高3He/4He羽流更热,更容易融化:来自海洋岛屿玄武岩的岩石学和地球化学证据

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Sunna Harðardóttir, Matthew G. Jackson
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引用次数: 0

摘要

高3He/4He(即在对流上地幔洋中脊玄武岩范围(8±2 RA)之上的3He/4He)是在地球早期形成、脱气较少的热点地区发现的罕见成分。最大3He/4He与高热点浮力通量、最大3He/4He与低地震横波速度异常之间的关系表明,高3He/4He只被最热、浮力最强的地幔柱所携带。该模型预测高3He/4He组分通过高熔点取样。利用新的海洋岛屿熔岩地球化学数据库,我们发现高3He/4He仅存在于拉斑岩(低碱指数)和轻度碱(中碱指数)熔岩中,它们分别是由高熔融和中等熔融造成的。低熔融度形成的高碱性(高碱指数)熔岩没有很高的3He/4He。这些观测结果支持一个模型,即最高的3He/4He羽流是最热的,因此融化到很高的程度,这导致了拉斑岩和轻度碱性熔岩的产生。然而,我们的观测表明,热柱的高度熔融是产生高3He/4He熔岩的必要条件,但不是充分条件。具有高比例的再循环物质和/或枯竭地幔物质(两者都具有低3He/4He)的地幔域的高熔融程度将产生低3He/4He熔岩。因此,只有具有相对纯的高3He/4He源物质的地幔域(即低3He/4He源物质很少或没有再循环物质或低3He/4He源物质枯竭)的热熔才能产生高3He/4He熔岩。高3He/4He羽流更容易熔化的结论得到了地球物理观测的支持。地球物理观测表明,高3He/4He羽流更热——它们在上地幔有更高的浮力通量和更低的剪切波速度异常——并且热羽流比冷羽流熔化得更多。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
High 3He/4He plumes are hotter and melt more: evidence from the petrology and geochemistry of ocean island basalts
High 3He/4He (i.e., 3He/4He above the convecting upper mantle mid-ocean ridge basalt range (8 ± 2 RA)) is a rare component identified in hotspots that sample an early-formed, less-degassed domain in the planet. Relationships between the maximum 3He/4He and high hotspot buoyancy flux, and between maximum 3He/4He and low seismic shear-wave velocity anomalies, suggest that high 3He/4He is entrained only by the hottest and most buoyant mantle plumes. A prediction of this model is that the high 3He/4He component is sampled by high-degree melting. We use a new geochemical database of ocean island lavas to demonstrate that high 3He/4He is found only in tholeiitic (low alkali index) and mildly alkalic (intermediate alkali index) lavas, which result from high and moderate degrees of melting, respectively. Highly alkalic (high alkali index) lavas that are generated by low degrees of melting are not observed to have very high 3He/4He. These observations support a model where the highest 3He/4He plumes are the hottest and therefore melt to high degrees, which results in generation of tholeiites and mildly alkalic lavas. However, our observations suggest that high degrees of melting of hot plumes is a necessary but insufficient condition for generation of high 3He/4He lavas. High degrees of melting of mantle domains with a high fraction of recycled material and/or depleted mantle material—both of which have low 3He/4He—will generate low 3He/4He lavas. Thus, only hot melting of mantle domains that have relatively pure high 3He/4He source material (i.e., little or no recycled material or depleted low 3He/4He mantle material) will result in generation of high 3He/4He lavas. The conclusion that high 3He/4He plumes melt more is supported by geophysical observations that suggest high 3He/4He plumes are hotter—they have higher buoyancy flux and lower shear-wave velocity anomalies in the upper mantle—and hotter plumes should melt more than cooler plumes.
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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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