Microbial evolution and phylogeny

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Microbial evolution and phylogeny Evolution Changes over time within the lineage of an organism that leads to the formation of novel species or to a variation within a species. 1

Evolution of life on Earth Geological und fossile evidences Million years ago 4600 Formation of planet Earth 3500 Microbial life (stromatolites) 2800 O 2 -producing photosynthesis by Cyanobacteria 2000-1800 Accumulation of O 2 in the atmosphere Early microorganisms have developed app. 3.6 to 4.0 billion years ago Metabolism ability to collect nutrients to transform them and to gain energy from it Reproduction ability to replicate own attributes and to transfer them to offsprings 2

Environmental conditions on early Earth reducing atmosphere. No oxygen (O 2 ) important compounds: H 2 O, CH 4, CO 2, N 2, NH 3, CO, H 2, H 2 S surface temperature: partly more than 100 C strong UV radiation, electric discharge Miller-(Urey) Experiment simulation of early earth conditions in the laboratory leads to the formation of biochemical relevant molecules: sugars, amino acids, purines & pyrimidines, nucleotides, thioester, fatty acids accumulation of these compounds due to a lack of biological degradation after cooling of earth: stabilisation of the organic compounds and inclusion in membrane-like structures Formation of cell-like structures 3

The Miller-Urey experiment Principle of the experiment Two main reaction chambers Water is circulating through the apparatus Lower vessel: simulation of the hot paleo-ocean Upper vessel: simulation of the paleo atmosphere: H 2, NH 3, methane and steam lightning simulated by electrodes Reaction products are led through a condensor W-formed construction: capture of water soluble reaction compounds at the bottom of the apparatus Miller-Urey experiment The products of the experiment Stanley L. Miller and his appatatus Tar 85 % div. Carbolic acids 13.0 % Glycin 1.05% Alanin 0.85% Glutamic acid traces Asparagic acid traces Valin traces Leucin traces Serin traces Prolin traces Threonin traces In 1969, a meteorite was found in Australia was showing the same composition of amino acids as the in the Miller-Urey experiment! 4

Building blocks of life in stellar dust and gas clouds? Simulation of environmental conditions in vacuum chambers (Uni Bremen) icy aluminum plate vaporization of simple chemical compounds H 2 O, CO 2, NH 4, CH 3 OH get attached radiation simulated by a strong UV-lamp formation of complex organic compounds detection with an Infrared-spectrometer After heating up of the aluminum block: Detection of Sixteen different amino acids within the icy-layers Habitability on Europa Thickness of the icy and dusty shield: more than 80 to 170 km The proposed ocean has a thickness of more than 100 km Regeneration every 10 million years (melting of the lowest layers) Gravity forces of Jupiter is dispersing the surface of Europa, meltwater is flowing upwards through cracks in the ice 5

Back to Earth Open question: How was the first organism formed? The RNA world: Possible scenario for the evolution of cellular life With time, proteins replaced the catalytic functions of RNA and DNA replaced the coding functions of RNA Self-replicating RNAs could have become cellular entities by becoming stably integrated into lipoprotein vesicles. 6

Metabolism: must have been anaerobically (no O 2 in the atmosphere) Energy yield: oxidation of organic compounds (chemoorganotrophy) oxidation of inorganic compounds (chemolithotrophy) (driven by light phototrophy) Metabolic pathway must have been simple e.g. formation of iron sulfide FeCO 3 + 2 H 2 S FeS 2 + H 2 + H 2 O + CO 2 FeS + H 2 S FeS 2 + H 2 only a few enzymes nessecary! Fossile evidences for microbial life Cyanobacteriea from the Precambrian (app. 3.5 billion years old), oldest known fossiles fossile Cyanobacterium from North-Australia (app. 1 billion years old) actual living Cyanobacterium (Oscillatoria) 7

Stromatolites Cyanobacteria can form Stromatolites Laminated structure, embeddind in sediments; Bacteria produce calcium carbonates Thin-sections show fossile cyanobacteria and algae Phylogeny: Classification of species in superior taxa and construction of phylogenetic trees based on evolutionary relationships. 8

Endosymbiotic theory: Proteobacteria Mitochondria Cyanobacteria Chloroplasts Novel theory: There was not the common ancestor Life has evolved out of multiple ancestoral cells. Some have prevailed to become ancestors of Bacteria, Archaea and Eukarya. Horizontal gene transfer between organisms (even from different domains) might have played an important role evolution. Darwinian threshold in the beginning: Horizontal gene transfer (open systems of cells) afterwards: Etablishment of cell compartments (Horizontal gene transfer less important) 9

Variety of ancestoral cells Horizontal gene transfer between organisms How many different bacteria do we expect? Validly described species: 5 000Prokaryotes (Bacteria und Archaea) 1 700 000Eukaryotes Estimations for different bacterial species in 30 g forrest soil The big debate: What is a species??? 3 000 (Torsvik et al., 1990) 500 000 (Dykhuizen 1998) (based on the same data set) 10

How to classify a microbe? Microbial morphology is limited only a weak hint to determine microbial affiliation 11

Identification of a microbe by classical microbiological methods Isolation from mammal gram negative gram staining gram positive rod shaped fakultative aerob obligate aerob not rod shaped fermentation of lactose, production of acid and gas no fermentation of lactose further metabolic tests Identification as Escherichia coli Hierarchical structure in taxonomy Bacteria Proteobacteria Gammaproteobacteria Enterobacteriales Enterobacteriaceae Escherichia Escherichia coli Escherichia coli K12 domain phylum class order family genus species strain 12

Phylogenetic overview on the bacterial domain Aquifex-Hydrogenobacter group hyperthermophile (opt. >80 C), chemolithotroph, Aquifex probably most similar to bacterial ancestor Thermotoga hyperthermophile, chemoorganotroph Green non sulfur bacteria (GNSB), Chloroflexi partly phototroph, thermophile (opt. 45-80 C), chemoorganotroph Deinococcus group partly radiation resistant (UV- and gamma ray) (D.radiodurans extremly effective DNA repair mechanisms), partly thermophile 13

Phylogenetic overview on the bacterial domain Spirochetes conspicious morphology, special apparatus of movement, partly pathogen Gree sulfur bacteria strictly anaerobic, obligat phototroph, can utilise simple organic compounds, if there are reduced sulfur compounds available Cytophaga Flavobacteria Bacteroidetes (CFB) aerobic and anaerobic, polymer degrader some show gliding movement Planctomyces reproduction by budding, no peptidoglycan aerobic, mainly aquatic 14

Phylogenetic overview on the bacterial domain Chlamydia obligate intracellular parasites, many pathogens Cyanobacteria oxygenic phototrophs Gram positives (Firmicutes) big heterogeneous group divided into two subgroups high GC (Actinobacteria) and low GC gram positives Proteobacteria biggest group, pysiologically diverse five subgroups (alpha, beta, gamma, delta, epsilon) 15

Molecular techniques Tree of life: Bacterial domain Green non-sulfur OP5 Planctomycetes WS1 Actinobacteria OP10 OP9 Dictyglomus Coprothermobacter Thermotogales Thermodesulfobacterium Aquificales OP3 Verrucomicrobia Chlamydia OS-K Nitrospira Acidobacterium OP8 Termite group I Proteobacteria Synergistes Flexistipes Cyanobacteria Fusobacteria Low G+C gram positive TM7 Fibrobacter Marine group A Green sulfur Thermus/Deinococcus TM6 WS6 Spirochetes Approximately 1/3 of bacterial phyla contains almost exclusively uncultured bacteria!!! Cytophagales OP11 Hugenholtz et al. 1997 Archaea 0,10 16

Analysis of ribosomal nucleic acids Ribosomes are cellular maschines for the construction of proteins and enzymes small subunit large subunit present in all living organisms high copy number up to 20.000 ribosomes per cell side view Ribosome (eucaryotes) front view The ribosomal RNA is the backbone of the ribosome sufficient number of nucleotides for phylogenetic analyses 16S rrna: app. 1.500 bp Ribosomal RNA for phylogenetic analyses Due to the essential function of ribosomal nucleic acids: Mutation is often lethal Independent (constant) pressure of selection Highly conserved at many positions Comparison of analogous, but variable sequences Almost no gene transfer Changes of sequences happen with a constant speed, but slowly enough to mirror the whole time of bacterial evolution (Carl Woese, 1987) The evolution of the molecule mirrors the evolution of its host ( molecular clock ) 17

The prokaryotic 16S rrna The molecular clock V6 V7 shows a different speed in some areas of the V5 V8 rrna. 5 Mutations in highly conserved regions happened evolutionary at earlier stages than in variable regions. V3 V1 V2 absolutely conserved highly variable E. coli, but not in > 75% of all bacteria 3 V9 Yves Van de Peer (1996), modifiied The 16S rrna as a molecular clock of evolution The investigation of phylogenetic relationships according to rrna-sequences by Woese & Fox (1977) finally led to the classification of all organisms into the domains: Bacteria, Archaea and Eukarya (Woese, 1990). 18

Alignment of 16S rrna sequences 16S rrnas in the database Currently 1 074 075 sequences Aug 31, 2009 19

Is it enough to define a species? DNA DNA hybridization 20

Results and interpretation The species level Application of molecular probes Hybridization Probe (Oligonucleotide) at a target sequence (mostly 16S rrna) Specificity Strain, family,... up to the domain (dependent on target sequence) Most important technique Fluorescence-In-Situ-Hybridization, FISH with fixed cells (binding at ribosomes) signal enhancement by higher ribosome content or enzymatic amplification (CARD-FISH) 21

Specific detection microorganisms Fluorescence In-situ Hybridisation, FISH: Cells fixed on filter Microbial community Hybridisation: Probe binds at a target sequence (mostly 16S rrna) Signal enhancement by higher ribosome content Specific probe Fluorescent dye Specificity: Strain, family,... up to domain 16S rrna Quantification: Non specific vs. specific signals DAPI Probe Analysis of bacterial communities by Fluorescence-In-Situ-Hybridization, FISH Coupling of molecular probes with fluorescent dyes Annealing at speciffic regions of the rrna Staining of cells on different phylogenetic levels Detection under a microscopic slide (in situ) Photo: Jiri Snaidr 22

Anaerobic methane oxidsing consortia ANME2 (EelMS932) Desulfosarcina (DSS658) DAPI CARD-FISH 5 µm Boetius, et al. (2000) Nature. 407:623-626 detected in gas hydrate bearing sediments 5 µm detected in tidal flat sediments Archaea (ARCH915) Desulfosarcina (DSS658) Stronghold of Fluorescence-In-Situ-Hybridization is the MPI in Bremen! Questions: Is there a 16S rdna? Why do we prefer to analyse DNA? When do we analyse RNA? How can we analyse strains below the species level? What will future bring? 23