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Colonization of subsurface microbial observatories deployed in young ocean crust

机译:部署在年轻洋壳中的地下微生物观测站的定殖

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摘要

Oceanic crust comprises the largest hydrogeologic reservoir on Earth, containing fluids in thermodynamic disequilibrium with the basaltic crust. Little is known about microbial ecosystems that inhabit this vast realm and exploit chemically favorable conditions for metabolic activities. Crustal samples recovered from ocean drilling operations are often compromised for microbiological assays, hampering efforts to resolve the extent and functioning of a subsurface biosphere. We report results from the first in situ experimental observatory systems that have been used to study subseafloor life. Experiments deployed for 4 years in young (3.5 Ma) basaltic crust on the eastern flank of the Juan de Fuca Ridge record a dynamic, post-drilling response of crustal microbial ecosystems to changing physical and chemical conditions. Twisted stalks exhibiting a biogenic iron oxyhydroxide signature coated the surface of mineral substrates in the observatories; these are biosignatures indicating colonization by iron oxidizing bacteria during an initial phase of cool, oxic, iron-rich conditions following observatory installation. Following thermal and chemical recovery to warmer, reducing conditions, the in situ microbial structure in the observatory shifted, becoming representative of natural conditions in regional crustal fluids. Firmicutes, metabolic potential of which is unknown but may involve N or S cycling, dominated the post-rebound bacterial community. The archaeal community exhibited an extremely low diversity. Our experiment documented in situ conditions within a natural hydrological system that can pervade over millennia, exemplifying the power of observatory experiments for exploring the subsurface basaltic biosphere, the largest but most poorly understood biotope on Earth.
机译:大洋地壳包括地球上最大的水文地质储层,其中的流体与玄武岩地壳处于热力学不平衡状态。对于居住在这个广阔领域并利用化学上有利的代谢活动条件的微生物生态系统知之甚少。从海洋钻探作业中回收的地壳样品通常无法用于微生物分析,从而阻碍了解决地下生物圈范围和功能的努力。我们报告了来自第一个用于研究海底生命的原位实验观测系统的结果。在胡安德富卡海岭东侧年轻的(3.5 Ma)玄武岩地壳中进行了为期4年的实验,记录了地壳微生物生态系统对钻井后微生物生态系统对物理和化学条件变化的动态响应。扭曲的秸秆表现出生物羟基氧化铁的特征,覆盖了天文台矿物底物的表面。这些是生物特征,表明在天文台安装后,在寒冷,有氧,富铁条件的初始阶段,铁氧化细菌会定居。随着热量和化学物质恢复到温暖,减少的条件,天文台的原位微生物结构发生了变化,成为区域性地壳流体中自然条件的代表。反弹后细菌群落中,主要具有代谢潜力的硬毛菌,但可能涉及N或S循环。古细菌群落表现出极低的多样性。我们的实验记录了可以渗透数千年的自然水文系统中的原位条件,证明了观测实验对探索地下玄武质生物圈(地球上最大,但最难理解的生物群落)的力量。

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