OAE1a期浅水海相碳酸盐岩局部成岩蚀变的全球地球化学信号解析

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Matthew D. Nadeau , Jack G. Murphy , Cedric J. Hagen , Ziman Wu , Alliya A. Akhtar , Anne-Sofie Ahm , Daniel A. Stolper , Adam C. Maloof , John A. Higgins
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引用次数: 0

摘要

浅水海洋碳酸盐被广泛用于重建全球地球化学循环(如碳、钙、锶和锂)的短期(~百万年)扰动。然而,局部环境现象,如大气和海洋成岩蚀变或碳酸盐岩相变化,往往使碳酸盐岩地球化学与公海海水化学分离。因此,为了利用浅水碳酸盐精确地重建全球地球化学循环,将局部环境现象的信号与公海海水化学的真实变化分开是至关重要的。海洋钻探计划866A地点(Resolution Guyot,中太平洋山脉)记录的浅水碳酸盐演替为解开早白垩世海洋缺氧事件1a (OAE1a)期间浅水碳酸盐记录的全球和局部信号提供了机会,这是一个短暂的全球相关碳循环扰动。最近的研究记录了δ13C偏移,87Sr/86Sr的适度下降,δ7Li和δ44Ca值的大地层变化,这些都被解释为反映了与OAE1a相关的开放海洋海水化学成分的时间变化。然而,该地点的其他工作显示了大气和海洋成岩作用的明确证据,以及OAE1a层段碳酸盐相的变化。本文采用一系列碳酸盐岩地球化学指标(δ7Li、δ13C、δ18Ocarb、δ26Mg、δ44Ca、Δ47、[Mg]、[Ca]、[Sr]、[Li])和碳酸盐岩成岩作用数值模型,将反映全球地球化学循环的信号与反映局部环境现象的信号区分出来。研究表明,该区87Sr/86Sr比值的变化反映了原生海水组成的变化,而其他地球化学系统(如δ7Li、δ26Mg和δ44Ca值及微量元素浓度)的地层变化主要来自早期海相和大气成岩作用,其中Li受到了共生粘土的污染。可以想象,由于碳酸盐岩成岩作用的起源,许多化学地层变异得以保存至今,并且认识到这些元素在海水中的停留时间(100万年)比短暂的OAE1a事件更长,我们认为,我们的模型衍生的海洋成岩流体中钙、镁和锂同位素组成的“快照”估计反映了一个稳定的早白垩世开放海洋海水特征。尽管全球δ13C信号可能仍然存在,但我们的研究结果表明,该地点整个OAE1a的δ13C值的地层记录是海洋和大气成岩作用以及碳酸盐相变化的复杂函数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Disentangling global geochemical signals from local diagenetic alteration in shallow-water marine carbonates during OAE1a
Shallow-water marine carbonates are widely used to reconstruct short-lived (∼ million years) perturbations to global geochemical cycles (e.g., carbon, calcium, strontium, and lithium). However, local environmental phenomena like meteoric and marine diagenetic alteration or changes in carbonate facies often decouple carbonate geochemistry from open-ocean seawater chemistry. To accurately reconstruct global geochemical cycles using shallow-water carbonates, it is therefor crucial to separate signals of local environmental phenomena from genuine changes in open-ocean seawater chemistry. The well-documented shallow-water carbonate succession from Ocean Drilling Program Site 866A (Resolution Guyot, Mid-Pacific Mountains) offers an opportunity to disentangle global and local signals recorded in shallow-water carbonates during the Early Cretaceous oceanic anoxic event 1a (OAE1a), a brief, globally correlative perturbation to the carbon cycle. Recent studies at this site have documented a δ13C excursion, a modest decline in 87Sr/86Sr, and large stratigraphic variability in δ7Li and δ44Ca values, all of which have been interpreted as reflecting temporal changes in the chemical composition of open-ocean seawater associated with OAE1a. However, other work at this site demonstrates clear evidence of meteoric and marine diagenesis as well as changes in carbonate facies across the OAE1a interval. Here, we aim to disentagle signals that reflect global geochemical cycling from those that reflect local environmental phenomena by employing a suite of carbonate-bound geochemical proxies (δ7Li, δ13C, δ18Ocarb, δ26Mg, δ44Ca, Δ47, [Mg], [Ca], [Sr], [Li]) and a numerical model of carbonate diagenesis. We show that while changes in 87Sr/86Sr ratios at this site reflect changes in primary seawater composition, stratigraphic variability in other geochemical systems (e.g., δ7Li, δ26Mg and δ44Ca values and trace element concentrations) arises primarily from early marine and meteoric diagenesis, with some contamination of Li from co-occurring clays. With much of the chemostratigraphic variability preserved today conceivably owing its origin to carbonate diagenesis and in recognition of the residence times for these elements in seawater (>1 million years) being longer than the short-lived OAE1a event, we make a case that our model-derived “snapshot” estimate for the calcium, magnesium, and lithium isotope composition of the marine diagenetic fluid reflects a stable open-ocean Early Cretaceous seawater signature. Although a global δ13C signal may still be present, our findings show how the stratigraphic record of δ13C values across the OAE1a at this site is a complex function of marine and meteoric diagenesis and changes in carbonate facies.
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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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