Heavy magnesium isotopic compositions of basalts erupted during arc inception: Implications for the mantle source underlying the nascent Izu-Bonin-Mariana arc

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Shuai Yuan , He Li , Richard J. Arculus , Yongsheng He , Shan Ke , Weidong Sun
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引用次数: 0

Abstract

Basalts formed during the early development of an arc are usually buried, but they record critical information relating to the mantle source of the overriding plate prior to the addition of subducting slab components. Basalts recovered at Site U1438 of International Ocean Discovery Program (IODP) Expedition 351, in the Amami Sankaku Basin (ASB), formed during the transition from forearc basalt (FAB) and boninite eruptions to stratovolcano developments in the Izu-Bonin-Mariana (IBM) arc. In this study, we present magnesium (Mg) isotopic data (δ26Mg) for the ASB basalt core samples, formed at arc inception in the absence of down-going slab components, and report the implications of these data for the characteristics of the mantle sources underlying the proto-IBM arc. The δ26Mg values of the ASB basalts range from −0.21‰ to +0.08‰, with an average value of −0.13 ± 0.07‰. These values are systematically higher than those of mid-ocean ridge basalts (MORBs) (−0.25 ± 0.06‰). No obvious effects of post-eruptive alteration, fractional crystallization, partial melting, or subduction component addition can be identified in the Mg isotopic compositions either of the ASB basalts or their mantle source, given the absence of correlations between the δ26Mg values and the proxies of these processes (e.g., K/Nb, Nb/Zr, Ba/La, Nb/Y, etc.). We conclude that the high δ26Mg values of the ASB basalts are inherited from their mantle source that was enriched in heavy Mg isotopes. Melting of an ultra-depleted, refractory spinel peridotite source containing talc-bearing serpentinite components can explain the origin of the heavy Mg isotopic compositions in the ASB basalts. The presence of water-rich serpentinite components in the mantle provides a new perspective on how a refractory mantle source can undergo partial melting at temperatures and pressures similar to the formation of MORBs without the influence of subducted materials, which has important implications for the initiation of plate subduction. Furthermore, the Mg isotopic contributions of subducted additions and mantle source materials should be carefully discussed in future studies due to the heterogeneity of Mg isotopes in the mantle.

弧开始时爆发玄武岩的重镁同位素组成:对新生伊豆-波宁-马里亚纳弧下地幔源的启示
在弧发育早期形成的玄武岩通常是埋藏的,但它们记录了在俯冲板块成分加入之前,与上覆板块的地幔源有关的重要信息。国际海洋发现计划(IODP) 351远征队在Amami Sankaku盆地(ASB) U1438遗址发现的玄武岩形成于伊扎-博宁-马里亚纳弧(IBM)弧前玄武岩(FAB)和博宁-马里亚纳弧(ibu - bonin - mariana弧)的层状火山发育过渡时期。在这项研究中,我们提供了ASB玄武岩岩心样品的镁(Mg)同位素数据(δ26Mg),这些样品形成于弧开始时,没有下降的板块成分,并报告了这些数据对原始ibm弧下地幔源特征的影响。ASB玄武岩的δ26Mg值范围为- 0.21‰~ +0.08‰,平均值为- 0.13±0.07‰。这些数值有系统地高于中洋脊玄武岩(MORBs)(- 0.25±0.06‰)。由于δ26Mg值与K/Nb、Nb/Zr、Ba/La、Nb/Y等指标之间没有相关性,因此ASB玄武岩及其地幔源的Mg同位素组成均未发现明显的喷发后蚀变、分离结晶、部分熔融或俯冲成分添加的影响。本文认为,ASB玄武岩的高δ26Mg值继承自富集重Mg同位素的地幔源。含有含滑石蛇纹石成分的超贫难熔尖晶石橄榄岩源区熔炼可以解释ASB玄武岩中重Mg同位素组成的来源。地幔中富水蛇纹岩组分的存在为研究难熔地幔源如何在类似morb形成的温度和压力下发生部分熔融而不受俯冲物质的影响提供了新的视角,这对板块俯冲的启动具有重要意义。此外,由于地幔中Mg同位素的非均质性,在未来的研究中应仔细讨论俯冲补充物和地幔源物质的Mg同位素贡献。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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