日本地球惑星科学連合2025年大会

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[E] ポスター発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG51] ハードロック掘削科学:陸上・深海底掘削、そしてオフィオライト

2025年5月26日(月) 17:15 〜 19:15 ポスター会場 (幕張メッセ国際展示場 7・8ホール)

コンビーナ:星出 隆志(秋田大学国際資源学部)、針金 由美子(産業技術総合研究所)、岡崎 啓史(広島大学先進理工系科学研究科地球惑星システム学プログラム)

17:15 〜 19:15

[SCG51-P08] イタリア、カラブリア-シチリア島弧系の南ティレニア背弧海盆から掘削されたかんらん岩の岩石学的特徴

*寺田 桜弥子1秋澤 紀克2芳川 雅子2柴田 知之2森下 知晃3田村 明弘3、Alessio Sanfilippo4、Ashutosh Pandey5、Eirini Poulaki6、Emily Cunningham7、Manon Bickert8、Paola Vannucchi9、Chao Lei10、Swanne Gontharet11安邊 啓明12、Agata Stefano13、Irina Filina14、Qi Fu15、Lorna Kearns16、Ravi Koorapati17、Filomena Loreto18、Luca Magri19、Walter Menapace20、Victoria Pavlovics7、Philippe Pezard21、Milena Rodriguez-Pilco22、Brandon Shuck6、Xiangyu Zhao23、Emily Estes24、Alberto Malinverno25、Nevio Zitellini18 (1.広島大学理学部地球惑星システム学プログラム、2.広島大学大学院先進理工系科学研究科地球惑星システム学プログラム、3.金沢大学 理工研究域 地球社会基盤学系、4.Uni Pavia、5.IISER TVM、6.Louisiana State Uni、7.Uni Utah、8.Uni Brest、9.Uni Florence、10.China Uni、11.Sorbonne 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.ICP、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:国際深海科学掘削計画第402次研究航海、南ティレニア海、背弧海盆、かんらん岩、メルト-マントル相互反応

In island arc systems, plate subduction is a unique phenomenon of the earth that has a significant impact on magmatism, seismic activity, and material circulation. The subduction of the plate can cause the back-arc side to stretch, resulting in the expansion and formation of back-arc basins. Although magmatism from the volcanic front to the back-arc of island arc has been studied extensively, the formation and activity of back-arc basins remains largely unexplored due to the difficulty of collecting samples. However, research into back-arc basins is important for understanding the magmatism of island arc systems, including that on the back-arc side. Furthermore, mantle materials collected there is expected to provide information on primary magmatism.
The International Ocean Drilling Program Expedition 402 (IODP Exp. 402) was conducted in the Tyrrhenian Sea from February to April 2024, and core samples including peridotite were collected at the U1614 and U1616 boreholes. The southern Tyrrhenian back-arc basin is believed to have formed in relation to the subduction zone of the Calabria-Sicilia island arc system (Artemieva, 2023), and geophysical surveys from the region have inferred that mantle material is exposed on the seafloor (Prada et al., 2015). Although peridotite samples had been collected and studied during previous drilling ploject, the significant alteration suffered by the samples were a limiting fuctor in obtaing primary information. The objective of this study is to elucidate the petrological characteristics of 30 peridotite samples drilled at the U1616 borehole in the southern Tyrrhenian back-arc basin by mineral identification and petrographic analysis using a polarizing microscope, and major element composition measurement using an electron probe microanalyzer (EPMA).
Although the samples had undergone severe serpentinization, primary minerals were still observed. The upper part of the borehole section is mainly composed of harzburgitic peridotite, which consists of olivine, orthopyroxene, clinopyroxene, and brown to dark brown spinel. The lower part of the borehole section is also predominantly composed of harzburgitic peridotite, which contains olivine, orthopyroxene, clinopyroxene, black- opaque-fine-grained spinel, and plagioclase. The presence of dunite veins was observed in some samples obtained from the upper and lower parts of the borehole cross section in this study. The Fo contents (= atomic Mg/(Mg+Fe) ratio) of olivine and TiO2 content of clinopyroxene increase and decrease, respectively, from the lower to the upper part of the section. These observations suggest that the upper part section is depleted in melt components. The Cr# (atomic Cr/(Cr+Al) ratio) values of the spinels decrease the lower to the upper part of the section, suggesting that the upper part is enriched with melt components. In addition, the TiO2 contents of the spinels at the lower part of the section are very high (TiO2 wt% = ~1.9 wt%) and display a large variation. These results also suggest that the peridotites from the lower part are enriched with melt components compared to the peridotites of the upper part.
The mineralogical and petrological characteristics of the studied samples, when considered in conjunction with previous interpretations (Arai, 2005; Dick and Bullen, 1984; Ohara, 2003; Ohara, 2012), suggest that dunite veins with low spinel Cr# values were probably formed by the interaction between primary melts and wall rock peridotite. Additionally, the presence of plagioclase-bearing peridotite in the lower part of the section is likely the result of a reaction with basaltic melt that was saturated with plagioclase. The studied peridotite body exposed on the seafloor, is assumed to have been transported to the seafloor surface as an oceanic core complex (OCC) by the development of detachment faulting during the formation of the back-arc basin.