Ultramafic-influenced submarine venting on basaltic seafloor at the Polaris site, 87°N, Gakkel Ridge

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Earth and Planetary Science Letters Pub Date : 2025-02-01 DOI:10.1016/j.epsl.2024.119166
Elmar Albers , Alexander Diehl , Jessica N. Fitzsimmons , Laramie T. Jensen , Frieder Klein , Jill M. McDermott , Autun Purser , Jeffrey S. Seewald , Maren Walter , Gunter Wegener , Wolfgang Bach , Antje Boetius , Christopher R. German
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Abstract

The nature of deep-sea hydrothermal systems is commonly inferred from physicochemical plume characteristics and seafloor observations, as was the case for the ‘Polaris’ site on the ultraslow-spreading Gakkel Ridge, Earth's northernmost hydrothermal system. Initial reports showing temperature and turbidity anomalies in its hydrothermal plume combined with its location on a neovolcanic axial seamount suggested a volcanically-hosted ‘black smoker’-type system. That interpretation, however, is inconsistent with our more complete data set derived from extensive water column sampling and seafloor surveys. The buoyant plume exhibits minor turbidity anomalies and low metal concentrations (dissolved Mn ≤ 3.1 nM), but contains substantial concentrations of H2 (275 nM) and 13C-enriched CH4 (365 nM, δ13C = –13.2). Instead of a ‘black smoker’ vent field, we observed small-scale chimney structures at the seafloor. Together, these data imply intermediate-temperature reaction of hydrothermal fluids with ultramafic rock in the subseafloor before discharge through pillow basalt outcrops at the seafloor. Our study challenges the ability of established approaches to vent exploration, reliant exclusively on in situ sensing to reveal the full geodiversity of subseafloor hydrothermal venting. Ultramafic-influenced systems, releasing H2 and CH4 into the ocean, may be a recurring feature along the entire 25% of the global ridge system that is ultraslow-spreading.
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Gakkel Ridge北极星站点87°N玄武岩海底超镁铁影响的海底喷口
深海热液系统的性质通常是从物理化学羽流特征和海底观测中推断出来的,就像地球最北端的热液系统——超低扩散的Gakkel Ridge上的“北极星”地点一样。最初的报告显示,热液柱的温度和浊度异常,加上它位于一个新火山轴向海山上,表明它是一个火山宿主的“黑烟”型系统。然而,这种解释与我们从广泛的水柱采样和海底调查中获得的更完整的数据集不一致。浮力羽流表现出轻微的浊度异常和低金属浓度(溶解Mn≤3.1 nM),但含有大量H2 (275 nM)和富集13c的CH4 (365 nM, δ13C = -13.2)。我们观察到的不是“黑烟”通风口,而是海底的小型烟囱结构。综上所述,这些数据表明,热液流体在通过海底露头的枕状玄武岩排出之前,与海底超镁质岩石发生了中温反应。我们的研究挑战了现有的喷口勘探方法的能力,这些方法完全依赖于原位传感来揭示海底热液喷口的全部地质多样性。受超镁铁质影响的系统向海洋释放H2和CH4,这可能是整个25%的超低扩散脊系统的一个反复出现的特征。
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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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