中太古代微生物Cd、Ba和Ni循环:Pongola组叠层石光合作用的新稳定同位素和高分辨率微量元素图证据。

IF 3.5 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Astrobiology Pub Date : 2024-12-01 Epub Date: 2024-11-29 DOI:10.1089/ast.2024.0041
Simon V Hohl, Yiwen Lv, Yi-Bo Lin, Yinggang Zhang, Yuxiang Jiang, Guang-Yi Wei, Sebastian Viehmann
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引用次数: 0

摘要

生物活性金属的非传统稳定同位素作为重建金属生物地球化学循环的新代用物,在主要代谢途径中起辅助作用。环境流体和微生物之间的金属同位素分馏最终记录在自生矿物中,如碳酸盐,这使得它们可能比有机物质中的标准生物标志物更可靠。叠层石碳酸盐岩是研究生物圈、大气和水圈长期相互作用的地球化学档案,具有研究早期生命环境和金属组演化的独特潜力。本研究利用来自29.5亿年前的Pongola超群(非洲南部)的叠层石作为现场实验室,结合原位痕量金属制图和特定层的新型稳定金属同位素组成,推断早期地球微生物金属循环通过光养和化学岩石自养代谢。定量原位微量元素图揭示了叠层石纹层中镍(Ni)、镉(Cd)、磷(P)、铁(Fe)和锰(Mn)的内在生物沉积富集。相比之下,钡(Ba)的分布更为均匀。原始叠层石纹层中自生碳酸盐的δ138Ba和δ112Cd分馏在碎屑背景和总体硅酸盐土值上表现出明显的分馏特征,但与微量金属浓度呈相反的相关性。自生δ60Ni值与中太古宙辉长岩组成重叠。自生叠层石碳酸盐中的镍同位素组成,可能是甲烷金属吸收的新代表,在本研究的样品中没有显示出这种代谢存在的任何证据。自生碳酸盐中Cd同位素组成遵循典型的瑞利同位素分馏;也就是说,Cd的同位素组成演变为接近现代地表组成的重值。δ112Cd与微量元素铜(Cu)、钼(Mo)和磷的正分馏碳(C)同位素(δ13C ~ +2‰)的相关性表明,Pongola微生物栖息地存在活跃的光合作用。我们表明,Ba同位素可以用来推断碳酸盐沉淀率类似于现代微生物碳酸盐。因此,Cd和Ni同位素组合具有独特的潜力,可以作为早期地球生物化学沉积记录的新型同位素生物标志物,而传统的脂质生物标志物由于有机质保存不完整而无法应用。关键词:早期生命-叠层石-新型稳定同位素-镉同位素-镍同位素-钡同位素-微量元素作图
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Mesoarchean Microbial Cd, Ba, and Ni Cycling: Evidence for Photosynthesis in Pongola Group Stromatolites through Novel Stable Isotopes and High-Resolution Trace Element Maps.

Nontraditional stable isotopes of bioactive metals emerged as novel proxies for reconstructing the biogeochemical cycling of metals, which serve as cofactors in major metabolic pathways. The fractionation of metal isotopes between ambient fluid and microorganisms is ultimately recorded in authigenic minerals, such as carbonates, which makes them potentially more reliable than standard biomarkers in organic matter. Stromatolitic carbonates are geochemical archives that allow for the study of the long-term interplay of the biosphere, atmosphere, and hydrosphere through deep time, with the unique potential to investigate early life environments and the evolution of the metallome. The present study uses stromatolites from the ∼2.95-billion-year-old Pongola Supergroup (S. Africa) as a field laboratory for combined in situ trace metal mapping and layer-specific, novel stable metal isotope compositions to infer early Earth microbial metal cycling via phototrophic and chemo-litho-autotrophic metabolisms. Quantitative in situ trace element maps reveal intrinsic biosedimentary enrichments of nickel (Ni), cadmium (Cd), phosphorus (P), iron (Fe), and manganese (Mn) in stromatolitic laminae. In contrast, barium (Ba) shows a more homogeneous distribution. Authigenic carbonates from pristine stromatolite laminae show distinct δ138Ba and δ112Cd fractionation above detrital background and bulk silicate Earth values, but opposing correlation with trace metal concentrations. Authigenic δ60Ni values overlap with Mesoarchean diamictite compositions. Nickel isotopic compositions in authigenic stromatolitic carbonates, potentially a new proxy for methanogenic metal uptake, do not show any proof of the presence of this metabolism in the samples of this study. Meanwhile, Cd isotopic compositions in authigenic carbonates follow typical Rayleigh-type isotope fractionation; that is, the isotopic composition of Cd evolves to heavy values close to modern surface compositions. Correlations of δ112Cd with the micronutrients copper (Cu), molybdenum (Mo), and P, at positively fractionated carbon (C) isotopes (δ13C ∼+2‰), argue for active photosynthesis in the Pongola microbial habitat. We show that Ba isotopes can be used to infer carbonate precipitation rates similar to modern microbial carbonates. Thus, the combination of Cd and Ni isotopes has the unique potential as novel isotope biomarkers for the biochemical sedimentary record of early Earth where traditional lipid biomarkers are not applicable due to the incomplete preservation of organic matter.

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来源期刊
Astrobiology
Astrobiology 生物-地球科学综合
CiteScore
7.70
自引率
11.90%
发文量
100
审稿时长
3 months
期刊介绍: Astrobiology is the most-cited peer-reviewed journal dedicated to the understanding of life''s origin, evolution, and distribution in the universe, with a focus on new findings and discoveries from interplanetary exploration and laboratory research. Astrobiology coverage includes: Astrophysics; Astropaleontology; Astroplanets; Bioastronomy; Cosmochemistry; Ecogenomics; Exobiology; Extremophiles; Geomicrobiology; Gravitational biology; Life detection technology; Meteoritics; Planetary geoscience; Planetary protection; Prebiotic chemistry; Space exploration technology; Terraforming
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