Tectonic and magmatic evolution of the southernmost Mariana convergent margin: Constraints from geochronology and geochemistry of the Challenger Deep sediments

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Lithos Pub Date : 2024-09-07 DOI:10.1016/j.lithos.2024.107796
Ming Yang , Tao Wu , Wen Zhang , Liyan Tian , Jianggu Lu , Taoran Song , Hengrui Zhu , Yidi Hong , Jiawang Chen
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Abstract

The southernmost Mariana convergent margin (SMCM) is a distinct segment of the Izu-Bonin-Mariana (IBM) subduction system with unique east-west orientation, however, its nature and tectonic history remains enigmatic. Here, for the first time, we present the detailed geochemical data of detrital minerals and UPb ages of accessory minerals from two sediment samples recovered at the deepest part of Southern Marianna Trench including the Challenger Deep. Detrital magmatic zircon UPb ages can be divided into three groups. Group 1 zircons show a weighted mean age of 50.3 ± 1.2 Ma, contemporary to the published boninites from northern IBM. The εHf(t) of these zircons (11.1–16.4) are also similar to the boninites (12.6–16.8) and volcanic arc rocks (4.2–14.2), but lower than forearc basalts (17.8–22.1), suggesting that these zircons are from boninitic or arc magmatism. The apatite UPb dating obtained a similar age of 55.0 ± 5.5 Ma. Therefore, if they are all from boninites, then subduction initiation magmatism ended at SMCM was likely coeval with northern IBM. Group 2 and Group 3 zircons have εHf(t) values similar to Group 1 zircons, but recorded younger 206Pb/238U ages of 16.8 ± 1.8 Ma and 11.0 ± 0.2 Ma, respectively, which are most likely related to the arc volcanism at West Mariana Ridge (WMR). Additionally, a rutile age of 19.0 ± 0.6 Ma is identified, which is also likely related to WMR. The chemical composition and calculated P-T conditions of clinopyroxenes indicate that they are mainly from the Mariana forearc basalts and arc volcanic rocks. In situ Sr isotopic compositions of plagioclases also show strong affinity to the Mariana forearc basalts and arc volcanic rocks. Therefore, our study indicates that sediments at the deep trench can record the long-term tectonic and magmatic evolution of the convergent margin.

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马里亚纳汇聚边最南端的构造和岩浆演化:挑战者深渊沉积物的地质年代和地球化学制约因素
最南端的马里亚纳汇聚边(SMCM)是伊豆-波宁-马里亚纳(IBM)俯冲系统的一个独特区段,具有独特的东西走向,但其性质和构造历史仍是一个谜。在此,我们首次展示了在南马里安纳海沟(包括挑战者深渊)最深处采集的两个沉积物样本中分离矿物的详细地球化学数据和附属矿物的 UPb 年龄。岩屑锆石的 UPb 年龄可分为三组。第 1 组锆石的加权平均年龄为 50.3 ± 1.2 Ma,与已发表的 IBM 北部倭黑岩的年龄相当。这些锆石的εHf(t)(11.1-16.4)也与倭黑岩(12.6-16.8)和火山弧岩(4.2-14.2)相似,但低于前弧玄武岩(17.8-22.1),表明这些锆石来自倭黑岩或火山弧岩浆活动。磷灰石 UPb 测定得到了类似的 55.0 ± 5.5 Ma 的年龄。因此,如果这些锆石都来自倭黑岩,那么在SMCM结束的俯冲起始岩浆活动很可能与北部IBM同时发生。第2组和第3组锆石的εHf(t)值与第1组锆石相似,但记录到的206Pb/238U年龄分别为16.8 ± 1.8 Ma和11.0 ± 0.2 Ma,这很可能与西马里亚纳海脊(WMR)的弧形火山活动有关。此外,金红石的年代为 19.0 ± 0.6 Ma,也很可能与西马里亚纳海脊有关。霞石的化学成分和计算的 P-T 条件表明,它们主要来自马里亚纳前弧玄武岩和弧形火山岩。斜长石的原位锶同位素组成也表明它们与马里亚纳前弧玄武岩和弧火山岩有很强的亲缘关系。因此,我们的研究表明,深海沟的沉积物可以记录汇聚边缘的长期构造和岩浆演化。
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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