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32 亿年前浅海硅质碎屑岩沉积中的有壁微体化石。

Organic-walled microfossils in 3.2-billion-year-old shallow-marine siliciclastic deposits.

机构信息

Department of Geology, University of Liège, 17 allée du 6 Août B18, Liège 4000, Belgium.

出版信息

Nature. 2010 Feb 18;463(7283):934-8. doi: 10.1038/nature08793. Epub 2010 Feb 7.

Abstract

Although the notion of an early origin and diversification of life on Earth during the Archaean eon has received increasing support in geochemical, sedimentological and palaeontological evidence, ambiguities and controversies persist regarding the biogenicity and syngeneity of the record older than Late Archaean. Non-biological processes are known to produce morphologies similar to some microfossils, and hydrothermal fluids have the potential to produce abiotic organic compounds with depleted carbon isotope values, making it difficult to establish unambiguous traces of life. Here we report the discovery of a population of large (up to about 300 mum in diameter) carbonaceous spheroidal microstructures in Mesoarchaean shales and siltstones of the Moodies Group, South Africa, the Earth's oldest siliciclastic alluvial to tidal-estuarine deposits. These microstructures are interpreted as organic-walled microfossils on the basis of petrographic and geochemical evidence for their endogenicity and syngeneity, their carbonaceous composition, cellular morphology and ultrastructure, occurrence in populations, taphonomic features of soft wall deformation, and the geological context plausible for life, as well as a lack of abiotic explanation falsifying a biological origin. These are the oldest and largest Archaean organic-walled spheroidal microfossils reported so far. Our observations suggest that relatively large microorganisms cohabited with earlier reported benthic microbial mats in the photic zone of marginal marine siliciclastic environments 3.2 billion years ago.

摘要

尽管在地球太古宙时期生命的早期起源和多样化的概念在地球化学、沉积学和古生物学证据中得到了越来越多的支持,但对于晚太古宙之前的记录的生物成因和同源性仍然存在一些模糊和争议。人们知道,非生物过程会产生与一些微生物类似的形态,而热液流体有可能产生具有贫碳同位素值的无生命有机化合物,这使得很难确定生命的明确痕迹。在这里,我们报告了在南非最古老的硅质碎屑冲积到潮汐河口沉积的中太古宙页岩和粉砂岩中发现了一群大的(直径可达约 300 微米)碳质球状体微观结构的情况。这些微观结构被解释为有机壁微化石,这是基于其内生性和同源性、碳质组成、细胞形态和超微结构、群体出现、软壁变形的埋藏特征以及对生命的地质背景的证据,以及缺乏否定生物起源的非生物解释。这些是迄今为止报道的最古老和最大的太古宙有机壁球状体微化石。我们的观察表明,相对较大的微生物与之前报道的边缘海硅质碎屑环境中浅海区域的早期底栖微生物垫共同存在,时间可追溯到 32 亿年前。

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