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海水中的分子氢支持多种海洋细菌的生长。

Molecular hydrogen in seawater supports growth of diverse marine bacteria.

机构信息

Department of Microbiology, Biomedicine Discovery Institute, Monash University, Melbourne, Victoria, Australia.

School of Biological Sciences, Monash University, Melbourne, Victoria, Australia.

出版信息

Nat Microbiol. 2023 Apr;8(4):581-595. doi: 10.1038/s41564-023-01322-0. Epub 2023 Feb 6.

Abstract

Molecular hydrogen (H) is an abundant and readily accessible energy source in marine systems, but it remains unknown whether marine microbial communities consume this gas. Here we use a suite of approaches to show that marine bacteria consume H to support growth. Genes for H-uptake hydrogenases are prevalent in global ocean metagenomes, highly expressed in metatranscriptomes and found across eight bacterial phyla. Capacity for H oxidation increases with depth and decreases with oxygen concentration, suggesting that H is important in environments with low primary production. Biogeochemical measurements of tropical, temperate and subantarctic waters, and axenic cultures show that marine microbes consume H supplied at environmentally relevant concentrations, yielding enough cell-specific power to support growth in bacteria with low energy requirements. Conversely, our results indicate that oxidation of carbon monoxide (CO) primarily supports survival. Altogether, H is a notable energy source for marine bacteria and may influence oceanic ecology and biogeochemistry.

摘要

分子氢(H)是海洋系统中丰富且易于获取的能源,但目前尚不清楚海洋微生物群落是否消耗这种气体。在这里,我们使用了一系列方法来表明海洋细菌消耗 H 来支持生长。用于 H 摄取的氢化酶基因在全球海洋宏基因组中普遍存在,在宏转录组中高度表达,并在八个细菌门中发现。H 氧化能力随深度增加而增加,随氧浓度降低而降低,表明 H 在初级生产力低的环境中很重要。对热带、温带和亚南极水域以及无菌培养物的生物地球化学测量表明,海洋微生物会消耗在环境相关浓度下供应的 H,产生足够的细胞特异性能量,以支持对能量要求较低的细菌生长。相反,我们的结果表明,一氧化碳(CO)的氧化主要支持生存。总的来说,H 是海洋细菌的一个重要能源,可能会影响海洋生态和生物地球化学。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/8af6/10305171/4a435b40e978/41564_2023_1322_Fig1_HTML.jpg

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