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早期分支蓝细菌的分布以及产生最早产氧光合生物的潜在栖息地。

Distribution of early-branching Cyanobacteriia and the potential habitats that gave rise to the earliest oxygenic phototrophs.

作者信息

Grettenberger Christen, Gold David A, Brown C Titus

机构信息

Department of Earth and Planetary Sciences, University of California Davis, Davis, California, USA.

Department of Environmental Toxicology, University of California Davis, Davis, California, USA.

出版信息

mSphere. 2025 Feb 25;10(2):e0101324. doi: 10.1128/msphere.01013-24. Epub 2025 Jan 30.

Abstract

The evolution of oxygenic photosynthesis in the Cyanobacteria was one of the most transformative events in Earth history, eventually leading to the oxygenation of Earth's atmosphere. However, it is difficult to understand how the earliest Cyanobacteria functioned or evolved on early Earth in part because we do not understand their ecology, including the environments in which they lived. Here, we use a cutting-edge bioinformatics tool to survey nearly 500,000 metagenomes for relatives of the taxa that likely bookended the evolution of oxygenic photosynthesis to identify the modern environments in which these organisms live. Ancestral state reconstruction suggests that the common ancestors of these organisms lived in terrestrial (soil and/or freshwater) environments. This restricted distribution may have increased the lag between the evolution of oxygenic photosynthesis and the oxygenation of Earth's atmosphere.IMPORTANCECyanobacteria generate oxygen as part of their metabolism and are responsible for the rise of oxygen in Earth's atmosphere over two billion years ago. However, we do not know how long this process may have taken. To help constrain how long this process would have taken, it is necessary to understand where the earliest Cyanobacteria may have lived. Here, we use a cutting-edge bioinformatics tool called branch water to examine the environments where modern Cyanobacteria and their relatives live to constrain those inhabited by the earliest Cyanobacteria. We find that these species likely lived in non-marine environments. This indicates that the rise of oxygen may have taken longer than previously believed.

摘要

蓝细菌中含氧光合作用的演化是地球历史上最具变革性的事件之一,最终导致了地球大气的氧化。然而,很难理解最早的蓝细菌在早期地球上是如何发挥作用或演化的,部分原因是我们不了解它们的生态,包括它们生活的环境。在这里,我们使用一种前沿的生物信息学工具,对近50万个宏基因组进行调查,以寻找可能标志着含氧光合作用演化的分类群的亲属,从而确定这些生物生存的现代环境。祖先状态重建表明,这些生物的共同祖先生活在陆地(土壤和/或淡水)环境中。这种有限的分布可能增加了含氧光合作用的演化与地球大气氧化之间的时间间隔。

重要性

蓝细菌在其新陈代谢过程中产生氧气,并导致了20多亿年前地球大气中氧气的增加。然而,我们不知道这个过程可能持续了多久。为了帮助确定这个过程持续的时间,有必要了解最早的蓝细菌可能生活在哪里。在这里,我们使用一种名为分支水的前沿生物信息学工具,来研究现代蓝细菌及其亲属生活的环境,以确定最早的蓝细菌所栖息的环境。我们发现这些物种可能生活在非海洋环境中。这表明氧气的增加可能比之前认为的要花更长时间。

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