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三种酶控制着地球上氧气的增加。

Three enzymes governed the rise of O on Earth.

机构信息

Department of Biology, Institute for Molecular Evolution, Heinrich Heine University of Duesseldorf, Duesseldorf, Germany.

Center for Genomic Sciences, UNAM Campus de Cuernavaca, Morelos, Mexico.

出版信息

Biochim Biophys Acta Bioenerg. 2024 Nov 1;1865(4):149495. doi: 10.1016/j.bbabio.2024.149495. Epub 2024 Jul 14.

DOI:10.1016/j.bbabio.2024.149495
PMID:39004113
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC7616410/
Abstract

Current views of O accumulation in Earth history depict three phases: The onset of O production by ∼2.4 billion years ago; 2 billion years of stasis at ∼1 % of modern atmospheric levels; and a rising phase, starting about 500 million years ago, in which oxygen eventually reached modern values. Purely geochemical mechanisms have been proposed to account for this tripartite time course of Earth oxygenation. In particular the second phase, the long period of stasis between the advent of O and the late rise to modern levels, has posed a puzzle. Proposed solutions involve Earth processes (geochemical, ecosystem, day length). Here we suggest that Earth oxygenation was not determined by geochemical processes. Rather it resulted from emergent biological innovations associated with photosynthesis and the activity of only three enzymes: 1) The oxygen evolving complex of cyanobacteria that makes O; 2) Nitrogenase, with its inhibition by O causing two billion years of oxygen level stasis; 3) Cellulose synthase of land plants, which caused mass deposition and burial of carbon, thus removing an oxygen sink and therefore increasing atmospheric O. These three enzymes are endogenously produced by, and contained within, cells that have the capacity for exponential growth. The catalytic properties of these three enzymes paved the path of Earth's atmospheric oxygenation, requiring no help from Earth other than the provision of water, CO, salts, colonizable habitats, and sunlight.

摘要

目前对地球历史上 O 积累的观点描绘了三个阶段:大约 24 亿年前 O 的产生开始;在现代大气水平的约 1%稳定了 20 亿年;大约 5 亿年前开始的上升阶段,其中氧气最终达到了现代水平。纯粹的地球化学机制被提出来解释地球氧合的这种三分期时间进程。特别是第二阶段,即 O 的出现与现代水平的后期上升之间的长时间稳定期,一直是个谜。提出的解决方案涉及地球过程(地球化学、生态系统、日照长度)。在这里,我们认为地球的氧合作用不是由地球化学过程决定的。相反,它是由与光合作用和只有三种酶的活性相关的新兴生物创新所导致的:1)蓝藻的产氧复合物,它产生 O;2)氮酶,其被 O 抑制导致 20 亿年的氧气水平稳定;3)陆地植物的纤维素合酶,它导致大量的碳沉积和埋藏,从而去除了一个氧气汇,因此增加了大气中的 O。这三种酶是由具有指数增长能力的细胞内源性产生的,并包含在细胞内。这三种酶的催化特性为地球的大气氧合铺平了道路,除了提供水、CO、盐、可殖民的栖息地和阳光外,不需要地球的任何帮助。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/5827e9766a63/EMS198314-f005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/2b63e52dff16/EMS198314-f001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/1c8cee8da206/EMS198314-f002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/b029a0a51f93/EMS198314-f003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/6dffadcf133a/EMS198314-f004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/5827e9766a63/EMS198314-f005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/2b63e52dff16/EMS198314-f001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/1c8cee8da206/EMS198314-f002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/b029a0a51f93/EMS198314-f003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/6dffadcf133a/EMS198314-f004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/cca6/7616410/5827e9766a63/EMS198314-f005.jpg

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