年轻火山海底的断裂带与构造应变

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Earth and Planetary Science Letters Pub Date : 2025-02-01 Epub Date: 2024-12-12 DOI:10.1016/j.epsl.2024.119174
Jie Chen , Javier Escartin , Mathilde Cannat
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引用次数: 0

摘要

洋中脊断崖在海底是可识别的,常用于估计板块分裂的构造成分。这种基于线性断层陡坡参数的估计在这里被称为视构造应变(ATS)。然而,ATS可能与岩石圈尺度上的实际构造应变不同。这一点在岩浆缺乏的慢速-超低扩展脊的拆离断层上表现得很明显,这些断层不对应于线状陡坡,但可容纳很高的应变。本文利用8个站点的高分辨率(1-2 m)测深数据,研究了MOR年轻火山海底的断层陡坡,扩展速率为14-110 km/Ma。我们的研究结果表明,ATS与扩散速率、熔体通量或热状态等因素之间的相关性较弱,这对ATS作为板块辐散的MOR构造成分的代表提出了挑战。相反,ATS具有时间依赖性和空间异质性,受岩脉侵入的频率和大小以及相关断层和火山喷发的控制,这些断层和火山喷发使海底重新出现并覆盖断层。我们的发现也对估计经历类似过程的陆基火山裂谷系统的构造伸展具有启示意义。
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Fault scarps and tectonic strain in young volcanic seafloor
Fault scarps at Mid-Ocean Ridges (MOR) are recognizable on the seafloor, and often measured to estimate the tectonic component of plate divergence. This estimate, based on linear fault scarp parameters, is referred to here as apparent tectonic strain (ATS). However, ATS may differ from the actual tectonic strain at a lithosphere scale. This is clear at detachment faults at magma-poor slow-ultraslow spreading ridges that do not correspond to linear scarps yet accommodate very high strain. Here we study fault scarps in young volcanic MOR seafloor, using high-resolution (1–2 m) bathymetry data of 8 sites with spreading rates of 14–110 km/Ma. Our results show a weak correlation between ATS and factors such as spreading rate, melt flux, or thermal regime, challenging the use of ATS as a proxy for the MOR tectonic component of plate divergence. Instead, ATS is time-dependent and heterogeneous spatially, controlled by the frequency and size of dike intrusions with associated faults and volcanic eruptions that resurface the seafloor and cover faults. Our findings also have implications for estimates of tectonic extension in subaerial volcanic rifting systems that undergo similar processes.
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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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