Large Lakes Observatory, University of Minnesota Duluth, 2205 E. 5th St., Duluth, MN, 55812, USA.
Department of Physics and Astronomy, University of Minnesota Duluth, Duluth, MN, 55812, USA.
Nat Commun. 2019 Oct 7;10(1):4556. doi: 10.1038/s41467-019-12396-y.
The chemistry of the Early Earth is widely inferred from the elemental and isotopic compositions of sulfidic sedimentary rocks, which are presumed to have formed globally through the reduction of seawater sulfate or locally from hydrothermally supplied sulfide. Here we argue that, in the anoxic Archean oceans, pyrite could form in the absence of ambient sulfate from organic sulfur contained within living cells. Sulfides could be produced through mineralization of reduced sulfur compounds or reduction of organic-sourced sulfite. Reactive transport modeling suggests that, for sulfate concentrations up to tens of micromolar, organic sulfur would have supported 20 to 100% of sedimentary pyrite precipitation and up to 75% of microbial sulfur reduction. The results offer an alternative explanation for the low range of δS in Archean sulfides, and raise a possibility that sulfate scarcity delayed the evolution of dissimilatory sulfate reduction until the initial ocean oxygenation around 2.7 Ga.
早期地球的化学性质广泛地从硫化物沉积岩的元素和同位素组成推断得出,这些硫化物沉积岩被认为是通过海水硫酸盐的还原或局部通过热液供应的硫化物在全球范围内形成的。在这里,我们认为,在缺氧的太古代海洋中,由于活细胞内的有机硫的存在,黄铁矿可以在没有环境硫酸盐的情况下形成。硫化物可以通过还原态硫化合物的矿化或有机来源的亚硫酸盐的还原来产生。反应传输模型表明,对于硫酸盐浓度高达数十微摩尔,有机硫将支持 20%至 100%的沉积黄铁矿沉淀和高达 75%的微生物硫还原。研究结果为太古宙硫化物中δS 范围较低提供了另一种解释,并提出了硫酸盐稀缺可能延迟异化硫酸盐还原的进化,直到大约 27 亿年前海洋最初氧化的可能性。