Hydrostatic pressure is the universal key driver of microbial evolution in the deep ocean and beyond
Hydrostatic pressure is the universal key driver of microbial evolution in the deep ocean and beyond
复制标题
静水压力是深海及其他海域微生物进化的普遍关键驱动力
DOI:
10.1111/1758-2229.12915
复制
发表时间:
2021
影响因子:
3.3
通讯作者:
Fengping Wang
中科院分区:
文献类型:
--
作者:
Xiang Xiao;Yu Zhang;Fengping Wang
Oceans cover approximately 70% of the Earth’s surface, and microbes comprise 90% of the ocean biomass and are regarded as an important ‘hidden’driver of essential elemental cycling, such as carbon cycling, in the oceans (Karl, 2007; Salazar and Sunagawa, 2017). Although the general public–even many scientists–think of the oceans as unified, stable water systems, they contain varied environments, including extreme environments such as oxygen-deficient zones, oligotrophic open ocean, polar water regions, deep ocean, hydrothermal vents, cold seeps, and so on, where specific microbial communities have evolved (Fig. 1). Hydrostatic pressure influences the physiology of organisms living at depth in the oceans, which is the largest habitat of the biosphere in terms of volume (1.3× 1018 m3)(Whitman et al., 1998). While traditional biological oceanographic research focuses more on the photic zone of the ocean, more attention is now being paid to the dark deep ocean due to the advancement of deep-ocean engineering technologies and the rapid progress of molecular biology, particularly next-generation DNA sequencing technologies. The deep ocean refers to those ocean waters with a depth greater than 1000 m, corresponding to a hydrostatic pressure of higher than 10 MPa. Knowledge of the composition and distribution of the microbiome in the deep ocean and subsurface environments is accumulating; for instance, mostly thermophilic, sulfur-metabolizing microbes, such as Thermoccoccus, Pyrococcus, and Episilonproteobacteria, are found to be the major functional groups in the hot fluid venting hydrothermal vent chimneys, and the microbial community has been discovered to shift to a community metabolizing iron–sulfur minerals after the venting ceased (Hou et al., 2020), indicating energy source is the driving force behind the microbiome shift. Microbes in the subsurface are shown to have metabolic flexibility, which helps them survive in energy-deficient environments (Li et al., 2020). Various environmental factors, such as temperature, salinity, nutrients, and chemical reactants (electron donors and electron acceptors), have been investigated to understand their roles on deep sea microbial growth, and some factors shown to be critical in shaping community structure and even the evolution of the microbiome. Although high hydrostatic pressure (HHP) is the most common environmental factor in the ocean and subsurface (Fig. 1), its independent and joint effects with other environmental factors on microbiomes (structure, function, and evolution) have never been systematically investigated and understood. Therefore, here we call for the scientific community to give special attention to this largely present but mostly ignored environmental parameter, ie, HHP, and its roles in shaping microbial physiology, community structure, and evolution. HHP has profound effects on cellular physiology and cytological behaviour, including transcription, translation, membrane compositions, multimeric protein assemblages, protein structure, and cellular motility, which have been studied in piezosensitive model organisms like