显示碳酸盐-硅酸盐耦合成因的埃迪卡拉统豆山头地层(华南)26Mg含量极高的自生粘土

IF 4 1区 地球科学 Q1 GEOGRAPHY, PHYSICAL Global and Planetary Change Pub Date : 2024-06-25 DOI:10.1016/j.gloplacha.2024.104500
Tianzheng Huang , Bing Shen , Xiaoli Wang , Haoran Ma , Chao Li , Chuanming Zhou
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引用次数: 0

摘要

在马里诺全球冰川期(650-635Ma)之后,冰川期强烈的大陆风化作用倾向于大幅降低大气中的 pCO2 水平,从而有可能使地球回到冰川期的气候条件。然而,随之而来的全球变冷和冰川并没有发生。大陆风化作用造成的二氧化碳减少可能通过海洋中的反向风化作用释放出更多的二氧化碳来补偿,这一点可以从自生粘土矿物的大量沉淀中得到证明,例如华南斗山坨地层(635-551 Ma)下部富含镁的皂石和clinochlore。富镁自生粘土的大量沉淀意味着埃迪卡拉早期海洋中存在一个独特的海洋镁循环,但其起源一直存在争议。在此,我们测量了豆山沱地层自生粘土的镁同位素组成。皂石和绿泥石的26Mg富集程度极高,皂石的镁同位素(δ26Mgsap)高达+0.39‰,绿泥石的镁同位素(δ26Mgsap)高达+1.26‰。考虑到皂石沉淀中的镁同位素分馏范围在-0.95‰到-1.45‰之间,高δ26Mgsap值需要极高的海水镁同位素组成(δ26Mgsw),而这无法通过海水镁供应的直接沉淀来解决。相反,这需要其他成岩过程来提高孔隙水的镁同位素组成(δ26Mgpw)。应用数值模型对成岩过程中的镁同位素分馏进行了量化。建模结果表明,相对于皂石沉淀而言,白云石化较早可能会使孔隙水镁同位素升高,随后沉淀出富含26Mg的皂石。碳酸盐-硅酸盐耦合成岩作用是维持海水镁浓度和δ26Mg稳定的关键机制,凸显了自生粘土矿物作为镁和碳循环的缓冲器,抵消了马里诺冰川作用后的大量风化输入。
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Extremely 26Mg-enriched authigenic clays from the Ediacaran Doushantuo Formation (South China) indicating the coupled carbonate-silicate diagenesis

In the aftermath of Marinoan global glaciation (∼650–635 Ma), the deglacial intense continental weathering tended to dramatically lower the atmospheric pCO2 level, potentially driving the Earth back to the glacial climatic condition. However, the resultant global cooling and glaciation did not occur. The CO2 drawdown by continental weathering might have been compensated by additional CO2 release via reverse weathering in the ocean, as evidenced by abundant precipitations of authigenic clay minerals, for example, Mg-rich saponite and clinochlore in the lower part of Doushantuo Formation (635–551 Ma) in South China. Massive precipitations of Mg-rich authigenic clays imply a distinct marine Mg cycle in the early Ediacaran ocean, but their origins have been debated. Here, we measured the Mg isotopic compositions of authigenic clays from the Doushantuo Formation. Both saponite and clinochlore are extremely 26Mg-enriched, with Mg isotopes of saponite (δ26Mgsap) up to +0.39‰ and clinochlore up to +1.26‰. Considering the Mg isotopic fractionation in saponite precipitation ranging from −0.95‰ to −1.45‰, high δ26Mgsap values requires extremely high seawater Mg isotopic composition (δ26Mgsw), which cannot be resolved by direct precipitation with seawater Mg supply. Instead, it requires other diagenetic processes that elevated the porewater Mg isotopic composition (δ26Mgpw). A numerical model was applied to quantify the Mg isotopic fractionation in diagenesis. The modeling result indicates an earlier dolomitization relative to saponite precipitation might have elevated the porewater Mg isotopes, followed by the precipitation of extremely 26Mg-enriched saponite. The coupled carbonate-silicate diagenesis is a key mechanism sustaining stable seawater Mg concentration and δ26Mg, highlighting authigenic clay mineral as a buffer for Mg and C cycles counterbalancing massive weathering input after Marinoan glaciation.

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来源期刊
Global and Planetary Change
Global and Planetary Change 地学天文-地球科学综合
CiteScore
7.40
自引率
10.30%
发文量
226
审稿时长
63 days
期刊介绍: The objective of the journal Global and Planetary Change is to provide a multi-disciplinary overview of the processes taking place in the Earth System and involved in planetary change over time. The journal focuses on records of the past and current state of the earth system, and future scenarios , and their link to global environmental change. Regional or process-oriented studies are welcome if they discuss global implications. Topics include, but are not limited to, changes in the dynamics and composition of the atmosphere, oceans and cryosphere, as well as climate change, sea level variation, observations/modelling of Earth processes from deep to (near-)surface and their coupling, global ecology, biogeography and the resilience/thresholds in ecosystems. Key criteria for the consideration of manuscripts are (a) the relevance for the global scientific community and/or (b) the wider implications for global scale problems, preferably combined with (c) having a significance beyond a single discipline. A clear focus on key processes associated with planetary scale change is strongly encouraged. Manuscripts can be submitted as either research contributions or as a review article. Every effort should be made towards the presentation of research outcomes in an understandable way for a broad readership.
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