Untangling the effects of crustal and source processes on the Mo isotope systematics of oceanic arcs: insights from the Tonga-Kermadec subduction system

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
R. Pontow , R. Bezard , M. Willbold , S. Turner , T. Di Rocco
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引用次数: 0

Abstract

The Mo stable isotope system is a promising tracer of crustal recycling. As subduction zones play a major role in returning crustal material back to the Earth’s mantle, understanding the Mo isotope behavior during processes operating at these settings is paramount. The Mo isotope compositions of arc lavas are highly variable and despite recent advances in this field, questions remain about Mo isotope fractionation and mobilization during slab processes and the relative effect of magmatic differentiation on the Mo isotope compositions (δ98/95Mo) of arc lavas. The Tonga-Kermadec arc is well suited to assess and disentangle crustal and source processes in intra-oceanic arc settings owing to widespread felsic volcanism and along-arc source variations, characterized by increasing proportions of a metasedimentary component from the northern Tonga to the southern Kermadec arc. In the pursuit of these objectives, we analyzed a set of basaltic to dacitic tholeiitic arc lavas from volcanoes covering the whole length of the Tonga-Kermadec arc and sediments from DSDP site 204. Tonga-Kermadec arc lavas have highly variable Mo concentrations (0.21 and 2.35 µg/g) and δ98/95Mo values (−0.29 to +0.34 ‰). At some volcanoes, considerable δ98/95Mo variations in samples as primitive as basalt are correlated with indices of differentiation and Sr-Nd radiogenic isotopes, indicating an impact of crustal assimilation on Mo isotope compositions. However, the δ98/95Mo of the most primitive lavas analyzed for each volcano appear to have preserved primary melt signatures, since they form an along-arc trend mirroring those of Pb isotope averages, a proxy that is controlled by source processes in the Tonga-Kermadec arc. Using these data, a north–south decrease in δ98/95Mo of the sources of arc magmas is resolved. This is interpreted to reflect the competing signals of isotopically heavy slab-fluids (δ98/95Mo higher than D-MORB values) with that of an increasing contribution of a metasedimentary component that is lighter than the DMM toward the south. Our data suggest that crustal assimilation can significantly distort primitive δ98/95Mo even in mafic magmas from simple intra-oceanic arcs. The induced intra-volcano δ98/95Mo scatter has the potential to obscure along-arc variability as well as systematics with typical chemical and isotopic proxies used to characterize arc lava sources (e.g., Ba/Th, radiogenic isotopes). However, we also show that a careful evaluation of these effects can, at least in the Tonga-Kermadec arc, allow the assessment of arc lava source compositions.
解开地壳和烃源过程对大洋弧Mo同位素系统的影响:来自汤加-克马德克俯冲系统的见解
Mo稳定同位素系统是一种很有前途的地壳循环示踪剂。由于俯冲带在地壳物质返回地幔的过程中起着重要作用,因此了解在这些环境下运行过程中的Mo同位素行为至关重要。弧熔岩的Mo同位素组成变化很大,尽管近年来在这一领域取得了进展,但关于板块过程中Mo同位素分馏和活化以及岩浆分异对弧熔岩Mo同位素组成(δ98/95Mo)的相对影响仍存在疑问。由于广泛的长英质火山作用和沿弧源的变化,汤加-克马德克弧非常适合评估和解离洋内弧背景下的地壳和源过程,其特征是从汤加北部到克马德克弧南部的变质沉积岩成分比例增加。为了实现这些目标,我们分析了一组覆盖整个汤加-克马德克弧长度的火山的玄武岩-英安质拉玄岩弧熔岩和来自DSDP站点204的沉积物。汤加-克马德克弧熔岩的Mo浓度(0.21和2.35µg/g)和δ98/95Mo值(- 0.29 ~ +0.34‰)变化很大。在一些火山中,原始到玄武岩样品中δ98/95Mo的显著变化与分异指数和Sr-Nd放射性同位素相关,表明地壳同化对Mo同位素组成的影响。然而,每个火山分析的最原始熔岩的δ98/95Mo似乎保留了原始熔体特征,因为它们形成了一个沿弧趋势,反映了Pb同位素平均值,这是一个受汤加-克马德克弧源过程控制的代理。利用这些资料,解决了弧源δ98/95Mo的南北递减问题。这反映了同位素重的板岩流体(δ98/95Mo高于D-MORB值)与向南的轻于DMM的变质沉积岩组分贡献增大的竞争信号。我们的数据表明,即使在简单的洋内弧的基性岩浆中,地壳同化也会显著扭曲原始δ98/95Mo。火山内诱发的δ98/95Mo散射有可能模糊沿弧变化,以及用于表征弧熔岩来源的典型化学和同位素代用物(例如Ba/Th,放射性同位素)的系统性。然而,我们也表明,至少在汤加-克马德克弧中,对这些影响的仔细评估可以评估弧熔岩的来源成分。
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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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