日本地球惑星科学連合2016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-IT09] Hard-Rock Drilling: Oceanic Lithosphere to Continental Crust Formation

2016年5月23日(月) 09:00 〜 10:30 コンベンションホールA (2F)

コンビーナ:*田村 芳彦(海洋研究開発機構 海洋掘削科学研究開発センター)、森下 知晃(金沢大学理工研究域自然システム学系)、Straub Susanne(コロンビア大学ラモント地球科学研究所)、佐野 貴司(国立科学博物館地学研究部)、海野 進(金沢大学理工研究域自然システム学系)、高澤 栄一(新潟大学理学部地質科学科)、道林 克禎(静岡大学学術院理学領域)、座長:森下 知晃(金沢大学理工研究域自然システム学系)、道林 克禎(静岡大学学術院理学領域)

09:15 〜 09:30

[SIT09-02] Izu-Bonin-Mariana Arc basement from IODP Exp. 351(Amami Sankaku Basin)

★招待講演

*石塚 治1Hickey-Vargas Rosemary2Yogodzinki Gene3周藤 正史4McCarthy Anders5Savov Ivan6草野 有紀1Arculus Richard7Bogus Kara8 (1.産業技術総合研究所活断層火山研究部門、2.Florida International University、3.University of South Carolina、4.Universitaet Potsdam、5.University of Lausanne、6.University of Leeds、7.Australian National University、8.Texas A&M University)

キーワード:arc basement, Izu-Bonin-Mariana arc, geochemical characteristics, Ar/Ar age

IODP (International Ocean Discovery Program) Exp.351 targeted, in particular, evidence for the earliest evolution of the Izu-Bonin-Mariana (IBM) arc system following inception. This can be obtained by identification and exploration of regions adjacent to an arc, where unequivocally pre-arc crust (basement) overlain by undisturbed arc-derived materials exists. The drill site (U1438) is located in Amami Sankaku Basin (ASB), west of the Kyushu-Palau Ridge (KPR), i.e., paleo-IBM arc. Exp.351 successfully recovered pre-Izu-Bonin-Mariana arc basement, a volcanic and geologic record spanning pre-Arc, arc initiation to remnant arc stages. In this contribution, age and geochemical characteristics of arc basement and its tectonic significance will be discussed.
At U1438, 1611m thick section in total was cored, comprising 1461m of sediment section and 150m of igneous basement. Numerous flow contacts were identified in the basement, several chilled margins could be identified but low recovery in basement rock makes their interpretation in terms of volcanic stratigraphy difficult. Paleomagnetic measurements show consistent shallow plunges of maximum anisotropy axes, and that implies these basalts were emplaced as sheet flows rather than pillow lavas.
Basalts have diverse textures that include aphyric to subophitic/ophitic. Phenocrysts are present in approximately half of the basalts and consist of plagioclase, clinopyroxene, titanomagnetite, spinel and minor olivine.
Age interpretations based on biostratigraphy (Arculus et al., Nat Geosci, 2015) determined that the basement section is between 64 and 51 Ma, and direct age determination of basement basalt by Ar/Ar dating is under way.
Whole rock geochemical analysis of the basement basalt shows that these basalts are low K tholeiitic basalts. They mostly have high-MgO (generally >8 wt%), low-TiO2 (0.6–1.1 wt%), Ti/V, low-Zr (mostly <50 ppm). On Ti/V plot, the U1438 basalts and forearc basalt (FAB) which is supposed to be associated with subduction initiation from IBM arc are similar to each other and clearly distinct from Philippine Sea backarc basin basalts and normal MORB by having low Ti/V.
One prominent characteristic of the basalts is their depletion of immobile highly incompatible elements compared with MORB, e.g., they are strikingly light REE (LREE) depleted. But La/Nd ratio and Th/LREE increases upcore in the uppermost part of the basement, and these trace element variations with depth is accompanied by variation of major element composition such as Si and Ti.
Hf-Nd isotopes for the basement basalts show a significant range of compositions, and relatively radiogenic Hf compared to Nd indicates an Indian Ocean-type MORB source. However, the dominant signature, with eHf >16.5, is more radiogenic than most Indian MORB.
Preliminary data suggests that the basement basalts are relatively primitive melts and likely derived from Indian Ocean-type MORB sources that are more strongly depleted in terms of incompatible trace elements than typical MORB or backarc basin basalt in the Philippine Sea. Geochemical variation in the uppermost part of the core might imply variability of slab-derived enrichment and/or fertility of mantle at the onset of subduction.
Geochemical characteristics of arc basement from Exp.351 imply that depleted MORB-like basalt (“FAB”) appears to have formed in wider area than previously thought, i.e., including “reararc”side of ancient IBM arc. However, critical assessment of genetic relation between FAB and basement basalt of ASB requires precise age determination to constrain tectonic setting where the ASB basalts formed.