PREFACE Biologists divide living organisms into prokaryotes, represented by the bacteria, and eukaryotes such as ourselves. In this scheme, bacteria are considered to be the most primitive form of life. One popular idea about how life arose supposes that humans evolved from bacteria. In this age of genomics, however, DNA sequence comparisons indicate that our genes are unlike those of bacteria. Where, then, did we come from? An answer to that question comes from a truly unexpected source, life in extreme environments. It was generally thought that boiling acid hot springs or saturating saline lakes were sterile, however, life is both present and highly suc- cessful. Many of the resident organisms are still microbes, just not bac- teria. We call them archaea. Whole-genome DNA sequences of five ar- chaeal species reveal remarkable gene matches to human genes and those of other eukaryotes. These matches occur in the most essential of the subcellular processes carried out by all organisms, the synthe- sis and repair of DNA, RNA, and protein. This suggests that eukaryotes evolved from archaea or perhaps that archaea and eukaryotes derive from a common ancestor. Gene sequences aside, archaea lay additional claim to the title of an- cient organism based on geologic and taxonomic considerations. The early Earth (Archean age) was a time of elevated surface temperatures. Fossil dating indicates the presence of microbes at the close of this pe- riod, suggesting that earlier forms of life from which these fossils would have derived must have been adapted to temperature extremes. Mi- crobes called hyperthermophiles with just these abilities are still found on the Earth in geothermal springs and hydrothermal ocean vents. These extreme locations exhibit geochemistries most like that of early Earth. To understand how such organisms relate to other forms of life, taxo- nomic methods based on ribosomal RNA sequences have been used to create phylogenetic “trees” of life. These hyperthermophilic microbes, dominated by the archaea, exhibit the deepest phylogenetic branches, suggesting that they have undergone the longest period of evolution among extant organisms. Taken together, these ideas suggest that hyper- thermophilic archaea may represent a form of the earliest type of life. The intent of this book is to expand the general understanding of the archaea. As simple organisms with sequenced genomes, they present unique opportunities to understand better our own origins and, indeed, ix X PREFACE the origin of life. As prokaryotes they provide powerful experimental systems for genetic and molecular experimentation. Acknowledgments I am most grateful for the support and interest of many colleagues, in- cluding Rolf Bernander, Mike Dyall-Smith, Peter Kennelly, John Leigh, William Metcalf, Kenneth Noll, Frank Robb, Richard Shand, Dieter Soll, and William Whitman. The pioneering interests of Thomas Brock, Richard Morita, Norman Pace, Carl Stetter, Carl Wose, and Wolfram Zillig helped create my interest in extreme environments and the evo- lutionary implications of life native to such habitats. INTRODUCTION Ribosomal RNA gene sequence comparisons separate life into three distantly related groups or domains (Fig. 1). Eukaryotes constitute one domain, encompassing single- and multicelled organisms such as plants and animals. Despite their morphologic simplicity and apparent simi- larity, the other two domains are both prokaryotic. These domains are represented by the bacteria and the archaea. Differences in rRNA se- quence are but one feature leading to this classification system. Most scientists are well versed about the evidence which distinguishes bac- terial from eukaryotic life. This includes a diversity of mechanisms governing all aspects of basic cell biology, from gene organization to gene expression, from signal transduction to metabolism. What, then, beyond differences in rRNA sequence supports the separate classifi- cation of the archaea from bacterial prokaryotes and eukaryotes? As predicted by their rRNA sequence divergence and by analogy to the dissimilarity between bacteria and eukaryotes, archaea are likely to em- ploy archaeal-specific subcellular mechanisms for conducting essential processes. While the existence of archaeal-specific subcellular mech- anisms is supported by the occurrence of a unique group of archaeal orthologous genes, the functions of these genes remain unknown. The truly remarkable discovery which is the focus of this book concerns the finding that archaea use eukaryotic-like mechanisms and not bacterial mechanisms for much of their information processing functions. The literature on bacterial prokaryotes is both extensive and diverse, however, such is not yet the case for archaea. As a recognized group, archaea are relative newcomers to the prokaryotic world. Despite their recent entry into the research arena, studies on archaea are blossom- ing, largely in response to the availability of whole-genome DNA se- quences. Three distinctive biotypes of archaea are best known: the methanogens, the halophiles, and the hyperthermophiles. Due to the radical nature of their respective niches, these organisms have been dubbed extremophiles. Studies on life in extreme environments portend many exciting areas in biology research including studies on the origins of life and the possibility of extraplanetary organisms. Archaea have contributed, and will continue to contribute, greatly to these areas. How- ever, phylogenetic studies of marine, dirt, and other environmental sam- ples indicate that some archaea are not extremophilic but mesophilic members of microbial communities. More importantly, these types of xi xii INTRODUCTION ‘Plants FIG. 1. Archaeal, bacterial, and eukaryotic sequences were aligned with ClustalW. The programs DNADIST, NEIGHBOR, CONSENSE, and FITCH, of the Phylip package, were used to build the tree. The alignment was bootstrapped 100 times with SEQBOOT. archaea appear to constitute a significant proportion of the total plane- tary microbial biomass. This book provides an overview of key aspects of the archaea includ- ing chapters on their genomics and phylogeny, micropaleontology, cell biology, and molecular genetics. This information should be useful to microbiology students at both the graduate and the undergraduate lev- els. More importantly, this text should focus the attention of researchers on the importance of archaea as model systems to address fundamental biological questions. As prokaryotes, archaea can and should be used to wield the power of haploid genetics providing cost-efficient systems for scientific investigations into life. Paleobiology of the Archean SHERRY L. CADY Department of Geology Portland State University PO. Box 751 Portland, Oregon 97207-0751 I. Introduction II. Historical Review A. Main Phases of Archean Paleobiological Studies B. Reviews of Archean Paleobiology III. Evidence for Life-Microbial Biosignatures A. Bona Fide Microfossils B. Microbialities and Biogenic Stromatolites C. Chemofossils-Biomarkers and Isotopes IV. Criteria for Assessing Biogenicity V. Biogeochemical Interactions and Biosignature Formation VI. Extreme Ecosystems VII. Geological and Paleobiological History of the Archean (4000-2500 Ma) A. Oldest Dated Terrestrial Rocks and Minerals B. Oldest Types of Crustal Terrane C. Chemofossils, West Greenland D. Oldest Microfossils E. Microfossils in Hydrothermal Deposits F. Oldest Stromatolites G. Oldest Isotopic Evidence of a Specific Metabolic Pathway in Archean Evaporite Deposits H. Evidence of Hydrothermal Oil Generation during the Archean I. Oldest Compelling Chemofossil Evidence of Methanogenic Archaea J. Oxygenic Phototrophy VIII. Conclusion References I. Introduction Four billion years ago our planet began accumulating a rock record, a geological event that heralded the beginning of the Archean Eon (Fig. 1). Though the Earth itself is approximately 4550 million years old, the oldest known rocks are the 4030 million-year-old Acasta gneisses of northwestern Canada (Bowring and Williams, 1999). These rocks, and others of comparable age, indicate that the ancient Earth harbored a number of environments that could have supported life. The presence of even older minerals, 4400 million-year-old detrital zircons from the Yilgarn Craton, Western Australia (Wilde et al., ZOOl), provides evidence 3 ADVANCES IN APPLIED MICROBIOLOGY, VOLUME 50 Copyright 0 2001 by Academic Press All rights of reproduction in any form reserved. 0065.2164/01535.00 4 SHERRY L. CADY LOGIC TIME SC 2 e 3 Selected benchmarks 4 (I) 4Dinosaurextlnctloo,oldest primates 1 8 e :: +Oldesl green algae II * 4Oldesl redalgae +Sudburysstrobleme +Oldest macrofossils (Grypsmaj (I ~Oldestcarbonateplatfotms ~~IdesreucatKptlcblpmarkers ldestcyano actertal btomarkers a 4-Oldest hydrothermal mwofossils 4 Oldest microfowls, stromatol!les**, +Marflan dublofosslls(ALH84001) +Oldestchemofosslls ~Oldestdatedlerrestr~al rocks +Olde?.tdaied tef18Stl~almlneralS +Orlgin of Earth, oldest metwriteS FIG. 1. Geological time scale. Geologic time is represented here by numerically desig- nated bins of geologic time, each 100 million years long. The intervals, called geons (from GEOlogical EON), are counted from the present. The geon scale allows for Earth history (and that of other planets) to be viewed in a succession of large, simply named, equal time units, in the same way that centuries and millennia are used for familiar smaller intervals. PALEOBIOLOGY OF THE ARCHEAN 5 that the Earth was tectonically active shortly after it formed. Without plate tectonic activity commencing early and persisting throughout our planet’s history, it is unlikely that life would exist today. It is yet a mystery when life began; its origin is not revealed in the paleobiological record. Chemical fossil evidence in rocks from West Greenland indicate, however, that microbial life had evolved by 3700 Ma (mega-annum; meaning million years) (Rosing, 1999). The possibility exists that life emerged within a few hundred million years after crustal rocks began accumulating and began to leave traces in the paleobiological record. The Archean Eon, by definition, ends at precisely 2500 Ma. Fossil evidence indicates that once life emerged it evolved rapidly and occupied new ecological niches as soon as they became available (e.g., hydrothermal systems, shallow coastlines, continental seas). The Archean paleobiological record is preserved in geological units that consist primarily of chemical precipitates and volcanogenic sediments. Such deposits accumulated on the edges of accreting continental cra- tons and along the rims of protocontinents. Although only meager bits of evidence have been discovered to date, new and significant discoveries regarding Archean paleobiology and paleoecology continue to be made. In general, paleobiological information comes from a potentially wide range of fossil data known collectively as biosignatures. Evidence for the existence of the Archean biosphere is preserved in the fossil remains of microorganisms (i.e., microfossils), in the sedimentary structures mi- croorganisms helped construct (i.e., stromatolites), and in the biomarker compounds, isotopic signatures, and biominerals life leaves behind (i.e., chemofossils). Bona fide microfossils, carbonaceous microorgan- isms preserved in three dimensions, contain structural and chemical rem- nants of cellular and extracellular components (e.g., cell walls, sheathes, exopolysaccharides), which together can provide direct evi- dence for life. Also, microbially influenced fabrics and structures that form in ecosystems where authigenic minerals precipitate and rock de- tritus accumulate provide indirect evidence of microscopic life forms. Microbially influenced accretionary growth structures and fabrics in- clude nonlaminated microbialites and laminated biogenic stromatolites. Although both types of biogenic structures are found throughout the Archean, they usually lack microfossils. Chemical fossils (“chemofos- sils”), such as biomarkers and isotopic signatures, also provide indirect The geon scale complements the traditional, history-based scale with complex names and unequal geologic periods, much like dynasties in history overlap centuries. The Archean Eon is defined as that interval of time that began with the formation of the oldest geological record and that ends at 2500 Ma (mega annum; meaning million years), which is the beginning of the Proterozoic Eon. [Reproduced with permission from Hofmann (1990, 1992, 2000).] 6 SHERRYL.CADY evidence for life. Biomarker compounds consist of organic molecules highly diagnostic for their parent organisms. Elements that can be iso- topically fractionated by biological or biochemical processes include carbon, sulfur, and nitrogen. Not only have a number of types of fossil biosignatures shown that life emerged and spread globally during the early Archean, but evidence for life has been reported from all of the major Archean cratons. The pa- leobiological record has shown that life occupied several niches during the Archean and, within a few hundred million years, diversified and became metabolically sophisticated. Although fossil evidence cannot provide precise data as to when a metabolic innovation evolved, it can reveal that a particular metabolic capability existed. Chemofossil evi- dence demonstrates that many major metabolic pathways evolved dur- ing the Archean. Though the data for these evolutionary innovations are scattered throughout the ancient rock record, the continuous and relatively robust paleontological record of the Proterozoic Eon (2500 to 543 Ma) has confirmed that prior to the end of the Archean, analogues of modern microbial ecosystems, including those considered extreme, were established. Several lines of evidence suggest that the earliest microbial inhabi- tants occupied sediments and colonized newly formed minerals that precipitated around hydrothermal vents, environments characterized by high temperatures and an abundance of dissolved metal ions (Nisbet, 1995). As shown in Fig. 2 molecular phylogenetic analysis of the small-subunit ribosomal RNA of extant life indicates that hy- perthermophiles in the bacterial and archaeal domains are the closest living relatives of the hypothetical last common ancestor (Pace, 1997). Whether life originated at high temperatures (Shock and Schulte, 1998) is not known, and evidence for a hyperthermophilic ancestry has been challenged (Doolittle, 2000; Galtier et al., 1999). The possibility exists that hyperthermophiles emerged during that brief but finite period of time after the collision that presumably formed the Earth-Moon sys- tem; after the collision (-4450 to 4500 Ma), when the Earth began to cool, surface temperatures could have hovered around 100°C for 100 to 200 million years (Sleep et al., 2001). The catastrophic conditions created by large impactor events during the latter part of the heavy bombardment period (-3900 to 3800 Ma) would also have created and sustained high-temperature habitats that could have supported hy- perthermophilic communities; large impactors ( >GIOOk m in diameter) could have vaporized the ocean, while smaller impactors (>200 km in diameter) might have been able to heat the ocean above 100°C (Sleep and Zahnle, 1998). Alternatively, if life originated at lower temper- atures, and then radiated and adapted to high-temperature environ- ments, hyperthermophiles living in the subsurface portions of deep-sea PALEOBIOLOGY OF THE ARCHEAN 3ACTERIA 3 f FIG. 2. Universal phylogenetic tree based on SSU rRNA sequences. The largest formal unit of the tree consists of domains that include the Archaea, Bacteria, and Eukarya. The tree can be considered a rough map of the evolutionary distance between the organisms shown. Although the nature of the hypothetical last common ancestor is not known, hyperthermophilic and thermophilic microbial lineages are clustered around the root of the microbial domains. Constructed by comparison of 16s small-subunit ribosomal RNA sequences, the tree includes 64 rRNA sequences representative of all known phylogenetic domains. [Reproduced with permission from Pace (lggi’).] hydrothermal systems may have been the only microbial communities that could have survived the impact-induced ocean sterilizing events (Maher and Stevenson, 1988). The Earth has always been a volcanically active planet, and hydrother- mal activity prevailed after liquid water became stable at the Earth’s
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