Sabkha - salina白云岩保存了其沉积古环境的生物地球化学条件

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Geochimica et Cosmochimica Acta Pub Date : 2023-09-01 DOI:10.1016/j.gca.2023.06.031
Mónica Sánchez-Román , Luis Gibert , Juan Diego Martín-Martín , Kirsten van Zuilen , Victoriano Pineda-González , Pieter Vroon , Sylvie Bruggmann
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引用次数: 1

摘要

镁碳酸盐矿物的沉淀,从镁方解石到富钙白云石,通常与微生物活动有关,通常与其他蒸发矿物一起发生在盐水环境中。这些蒸发矿物的地球化学特征有助于解释沉积时的环境条件和生物地球化学过程。我们采用多代理方法,结合地层学、岩石学、矿物学和地球化学数据,如Fe和Sr同位素值,以中新世Vilobí石膏单元(pened盆地,西班牙东北部)为例,描述了白云岩在sabkha/盐碱地环境下沉积的环境和生物地球化学条件。Vilobí石膏单元岩相解释为sabkha - coastal salina交替沉积环境。Vilobí白云岩的δ13C和δ18O值(分别为- 6.3 ~ - 0.4‰和0.2 ~ 2.3‰)与现代sabkha和沿海环境的微生物影响白云岩比较好。白云岩87Sr/86Sr比值(0.70816 ~ 0.70874)变化显著,表明滨海sabkha/salina受海水的强烈影响。岩石学(微生物诱发的沉积构造被解释为蓝藻席和具有空细菌空洞的球形白云岩)和地球化学数据(元素浓度富集于Fe2+和Mn2+,分别高达1388和605 ppm)证明了微生物活动;δ56Fe值介于- 0.16 ~ 0.44‰之间)。综上所述,这些数据表明,所研究的白云岩是一种原生沉淀物,记录了受微生物活动影响的咸化沉积环境的地球化学特征。通过对比白云石和牡蛎壳(壳在0.70870 ~ 0.70872之间)的87Sr/86Sr值与全球Sr曲线,Vilobí石膏单元的年代为16.05 Ma和16.30 Ma (Burdigalian)。此外,白云岩记录的海相(孔隙水)值(C-O-Fe-Sr)可用于推断沉积环境和沉积时的地球化学条件。非传统同位素和痕量金属浓度的结果支持将形成于蒸发环境的白云岩作为古环境条件的档案。
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Sabkha and salina dolomite preserves the biogeochemical conditions of its depositional paleoenvironment

Precipitation of Mg-carbonate minerals, ranging from Mg-calcite to Ca-rich dolomite, is typically associated with microbial activity, and commonly takes place in saline environments along with other evaporitic minerals. The geochemistry of such evaporitic minerals can contribute to the interpretation of the environmental conditions and those (bio)geochemical processes occurring at the time of deposition. We use a multiproxy approach that combines stratigraphic, petrographic, mineralogical and geochemical data, such as Fe and Sr isotope values, to describe the environmental and biogeochemical conditions under which dolomite precipitated in a sabkha/salina environment using the Miocene Vilobí Gypsum Unit (Penedès Basin, NE Spain) as a case study.

The lithofacies of Vilobí Gypsum Unit are interpreted to indicate sedimentary environments alternating between sabkha and coastal salina. The δ13C and δ18O values of Vilobí dolomites (from −6.3 to −0.4‰ and from 0.2 to 2.3‰, respectively) compare well with microbially influenced dolomite from modern sabkha and coastal environments. The dolomite 87Sr/86Sr ratios (0.70816 to 0.70874) show significant variations and indicate that the coastal sabkha/salina was strongly influenced by seawater. Microbial activity is evidenced by petrography (microbially induced sedimentary structures interpreted as cyanobacterial mats, and spheroidal dolomite with empty bacterial voids), and geochemical data (elemental concentrations enrichment in Fe2+ and Mn2+, up to 1388 and 605 ppm, respectively; supported by δ56Fe values of between −0.16 and 0.44‰). Collectively, these data suggest that the studied dolomite is a primary precipitate that records the geochemistry of the saline depositional environment influenced by microbial activity. The Vilobí Gypsum Unit is here dated to 16.05 Ma and 16.30 Ma (Burdigalian) by correlating the 87Sr/86Sr values of dolomite and shell of the oysters (shells between 0.70870 and 0.70872) with the global Sr curve. Moreover, dolomite records marine (porewater) values (C-O-Fe-Sr) that can be used to infer the depositional environment and geochemical conditions at the time of deposition. Results of non-traditional isotopes and trace metal concentrations support using dolomite formed in evaporitic environments as an archive of paleoenvironmental conditions.

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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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