日本地球惑星科学連合2025年大会

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[J] 口頭発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

[M-IS17] 地質学のいま

2025年5月26日(月) 15:30 〜 17:00 201A (幕張メッセ国際会議場)

コンビーナ:辻森 樹(東北大学)、山口 飛鳥(東京大学大気海洋研究所)、尾上 哲治(九州大学 大学院理学研究院 地球惑星科学部門)、小宮 剛(東京大学大学院総合文化研究科広域科学専攻)、座長:辻森 樹(東北大学)、山口 飛鳥(東京大学大気海洋研究所)

16:15 〜 16:30

[MIS17-10] Geochemical characteristics of felsic granitoids hosted by mantle peridotites at a continent-ocean transition zone in the Tyrrhenian Sea

*秋澤 紀克1、Poulaki Eirini 2、Cunningham Emily 3、Sanfilippo Alessio 4森下 知晃5、Pandey Ashutosh 6、Bickert Manon 7、Vannucchi Paola 8、Lei Chao 9、Gontharet Swanne 10小木曽 哲11田村 明弘5安邊 啓明12、Stefano Agata 13、Filina Irina14、Fu Qi 15、Kearns Lorna16、Kiran Koorapati Ravi 17、Loreto Filomena18、Magri Luca 19、Menapace Walter 20、Pavlovics Victoria3、Pezard Philippe21、Rodriguez-Pilco Milena22、Shuck Brandon 2、Zhao Xiangyu 23、Estes Emily24、Malinverno Alberto25、Zitellini Nevio 18 (1.広島大学 地球惑星システム学プログラム、2.Louisiana State Uni、3.Uni Utah、4.Uni Pavia、5.Kanazawa Uni、6.IISER TVM、7.Uni Brest、8.Uni Florence、9.China Uni、10.Sorbonne Uni、11.Kyoto Uni、12.JAEA、13.Uni Catania、14.Uni Nebraska、15.Uni Houston、16.Uni Leeds、17.Binghamton Uni、18.CNR-ISMAR、19.Uni Tasmania、20.ICM、21.Montpellier Uni、22.Texas A&M Uni at Galveston、23.Shanghai Jiao Tong Uni、24.Texas A&M Uni、25.Columbia Uni)

キーワード: IODP Exp.402、海洋コアコンプレックス、背弧海盆、地中海

The Continent-Ocean Transition (COT) zone is a fundamental place where we can understand the Earth’s unique process of continental lithosphere break-up and formation of new oceanic crust. The Tyrrhenian Sea is an ideal study area to investigate the COT process because deep-mantle materials with different COT magmatic records have been exhumed to the seafloor by detachment faults. IODP Exp 402 took place from 9 February to 8 April 2024 in the Tyrrhenian Sea and recovered mantle peridotites from two drill sites. The peridotites are intercalated with felsic granitoids with various deformation intensities. Calculated normative anorthite-albite-orthoclase compositions of the granitoids show that these samples are classified in the trondhjemite to granite series. The granitoids are abundant in Na2O content up to 7.6 wt% and are subaluminous in terms of Aluminous Saturation Index (ASI < 0.9). Because these granitoids are similar in chemical characteristics to those of igneous-type granitoids, we hypothesize that the granitoid magmas were generated during the COT in the Tyrrhenian Sea. Considering their zircon-apatite U-Pb geochronology data and microstructures (Poulaki et al., 2025; Abstract of EGU annual conference), the granitoid magmas intruded into the peridotites at Pliocene ages and the granitoids accommodated strain during exhumation along the detachment fault. The “unusual” granitoid magmas probably facilitated the formation of the oceanic core complex in this magma-poor continental margin.