H2O contents up to ~25 mol%. During late-stage crystallization of a mushy magma ocean, a transient melt-rich layer can form at the top of the lower mantle when melt percolation dominates. As crystallization of this layer exceeds ~98%, hydrous melts (>25 mol% H2O) become buoyant and migrate upward. This process provides a mechanism for hydrating the MTZ from a primary water source, offering new insights into the deep Earth's water cycle.

References:
Hallis, L.J., Huss, G.R., Nagashima, K., Taylor, G.J., Halldórsson, S.A., Hilton, D.R., Mottl, M.J., Meech, K.J., 2015. Evidence for primordial water in Earth’s deep mantle. Science 350, 795–797. https://doi.org/10.1126/science.aac4834
Kuritani, T., Ohtani, E., Kimura, J.-I., 2011. Intensive hydration of the mantle transition zone beneath China caused by ancient slab stagnation. Nat Geosci 4, 713–716. https://doi.org/10.1038/ngeo1250
Ohtani, E., 2021. Hydration and dehydration in Earth’s interior. Annu Rev Earth Planet Sci 49, 253–278. https://doi.org/10.1146/annurev-earth-080320-062509
Richard, G., Bercovici, D., Karato, S.-I., 2006. Slab dehydration in the Earth’s mantle transition zone. Earth Planet Sci Lett 251, 156–167. https://doi.org/10.1016/j.epsl.2006.09.006