Reassessing sedimentary sulfur isotope records: Local glacial-sedimentary processes, not global anoxia, drove the Hirnantian δ34Spy excursion

IF 11.3 1区 地球科学 Q1 GEOSCIENCES, MULTIDISCIPLINARY
Earth-Science Reviews Pub Date : 2026-08-01 Epub Date: 2026-05-19 DOI:10.1016/j.earscirev.2026.105548
Dongping Hu
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引用次数: 0

Abstract

The Hirnantian Stage (ca. 445.21–443.07 Ma) of the Late Ordovician records a pronounced positive excursion in pyrite sulfur isotopes (δ34Spy) concurrent with Gondwanan glaciation and the Late Ordovician Mass Extinction (LOME). This δ34Spy excursion is conventionally attributed to increased pyrite burial in anoxic seafloor, linking marine anoxia to the LOME. This hypothesis, however, lacks verification from global sedimentary sulfur content data and fundamentally conflicts with the stability of carbonate-associated sulfate sulfur isotopes (δ34SCAS: ∼ 25‰), which indicates minimal changes in global pyrite burial flux, thus hindering our understanding of the underlying mechanisms of the Hirnantian δ34Spy excursion and its paleoenvironmental implications. Here, I integrate geochemical data (δ34Spy, Δ33Spy, δ34SCAS, total sulfur (TS), total organic carbon (TOC), and Fe-speciation) from 13 globally distributed successions with well-constrained graptolite biozones to decipher controls on Hirnantian δ34Spy shift and their linkage to marine sulfur cycling. The results reveal a continuous decline in pyrite burial from the early to middle Hirnantian, coincident with Hirnantian glacial advance and the δ34Spy excursion, contradicting hypotheses of enhanced pyrite burial. Notably, the Hirnantian δ34Spy enrichment correlates with lithofacies changes (from organic-rich shales to carbonaceous mudstone/limestones), increased sedimentation rates, and oceanic oxygenation during glacial-eustatic sea-level fall, rather than with marine anoxia. I interpret the observed S-isotopic variations as reflecting a transition of microbial sulfate reduction in open-system (pre-Hirnantian) to closed-system, sulfate-limited conditions during the Hirnantian. I propose this marked shift was driven by glaciation-induced sea-level fall, which enhanced shallow marine oxygenation and increased sedimentation rates. Mechanistically, global shallowing of depositional settings and intensified ocean ventilation would deepen the microbial sulfate reduction zone within sediments. When coupled with higher sedimentation rates, these processes promoted a Rayleigh distillation behavior, enriching δ34Spy values. Numerical modeling of multiple S-isotopic covariations (δ34Spy-Δ33Spy) further corroborate the dominant influence of local processes on the S-isotopic trends observed before and across the Hirnantian. These findings demonstrate the Hirnantian positive δ34Spy excursion primarily reflects local sedimentological responses to glaciation, rather than globally enhanced pyrite burial and oceanic anoxia. This necessitates a reevaluation of the late Ordovician sulfur cycling and careful assessment of the global paleoenvironmental significance of sedimentary δ34Spy records over geological time.
沉积硫同位素记录的重新评估:局部冰川沉积过程,而不是全球缺氧,驱动了Hirnantian δ34Spy漂移
晚奥陶世希尔南天期(约445.21 ~ 443.07 Ma)黄铁矿硫同位素δ34Spy显著正偏移,与冈瓦南冰期和晚奥陶世大灭绝(LOME)同时发生。这种δ34Spy偏移通常归因于缺氧海底黄铁矿埋藏增加,将海洋缺氧与LOME联系起来。然而,这一假设缺乏全球沉积硫含量数据的验证,并且与碳酸盐相关硫酸盐硫同位素(δ34SCAS: ~ 25‰)的稳定性存在根本冲突,后者表明全球黄铁矿埋藏通量的变化很小,从而阻碍了我们对Hirnantian δ34Spy偏移的潜在机制及其古环境意义的理解。在此,作者整合了13个全球分布序列的地球化学数据(δ34Spy, Δ33Spy, δ34SCAS,总硫(TS),总有机碳(TOC)和铁物种),并结合了良好约束的笔石生物带,以破译Hirnantian δ34Spy位移的控制因素及其与海洋硫循环的联系。结果表明,从海南天早期到中期,黄铁矿埋藏持续下降,与海南天期冰川推进和δ34Spy漂移相一致,与黄铁矿埋藏增强的假设相矛盾。值得注意的是,Hirnantian δ34Spy富集与冰川-上升海平面下降期间的岩相变化(从富有机质页岩到碳质泥岩/灰岩)、沉积速率增加和海洋氧合作用有关,而与海洋缺氧无关。我将观测到的s同位素变化解释为反映了在Hirnantian时期开放体系(前Hirnantian)向封闭体系(硫酸盐限制条件)的微生物硫酸盐还原的转变。我认为这种明显的转变是由冰川引起的海平面下降所驱动的,海平面下降增强了浅海的氧合作用,增加了沉积速率。从机制上讲,沉积环境的全球变浅和海洋通风的加强将加深沉积物内的微生物硫酸盐还原带。当与较高的沉积速率相结合时,这些过程促进了瑞利蒸馏行为,使δ34Spy值富集。多重s同位素共变的数值模拟(δ34Spy-Δ33Spy)进一步证实了局部过程对希尔南梯之前和整个希尔南梯观测到的s同位素趋势的主要影响。这些发现表明,Hirnantian正δ34Spy偏移主要反映了对冰川作用的局部沉积学响应,而不是全球增强的黄铁矿埋藏和海洋缺氧。这就需要对晚奥陶世硫循环进行重新评价,并仔细评估沉积δ34Spy记录在地质时间上的全球古环境意义。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Earth-Science Reviews
Earth-Science Reviews 地学-地球科学综合
CiteScore
21.70
自引率
5.80%
发文量
294
审稿时长
15.1 weeks
期刊介绍: Covering a much wider field than the usual specialist journals, Earth Science Reviews publishes review articles dealing with all aspects of Earth Sciences, and is an important vehicle for allowing readers to see their particular interest related to the Earth Sciences as a whole.
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