Uranium and molybdenum isotope evidence for globally extensive marine euxinia on continental margins and in epicontinental seas during the Devonian-Carboniferous Hangenberg Crisis

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Shuai Yang , Xinze Lu , Xinming Chen , Wang Zheng , Jeremy D. Owens , Seth A. Young , Brian Kendall
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引用次数: 0

Abstract

The end-Devonian Hangenberg Crisis was one of the biggest Phanerozoic mass extinctions. However, the mechanism(s) that triggered this event is still debated. In this study, multiple geochemical paleoredox proxies (redox-sensitive trace metals [e.g., Mo, U, Re, V] and isotope systems [Mo, U, S, C]) were applied to the Exshaw Formation black shales to infer ocean redox conditions during the Hangenberg Crisis. The measured δ13Corg values generally decrease upsection in the Exshaw Formation. The Exshaw black shales have increasing maturity levels from east to west in the Western Canada Sedimentary Basin. Large sulfur isotope fractionations (–15‰ to 65‰) between original seawater sulfate and pyrite is best explained by microbial sulfate reduction during deposition and early diagenesis rather than thermochemical sulfate reduction. Precise Re-Os ages previously reported for the Exshaw Formation suggest that metal geochemical signatures in these shales, including overmature shales, were minimally affected by hydrocarbon maturation and reflected depositional conditions. Both Sr/Ba and TS/TOC ratios (the latter only from immature shales affected minimally by hydrocarbon generation) suggest predominantly brackish and marine settings with significant water exchange between the basin and open ocean. The TOC contents, redox-sensitive trace metal concentrations (Mo, U, Re), and Fe speciation indicate local bottom waters ranged from suboxic (with sulfidic pore waters) to euxinic. The authigenic δ98Mo and δ238U values for the Exshaw shales range from 0.3‰ to 1.1‰, and from –0.23‰ to 0.39‰, respectively. The δ98Mo of the Exshaw Formation may have been offset to lower values than coeval seawater because of a local particulate Fe-Mn shuttle and/or local weakly euxinic bottom waters. Two different correlation patterns (positive correlation and no correlation) of δ238U and U enrichment factors (EF) were observed for Exshaw black shales deposited from locally euxinic bottom waters. The positive correlation group samples (−0.13‰ to 0.23‰) suggest U isotope fractionations (0.4‰ to 0.8‰) between sediments and seawater like those observed in modern euxinic basins. Higher δ238U values (>0.2‰) in the no correlation group suggest even larger U isotope offsets (0.8–1.2‰) from seawater, possibly associated with removal of U into organic floccule layers during deposition. Applying the above Mo and U isotope fractionations to the Exshaw shales, global seawater δ98Mo and δ238U at the Devonian-Carboniferous boundary (DCB) may have been in the range of 1.4‰ to 1.9‰ and −0.9‰ to −0.5‰, respectively. A Mo and U isotope mass balance model suggests a large areal extent of euxinic seafloor (6–10%) at the DCB, which could be pervasive along continental margins and in epicontinental seas during transgression. Therefore, our data support expanded ocean euxinia at the DCB as an important contributor to the Hangenberg Crisis.

泥盆纪-石炭纪汉根堡危机期间全球广泛分布的大陆边缘和陆表海海洋含氧生物的铀和钼同位素证据
泥盆纪末的汉根堡危机是显生宙最大的物种大灭绝之一。然而,引发这一事件的机制仍存在争议。本文采用多种地球化学古氧化还原指标(氧化还原敏感微量金属[如Mo, U, Re, V]和同位素系统[Mo, U, S, C])对Exshaw组黑色页岩进行分析,推测Hangenberg危机时期海洋氧化还原条件。测量的δ13Corg值一般在Exshaw组向上递减。加拿大西部沉积盆地Exshaw黑色页岩成熟度自东向西递增。原始海水硫酸盐与黄铁矿之间存在较大的硫同位素分异(-15‰~ 65‰),最好的解释是沉积和早期成岩过程中微生物硫酸盐还原作用,而不是热化学硫酸盐还原作用。先前报道的Exshaw组精确Re-Os年龄表明,这些页岩(包括过成熟页岩)的金属地球化学特征受油气成熟程度的影响最小,反映了沉积条件。Sr/Ba和TS/TOC比值(后者仅来自受生烃影响最小的未成熟页岩)表明,盆地和大洋之间的水交换明显,主要是咸淡水和海洋环境。TOC含量、氧化还原敏感的微量金属(Mo、U、Re)浓度和铁的形态表明,当地底水从亚氧(含硫化物孔隙水)到富氧。Exshaw页岩自生δ98Mo值为0.3‰~ 1.1‰,δ238U值为-0.23‰~ 0.39‰。Exshaw组的δ98Mo可能由于局部颗粒Fe-Mn的流动和/或局部弱缺氧的底水而被抵消到低于同期海水的值。Exshaw黑色页岩δ238U与铀富集因子EF有两种不同的相关模式(正相关和不相关)。正相关组样品(- 0.13‰~ 0.23‰)表明沉积物与海水之间的U同位素分馏(0.4‰~ 0.8‰)与现代富氧盆地相似。不相关组δ238U值较高(>0.2‰),表明来自海水的U同位素偏移更大(0.8-1.2‰),可能与沉积过程中U被有机絮凝层去除有关。将上述Mo和U同位素分馏应用于Exshaw页岩,泥盆纪-石炭系界线(DCB)全球海水δ98Mo和δ238U可能分别在1.4‰~ 1.9‰和- 0.9‰~ - 0.5‰之间。Mo和U同位素质量平衡模型表明,DCB地区存在大面积的含氧海底(6-10%),在海侵期间沿大陆边缘和陆表海可能普遍存在。因此,我们的数据支持DCB扩大海洋环境是造成Hangenberg危机的重要因素。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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