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The First 10 Million Years of Rear‐Arc Magmas Following Backarc Basin Formation Behind the Izu Arc
Geochemistry, Geophysics, Geosystems ( IF 2.9 ) Pub Date : 2020-09-16 , DOI: 10.1029/2020gc009114
T. Miyazaki 1 , J. B. Gill 2 , C. Hamelin 3 , S. M. DeBari 4 , T. Sato 1 , Y. Tamura 1 , J. ‐I. Kimura 1 , B. S. Vaglarov 1 , Q. Chang 1 , R. Senda 5 , S. Haraguchi 6
Affiliation  

IODP Site U1437 is located in the Izu rear‐arc region, approximately 330 km west of the Izu‐Bonin trench axis. The oldest four units (Units IV through Unit VII) include volcaniclastic sediment and in situ hyaloclastites. They have ages of about 6–15 Ma, shortly after cessation of Shikoku backarc basin opening. Three magma types are identified by their distinct geochemistry; they are similar types to those found in the modern Izu arc (Rear Arc Seamount Chain [RASC]‐type, Rift‐type, and volcanic front [VF]‐type). RASC‐type has the most enriched Nd and Hf isotope and fluid‐immobile trace element ratios and dominates from 9 to 6 Ma. Rift‐type, dominant from 15 to 9 Ma, is similar to VF‐type in Nd‐Hf isotopes but has the least radiogenic Sr and Pb, and intermediate La/Yb and Nb/Yb, indicating a more fertile mantle source and less hydrous slab component than VF‐type. Less common and randomly distributed VF‐type sediments have the most radiogenic Sr and Pb, and the highest Ba/(Th, LREE [light rare earth element]) ratios, and are interpreted to be distally derived. The genesis of mafic Unit VII samples (~15 Ma) was modeled using the Arc Basalt Simulator. Results are most similar to those for basalts in the modern rift environment indicating the addition of ~1% of a melt‐rich slab component generated at ~125 km, to a Philippine Sea Plate ambient mantle that was more depleted than DMM (depleted MORB mantle). The initial post‐Shikoku basin magmatism in the Izu rear‐arc generated Rift‐type magmas for about 6 million years before the distinctive RASC‐type magmatism began, which then became increasingly enriched.

中文翻译:

伊豆弧后的后弧盆地形成之后的前弧岩浆的前一千万年

IODP站点U1437位于伊豆后电弧区,在伊豆-波宁沟槽轴线以西约330公里处。最古老的四个单元(第IV单元至第VII单元)包括火山碎屑沉积物和原位透明质碎屑岩。在四国后弧盆地开放停止后不久,它们的年龄约为6-15 Ma。三种岩浆类型通过其独特的地球化学来识别。它们与现代Izu弧中的类型相似(后弧海山链[RASC]型,裂谷型和火山锋[VF]型)。RASC型具有最丰富的Nd和Hf同位素以及流体不流动的痕量元素比,且主要为9-6 Ma。在Nd-Hf同位素中占优势的裂谷型从15Ma到9Ma,类似于VF型,但放射源的Sr和Pb最少,中间有La / Yb和Nb / Yb,表示与VF型相比,地幔来源更肥沃,含水层成分更少。不太常见且随机分布的VF型沉积物具有最强的放射源性Sr和Pb,并且具有最高的Ba /(Th,LREE [轻稀土元素])比,并且被解释为是远距离衍生的。使用弧形玄武岩模拟器模拟了镁铁质VII单元样品(约15 Ma)的成因。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的平板成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。不太常见且随机分布的VF型沉积物具有最强的放射源性Sr和Pb,并且具有最高的Ba /(Th,LREE [轻稀土元素])比,并且被解释为是远距离衍生的。使用弧形玄武岩模拟器模拟了镁铁质VII单元样品(约15 Ma)的成因。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的平板成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。不太常见且随机分布的VF型沉积物具有最强的放射源性Sr和Pb,并且具有最高的Ba /(Th,LREE [轻稀土元素])比,并且被解释为是远距离衍生的。使用弧形玄武岩模拟器模拟了镁铁质VII单元样品(约15 Ma)的成因。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的板状成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。LREE [轻稀土元素])比率,并被解释为向远侧推导。使用弧形玄武岩模拟器模拟了镁铁质VII单元样品(约15 Ma)的成因。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的板状成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。LREE [轻稀土元素])比率,并被解释为向远侧推导。使用弧形玄武岩模拟器模拟了镁铁质VII单元样品(约15 Ma)的成因。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的平板成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的平板成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。结果与现代裂谷环境中的玄武岩最相似,表明在〜125 km处向菲律宾海床周围地幔中添加了〜1%的富含熔体的平板成分,该地幔比DMM(贫化的MORB地幔)耗尽)。在独特的RASC型岩浆作用开始之前,伊豆后弧中最初的四国后盆地岩浆作用产生了约600万年的裂谷型岩浆。
更新日期:2020-10-23
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