A Geochemical Mechanism for >10 m Apparent Downward Offsets of Magnetic Reversals Inferred From Comparison of Two Scotia Sea Drill Sites

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS Geochemistry Geophysics Geosystems Pub Date : 2024-07-18 DOI:10.1029/2023GC011325
Brendan T. Reilly, Lisa Tauxe, Stefanie A. Brachfeld, Bridget Kenlee, Marcus Gutjahr, Andrew W. Dale, Iván Hernández-Almeida, Sidney Hemming, Ian Bailey, Xufeng Zheng, Daven Cheu, Reece Taglienti, Michael E. Weber, Maureen E. Raymo, Trevor Williams
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Abstract

We document an apparent downward displacement of the Matuyama-Brunhes magnetic reversal by ∼20 m at Scotia Sea International Ocean Discovery Program Site U1538 (Pirie Basin) by comparison with the well-defined paleomagnetic record at nearby Site U1537 (Dove Basin). Detailed stratigraphic correlation between the two sites is possible due to similar lithologic variations. However, the two sites have distinctly different porewater geochemistry. Notably, Site U1538 indicates a greater demand for electron acceptors to oxidize organic carbon and Fe2+ enrichment below the depth of SO42− depletion. Magnetic parameters indicate enrichment of an authigenic magnetic mineral with strong remanence properties around the depth of SO42− depletion (∼46 m at Site U1538) relative to magnetic parameters at correlative depths at Site U1537. Fe2+ enrichment below the depth of SO42− depletion is not predicted based on the energetically favorable order of electron acceptors for microbial respiration but is documented here and in other depositional settings. This indicates Fe2+ production exceeds the production of H2S by SO42− reduction, providing a geochemical environment that favors the production and preservation of ferrimagnetic remanence-bearing iron sulfides over paramagnetic pyrite and, thus, a mechanism for deep chemical remanent magnetization acquisition at depths of tens of meters. The influence of authigenic ferrimagnetic iron sulfides on paleomagnetic signals can be difficult to demonstrate with magnetic properties alone; therefore, this finding has implications for evaluating the fidelity of magnetostratigraphic records with complementary geochemical data. Such situations should be considered in other depositional environments with similar porewater Fe2+ accumulation below the SO42− reduction depth.

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通过比较两个斯科舍海钻探地点,推断出磁反转超过 10 米明显向下偏移的地球化学机制
通过与附近的 U1537 号站点(鸽子盆地)清晰的古地磁记录进行比较,我们记录了斯科舍海国际大洋发现计划 U1538 号站点(皮里盆地)的 Matuyama-Brunhes 磁反转明显向下位移了 ∼ 20 米。由于岩性变化相似,这两个地点之间可能存在详细的地层关联。然而,这两个地点的孔隙水地球化学特征却截然不同。值得注意的是,U1538 岩石表明氧化有机碳对电子受体的需求更大,SO42- 贫化深度以下富含 Fe2+。磁性参数表明,与 U1537 岩石相关深度的磁性参数相比,SO42-贫化深度(U1538 岩石 ∼ 46 米)附近富集了一种具有强剩磁特性的自生磁性矿物。根据微生物呼吸电子受体的能量有利顺序,SO42-耗竭深度以下的Fe2+富集是无法预测的,但在这里和其他沉积环境中都有记录。这表明Fe2+的产生超过了SO42-还原产生的H2S,从而提供了一种地球化学环境,有利于含铁磁性剩磁的硫化铁的产生和保存,而不是顺磁性黄铁矿,因此也就提供了一种在几十米深处获得深层化学剩磁的机制。自生铁磁性硫化铁对古地磁信号的影响很难单独用磁性能来证明;因此,这一发现对利用补充地球化学数据评估磁地层记录的真实性具有重要意义。在 SO42- 还原深度以下有类似孔隙水 Fe2+ 聚集的其他沉积环境中,也应考虑这种情况。
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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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