冲绳海槽海底黑烟囱中微生物化石的发现及其意义

采用光学显微镜以及扫描电镜对冲绳海槽海底黑烟囱样品进行研究,发现了大量的微生物化石,它们保留了完好的形态,主要有四种不同类型的丝状体,可能是硫或者铁氧化化能自养细菌和真菌。这些化石微生物的鉴别基于大小、形状、细胞分裂、群落聚集等物理标志。初步研究表明这些微生物不仅依存于海底热液活动,同时在热液成矿过程中起着重要的作用。     

嗜热微生物及在高温生物冶金过程中的应用

嗜热微生物包括中度嗜热微生物和极端嗜热微生物,主要栖息于热泉、火山口、海底热液喷口、高温反应器以及工厂高温废水排放区等自然或人为产生的高温环境中。它们可以生活在40-80°C、甚至更高的温度中,其中有些具备嗜酸性及特殊的代谢类型,在高温生物冶金过程中具有应用潜力。高温生物冶金较传统中温生物冶金更具优势,其能浸出某些难处理矿、解决浸矿过程的钝化问题,以及提高浸出效率等,目前已引起了生物冶金工业的重视。本文概述了应用于生物冶金的主要嗜热微生物的生理特点、耐热机制以及对铁、铜和砷等离子的耐受机制,进一步介绍了嗜热微生物在高温生物冶金中的发展及应用。     

分子生物学技术在热泉地质微生物学研究中的应用

陆地热泉是一类典型的极端生命-环境互作的地质系统,是我们认识生命与环境协同演化的天然实验室。然而,受限于有限的研究手段,热泉中仍存在大量未解密的微生物"暗物质"。这种困境随着技术的革新得到了改善,尤其是近几年来基于组学、探针和同位素标记的多元化检测手段在嗜热微生物多样性的挖掘、新物种和新代谢途径的发现以及嗜热微生物对元素地球化学循环的调控和响应等方面取得了一系列令人瞩目的研究成果,使得热泉极端微生物和地质环境内在联系的研究也成为地质微生物学研究的热点。立足于前人研究成果,本文将简述常用于热泉地质微生物学研究的分子生物学手段的发展,重点总结其在挖掘热泉微生物多样性和热泉微生物的环境功能研究中的应用及进展,最后对未来研究方向提出展望。     

微生物在珊瑚礁生态系统中的作用与功能

珊瑚礁是由珊瑚、鱼类、底栖生物、藻类以及微生物等多种生命形式组成的聚集体,代表着一类典型的海洋生态系统.珊瑚礁存在于热带和亚热带的寡营养环境,拥有极高的初级生产力和生产效率,被誉为“海底热带雨林”.微生物在珊瑚礁生态系统的生物地球化学循环、物质转化以及健康维护上具有重要作用.随着分子生态学的发展,微生物在珊瑚中的作用和功能日益凸显.本文总结了微生物生态学的研究现状,包括珊瑚生态系统中微生物的定植方式,共生微生物的特性(专一性、可塑性、协同进化),共生微生物与珊瑚疾病的关系与信号调节,以及微生物应对全球变化(气温升高、海水酸化、富营养化)的响应.从“珊瑚 微生物”共生体的发生、共生微生物的特性与生态功能,以及全球环境变化下微生物的衍生效应来梳理最新理论与成果,明确珊瑚微生物生态学机制,为更好地保护珊瑚资源、维护海洋生物多样性提供理论借鉴.     

热泉微生物驱动的氮循环研究进展及展望

热泉微生物是驱动热泉氮(N)循环的主导力量,开展热泉生态系统中驱动氮循环微生物种群构成及其与环境响应的研究,对于探索热泉中氮的生物地球化学循环、生命进化、生物修复等方面都具有重要的理论和应用价值。本文综合阐述了热泉生态系统驱动氮循环的功能微生物(如固氮菌、氨氧化菌、厌氧氨氧化菌、反硝化菌、异化硝酸盐还原菌)在系统发育学上的分布、功能基因的相对丰度、活性及其与环境因子(如温度、pH)的相关性等方面的研究现状和亟待解决的问题。并展望了热泉生境中驱动氮循环微生物未来的研究方向。     

多重极端环境中的生命:深海热液中的超嗜热古菌Thermococclaes

超嗜热古菌Thermococcales是一类在类早期地球环境深海热液系统中常见的优势微生物类群,同时也是一类很好地适应了热液系统中剧烈波动的理化因子的微生物,部分Thermococcales微生物具有惊人的生长跨度(超过40℃的温度生长跨度、超过5个pH单位的pH生长跨度以及超过80 MPa的压力生长跨度),同时与其他绝大多数微生物相比具有较小的基因组(2.3 Mb).有关Thermococcales在不同极端环境下的适应性研究发现,其特殊的代谢途径与多重极端环境适应相关,这些代谢途径包括:相容性溶质、能量代谢、膜脂、氨基酸代谢及抗氧化途径,进而发现可能存在应对多重极端环境的共同适应机制.研究Thermococcales的共同适应机制,可帮助探索深部生物圈这样低能、高温极端环境下(包括域外)微生物的生存策略,将为探究早期生命的代谢特点,进而更好地理解生命起源提供宝贵的模型和研究思路,也为合成生物学研究及工业化应用提供理论借鉴与生物材料.     

西南印度洋中脊热液羽状流中微生物化石的发现及意义

深海热液微生物因其生存于海底极端环境,能够提供深部生物圈和生物地球化学信息而成为当今海洋科学领域关心的热点问题之一.本文以西南印度洋中脊热液羽状流水体中悬浮颗粒物为研究对象,选取典型的3个CTD采水站位,对离底42-500m的不同水层悬浮体过滤的滤膜进行扫描电镜观察和X射线能谱面扫描分析.结果表明,热液羽状流颗粒物中含有大量的微生物化石,包括丝状、球状、杆状和簇状等4种形态.对不同形态微生物化石能谱分析表明Si、O、Ca、Fe和Zn等元素在微生物化石中都有高值出现,其中丝状体中具有Ti和Mn的高值出现,球状体中Ba具有高值,说明微生物化石化过程中不同类型的微生物体对金属元素的选择性吸收,钙化和铁硅酸盐岩化是微生物化石化的主要机制.微生物化石在羽状流中的分布状况能够提供活动热液喷口的空间信息,为我们寻找喷口提供帮助.     

河北兴隆中元古代古海底黑烟囱中微生物化石的发现及其意义

采用显微镜以及扫描电镜对冀东中元古代块状硫化物黑烟囱样品进行研究,首次发现了矿化微生物化石。它们为丝状体,均已黄铁矿化,经过激光拉曼光谱测试发现还保留少量有机质,可以与现代海底黑烟囱周围矿化微生物对比。这些化石微生物的鉴别基于大小、形状和群落聚集等物理标志。     

云南地区热泉中氨氧化菌丰度对环境条件的响应

【目的】研究热泉中的氨氧化菌对于理解全球氮循环作用至关重要,而人们对于热泉中环境条件对氨氧化菌丰度分布的影响还知之甚少。本研究旨在研究云南热泉中氨氧化菌的丰度以及热泉环境因子(例如:温度、氨浓度及pH等)对氨氧化菌丰度的影响。【方法】在所选取的热泉中,采集沉积物、菌席或泉华样品。使用RNA逆转录、定量聚合酶链式反应及荧光原位杂交等技术对样品中各微生物种群进行定量分析。【结果】所选取的热泉沉积物、菌席或泉华中微生物总量大约为108-109细胞/g。其中,氨氧化古菌(AOA)占样品中微生物总量的0.02-1.32%,而氨氧化细菌数量低于检测下限。地球化学参数和AOA相对丰度的相关性统计分析显示,氨氧化古菌相对丰度值与NH3、NO2-、NO3-浓度和温度等具有统计学意义上的相关性,而其与Fe2+和及盐度无统计学意义上的相关性。【结论】在所调查的热泉中,氨氧化微生物种群主要由AOA组成,AOA在热泉中的氨氧化生物地球化学过程中起着重要作用。热泉中多个环境因子一起控制着AOA丰度在不同热泉中的分布特征,而某些环境因子,如盐度-和Fe2+浓度,可能不是控制AOA分布特征的关键因素。     

深海极端微生物菌群及代谢产物多样性的研究进展

海洋覆盖了地球表面积的四分之三,它不仅是生命的起源,而且还孕育了各种极端微生物。它们存在于海洋极端环境中,如热液喷口、热泉、咸湖和深海层等,由于生境太过恶劣,一度被认为是生命的禁区。随着人类对深海极端环境微生物研究的不断深入,已经探索到那里具有丰富的菌群资源和具有潜在价值的天然生物活性产物。这些极端微生物能够适应极高温、极低温、高压、高盐、高放射性和极度酸碱性等极端环境,具有特殊的生物多样性、遗传背景和代谢途径,能够产生各种具有特殊功能的酶类及其他活性物质,展现出巨大的研究价值和应用潜力。研究海洋极端微生物对探索生物多样性、新资源开发利用及对地球生物学研究等都具有重要意义。     

Microbial biosignatures in ancient deep-sea hydrothermal sulfides

Deep-sea hydrothermal systems provide ideal conditions for prebiotic reactions and ancient metabolic pathways and, therefore, might have played a pivotal role in the emergence of life. To understand this role better, it is paramount to examine fundamental interactions between hydrothermal processes, non-living matter, and microbial life in deep time. However, the distribution and diversity of microbial communities in ancient deep-sea hydrothermal systems are still poorly constrained, so evolutionary, and ecological relationships remain unclear. One important reason is an insufficient understanding of the formation of diagnostic microbial biosignatures in such settings and their preservation through geological time. This contribution centers around microbial biosignatures in Precambrian deep-sea hydrothermal sulfide deposits. Intending to provide a valuable resource for scientists from across the natural sciences whose research is concerned with the origins of life, we first introduce different types of biosignatures that can be preserved over geological timescales (rock fabrics and textures, microfossils, mineral precipitates, carbonaceous matter, trace metal, and isotope geochemical signatures). We then review selected reports of biosignatures from Precambrian deep-sea hydrothermal sulfide deposits and discuss their geobiological significance. Our survey highlights that Precambrian hydrothermal sulfide deposits potentially encode valuable information on environmental conditions, the presence and nature of microbial life, and the complex interactions between fluids, micro-organisms, and minerals. It further emphasizes that the geobiological interpretation of these records is challenging and requires the concerted application of analytical and experimental methods from various fields, including geology, mineralogy, geochemistry, and microbiology. Well-orchestrated multidisciplinary studies allow us to understand the formation and preservation of microbial biosignatures in deep-sea hydrothermal sulfide systems and thus help unravel the fundamental geobiology of ancient settings. This, in turn, is critical for reconstructing life's emergence and early evolution on Earth and the search for life elsewhere in the universe.     

Exploration of deep intraterrestrial microbial life: current perspectives

Intraterrestrial life has been found at depths of several thousand metres in deep sub-sea floor sediments and in the basement crust beneath the sediments. It has also been found at up to 2800-m depth in continental sedimentary rocks, 5300-m depth in igneous rock aquifers and in fluid inclusions in ancient salt deposits from salt mines. The biomass of these intraterrestrial organisms may be equal to the total weight of all marine and terrestrial plants. The intraterrestrial microbes generally seem to be active at very low but significant rates and several investigations indicate chemolithoautotrophs to form a chemosynthetic base. Hydrogen, methane and carbon dioxide gases are continuously generated in the interior of our planet and probably constitute sustainable sources of carbon and energy for deep intraterrestrial biosphere ecosystems. Several prospective research areas are foreseen to focus on the importance of microbial communities for metabolic processes such as anaerobic utilisation of hydrocarbons and anaerobic methane oxidation.     

Biomarkers Reveal Diverse Microbial Communities in Black Smoker Sulfides from Turtle Pits (Mid-Atlantic Ridge,Recent) and Yaman Kasy (Russia,Silurian)

The steep biogeochemical gradients near deep sea hydrothermal vents provide various niches for microbial life. Here we present biosignatures of such organisms enclosed in a modern and an ancient hydrothermal sulfide deposit (Turtle Pits, Mid-Atlantic Ridge, Recent; Yaman Kasy, Russia, Silurian). In the modern sulfide we found high amounts of specific bacterial and archaeal biomarkers with δ¹³C values between ?8 and ?37‰ VPDB. Our data indicate the presence of thermophilic members of the autotrophic Aquificales using the reductive tricarboxylic acid (rTCA) cycle as well as of methanogenic and chemolithoheterotrophic Archaea. In the ancient sample, most potential biomarkers of thermophiles were obscured by compounds derived from allochthonous organic matter (OM), except for an acyclic C₄₀ biphytane and its C₃₉ breakdown product. Both samples contained high amounts of unresolved complex mixtures (UCM) of hydrocarbons. Apparently, OM in the sulfides had to withstand high thermal stress, indicated by highly mature hopanes, steranes, and cheilanthanes with up to 41 carbon atoms.     

Search for life in deep biospheres]

The life in deep biospheres bridges conventional biology and future exobiology. This review focuses the microbiological studies from the selected deep biospheres, i.e., deep-sea hydrothermal vents, sub-hydrothermal vents, terrestrial subsurface and a sub-glacier lake. The dark biospheres facilitate the emergence of organisms and communities dependent on chemolithoautotrophy, which are overwhelmed by photoautotrophy (photosynthesis) in the surface biospheres. The life at deep-sea hydrothermal vents owes much to chemolithoautotrophy based on the oxidation of sulfide emitted from the vents. It is likely that similarly active bodies such as the Jovian satellite Europa may have hydrothermal vents and associated biological communities. Anoxic or anaerobic condition is characteristic of deep subsurface biospheres. Subsurface microorganisms exploit available oxidants, or terminal electron acceptors (TEA), for anaerobic respiration. Sulfate, nitrate, iron (III) and CO2 are the representative TEAs in the deep subsurface. Below the 3000-4000 m-thick glacier on Antarctica, there have been >70 lakes with liquid water located. One of such sub-glacial lakes, Lake Vostok, is about to be drill-penetrated for microbiological studies. These deep biosphere "platforms" provide new knowledge about the diversity and potential of the Earth's life. The expertise obtained from the deep biosphere expeditions will facilitate the capability of exobiologial exploration.     

Phylogenetic diversity of nitrogenase (nifH) genes in deep-sea and hydrothermal vent environments of the Juan de Fuca Ridge

The subseafloor microbial habitat associated with typical unsedimented mid-ocean-ridge hydrothermal vent ecosystems may be limited by the availability of fixed nitrogen, inferred by the low ammonium and nitrate concentrations measured in diffuse hydrothermal fluid. Dissolved N2 gas, the largest reservoir of nitrogen in the ocean, is abundant in deep-sea and hydrothermal vent fluid. In order to test the hypothesis that biological nitrogen fixation plays an important role in nitrogen cycling in the subseafloor associated with unsedimented hydrothermal vents, degenerate PCR primers were designed to amplify the nitrogenase iron protein gene nifH from hydrothermal vent fluid. A total of 120 nifH sequences were obtained from four samples: a nitrogen-poor diffuse vent named marker 33 on Axial Volcano, sampled twice over a period of 1 year as its temperature decreased; a nitrogen-rich diffuse vent near Puffer on Endeavour Segment; and deep seawater with no detectable hydrothermal plume signal. Subseafloor nifH genes from marker 33 and Puffer are related to anaerobic clostridia and sulfate reducers. Other nifH genes unique to the vent samples include proteobacteria and divergent ARCHAEA: All of the nifH genes from the deep-seawater sample are most closely related to the thermophilic, anaerobic archaeon Methanococcus thermolithotrophicus (77 to 83% amino acid similarity). These results provide the first genetic evidence of potential nitrogen fixers in hydrothermal vent environments and indicate that at least two sources contribute to the diverse assemblage of nifH genes detected in hydrothermal vent fluid: nifH genes from an anaerobic, hot subseafloor and nifH genes from cold, oxygenated deep seawater.     

Organic sulfur metabolisms in hydrothermal environments

Sulfur is central to the metabolisms of many organisms that inhabit extreme environments. While biotic and abiotic cycling of organic sulfur compounds has been well documented in low‐temperature anaerobic environments, cycling of organic sulfur in hydrothermal environments has received less attention. Recently published thermodynamic data have been used to estimate aqueous alkyl thiol and sulfide activities in deep‐sea hydrothermal systems. Here we use geochemical mixing models to predict fluid compositions that result from mixing end‐member hydrothermal fluid from the East Pacific Rise with bottom seawater. These fluid compositions are combined with estimates of methanethiol and dimethylsulfide activities to evaluate energy yields for potential organic sulfur‐based metabolisms under hydrothermal conditions. Aerobic respiration has the highest energy yields (over ?240 kJ/mol e^?) at lower temperature; however, oxygen is unlikely to persist at high temperatures, restricting aerobic respiration to mesophilic communities. Nitrite reduction to N₂ has the highest energy yields at higher temperatures (greater than ～40 °C). Nitrate and nitrite reduction to ammonium also yield significant energy (up to ?70 kJ/mol e^?). Much lower, but still feasible energy yields are calculated for sulfate reduction, disproportionation, and reduction with H₂. Organic compound family and the activity of methanethiol and dimethylsulfide were less important than metabolic strategy in determining overall energy yields. All metabolic strategies considered were exergonic within some portion of the mixing regime suggesting that organic sulfur‐based metabolisms may be prevalent within deep‐sea hydrothermal vent microbial communities.     

Incidence of novel and potentially archaeal nitrogenase genes in the deep Northeast Pacific Ocean

Archaea have been detected throughout the oceanic water column and are quantitatively important members of picoplankton in the deep ocean. Two common groups, group I Crenarchaeota and group II Euryarchaeota, are consistently detected in warm hydrothermal fluid and are assumed to have been drawn into the subseafloor, mixed with hydrothermal fluid and then expelled. However, because they remain resistant to cultivation, very little is known about their physiology. Here we show that cold deep-seawater from the axial valley of Endeavour Segment on the Juan de Fuca Ridge contains not only groups I and II archaea as expected, but also unique potentially archaeal nitrogenase (nifH) genes, which are required for nitrogen fixation. These nifH genes are phylogenetically distinct and have dissimilar G+C content compared with those of hydrothermal vent archaea, suggesting that they belong to non-thermophilic deep-sea archaea. Furthermore, this sample did not contain mcrA genes, which are present in methanogens, the only known archaeal nitrogen fixers. These nifH genes were not detected in upper water column samples, or in a deep-seawater sample 100 km away from the spreading axis of the Juan de Fuca Ridge. We propose that these unique nifH genes may be localized to archaea that circulate through the nitrogen-poor subseafloor at the mid-ocean ridge as part of their life cycle.     

Phylogenetic Diversity of Nitrogenase (nifH) Genes in Deep-Sea and Hydrothermal Vent Environments of the Juan de Fuca Ridge

The subseafloor microbial habitat associated with typical unsedimented mid-ocean-ridge hydrothermal vent ecosystems may be limited by the availability of fixed nitrogen, inferred by the low ammonium and nitrate concentrations measured in diffuse hydrothermal fluid. Dissolved N₂ gas, the largest reservoir of nitrogen in the ocean, is abundant in deep-sea and hydrothermal vent fluid. In order to test the hypothesis that biological nitrogen fixation plays an important role in nitrogen cycling in the subseafloor associated with unsedimented hydrothermal vents, degenerate PCR primers were designed to amplify the nitrogenase iron protein gene nifH from hydrothermal vent fluid. A total of 120 nifH sequences were obtained from four samples: a nitrogen-poor diffuse vent named marker 33 on Axial Volcano, sampled twice over a period of 1 year as its temperature decreased; a nitrogen-rich diffuse vent near Puffer on Endeavour Segment; and deep seawater with no detectable hydrothermal plume signal. Subseafloor nifH genes from marker 33 and Puffer are related to anaerobic clostridia and sulfate reducers. Other nifH genes unique to the vent samples include proteobacteria and divergent Archaea. All of the nifH genes from the deep-seawater sample are most closely related to the thermophilic, anaerobic archaeon Methanococcus thermolithotrophicus (77 to 83% amino acid similarity). These results provide the first genetic evidence of potential nitrogen fixers in hydrothermal vent environments and indicate that at least two sources contribute to the diverse assemblage of nifH genes detected in hydrothermal vent fluid: nifH genes from an anaerobic, hot subseafloor and nifH genes from cold, oxygenated deep seawater.     

Ancient life and moving fluids

Over 3.7 billion years of Earth history, life has evolved complex adaptations to help navigate and interact with the fluid environment. Consequently, fluid dynamics has become a powerful tool for studying ancient fossils, providing insights into the palaeobiology and palaeoecology of extinct organisms from across the tree of life. In recent years, this approach has been extended to the Ediacara biota, an enigmatic assemblage of Neoproterozoic soft-bodied organisms that represent the first major radiation of macroscopic eukaryotes. Reconstructing the ways in which Ediacaran organisms interacted with the fluids provides new insights into how these organisms fed, moved, and interacted within communities. Here, we provide an in-depth review of fluid physics aimed at palaeobiologists, in which we dispel misconceptions related to the Reynolds number and associated flow conditions, and specify the governing equations of fluid dynamics. We then review recent advances in Ediacaran palaeobiology resulting from the application of computational fluid dynamics (CFD). We provide a worked example and account of best practice in CFD analyses of fossils, including the first large eddy simulation (LES) experiment performed on extinct organisms. Lastly, we identify key questions, barriers, and emerging techniques in fluid dynamics, which will not only allow us to understand the earliest animal ecosystems better, but will also help to develop new palaeobiological tools for studying ancient life.     

Biomarkers as Tracers for Life on Early Earth and Mars

Biomarkers in geological samples are products derived from biochemical (natural product) precursors by reductive and oxidative processes (e.g., cholestanes from cholesterol). Generally, lipids, pigments and biomembranes are preserved best over longer geological times and labile compounds such as amino acids, sugars, etc. are useful biomarkers for recent times. Thus, the detailed characterization of biomarker compositions permits the assessment of the major contributing species of extinct and/or extant life. In the case of the early Earth, work has progressed to elucidate molecular structure and carbon isotopic signals preserved in ancient sedimentary rocks. In addition, the combination of bacterial biochemistry with the organic geochemistry of contemporary and ancient hydrothermal ecosystems permits the modeling of the nature, behavior and preservation potential of primitive microbial communities. This approach uses combined molecular and isotopic analyses to characterize lipids produced by cultured bacteria (representative of ancient strains) and to test a variety of culture conditions which affect their biosynthesis. On considering Mars, the biomarkers from lipids and biopolymers would be expected to be preserved best if life flourished there during its early history (3.5–4 × 10⁹ yr ago). Both oxidized and reduced products would be expected. This is based on the inferred occurrence of hydrothermal activity during that time with the concomitant preservation of biochemically-derived organic matter. Both known biomarkers (i.e., as elucidated for early terrestrial samples and for primitive terrestrial microbiota) and novel, potentially unknown compounds should be characterized.