Worldtraveller
Veteran Member
I have to say, reading through all this makes me wish I'd paid more attention to my chemistry classes.
... and, of course:So prokaryotedom has a big world of energy metabolism beyond heterotrophy and oxygenic photosynthesis. This is the missing piece of the puzzle, because it enables organisms to be autotrophic without needing to photosynthesize. Indeed, the authors of that recent Nature conclude that the LUCA was an autotroph, making all its biological molecules as a plant does.
As an illustration, I note Bacterial Manganese Reduction and Growth with Manganese Oxide as the Sole Electron Acceptor. That was discovered for Alteromonas putrefaciens MR-1, isolated from lake-bottom sediments. This organism can use a variety of other electron acceptors if they are available: O2, NO3-, NO2-, Fe+++, S2O3--, SO3--, S4O6--, MnO2, glycine, fumarate, trimethylamine-N-oxide. However, it does not use SO4--, MoO4--, CO2.
Now for some troph terminology.
- Autotrophy - making all one's biological molecules.
- Heterotrophy - needing to consume some biological molecules.
- Lithotrophy - living off of inorganic molecules.
- Organotrophy - living off of organic molecules.
- Chemotrophy - getting one's energy from chemical reactions.
- Phototrophy - getting one's energy from light.
- Mixotrophy - mixtures of various modes: auto- and hetero-, litho- and organo-, chemo- and photo-.
Hot volcanic vents promote the thermal fixation of atmospheric N2 into biologically available forms. The importance of this process for the global nitrogen cycle is poorly understood. At Masaya volcano, Nicaragua, NO and NO2 are intimately associated with volcanic aerosol, such that NOx levels reach as much as an order of magnitude above local background. In-plume HNO3 concentrations are elevated above background to an even greater extent (≤50 μmol·m^(−3)). We estimate the production efficiency of fixed nitrogen at hot vents to be ∼3 × 10^(−8) mol·J^(−1), implying present-day global production of ∼10^(9) mol of fixed N per year. Although conversion efficiency would have been lower in a preoxygenated atmosphere, we suggest that subaerial volcanoes potentially constituted an important source of fixed nitrogen in the early Earth, producing as much as ∼10^(11) mol·yr^(−1) of fixed N during major episodes of volcanism. These fluxes are comparable to estimated nitrogen-fixation rates in the prebiotic Earth from other major sources such as bolide impacts and thunderstorm and volcanic lightning.
So the LUCA could use O2, NO3-, SO4--, and S as electron acceptors. At least if the enzymes for doing so had not spread by lateral gene transfer.Sequences in current databases show that a number of proteins involved in respiratory processes are homologous in archaeal and bacterial species. In particular, terminal oxidases belonging to oxygen, nitrate, sulfate, and sulfur respiratory pathways have been sequenced in members of both domains. They include cytochrome oxidase, nitrate reductase, adenylylsulfate reductase, sulfite reductase, and polysulfide reductase.
So our ancestors breathed nitrogen oxides before they breathed oxygen.The heme–copper oxidases (HCOs) catalyze the reduction of O2 to water, and couple the free energy to proton pumping across the membrane. HCOs are divided into three sub-classes, A, B and C, whose order of emergence in evolution has been controversial. Here we have analyzed recent structural and functional data on HCOs and their homologues, the nitric oxide reductases (NORs). We suggest that the C-type oxidases are ancient enzymes that emerged from the NORs. In contrast, the A-type oxidases are the most advanced from both structural and functional viewpoints, which we interpret as evidence for having evolved later.
I have to say, reading through all this makes me wish I'd paid more attention to my chemistry classes.
Meaning that a lot of electron-transfer metabolism is pre-LUCA.Genome analyses and the resolution of three-dimensional structures have provided evidence in recent years for hitherto unexpected family relationships between redox proteins of very diverse enzymes involved in bioenergetic electron transport. Many of these enzymes appear in fact to be constructed from only a limited set of building blocks. Phylogenetic analysis of selected units from this "redox enzyme construction kit" indicates an origin for several prominent bioenergetic enzymes that is very early, lying before the divergence of Bacteria and Archaea. Possible scenarios for the early evolution of selected complexes are proposed based on the obtained tree topologies.
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With the possible exception of photosynthesis and methanogenesis, which have so far only been found in Bacteria and Archaea, respectively, all major energy-conserving electron transport chains are operative in both prokaryotic kingdoms (Castresana & Moreira 1999). Phylogenetic analyses of constituent enzymes in most cases argue against lateral gene transfer of these mechanisms between kingdoms—a notable exception being sulphate reduction where evidence for inter-kingdom lateral transfer has been reported (Klein et al. 2001).
These genes were acquired by the ancestor of Haloarchaea, and in the process, that ancestor lost methanogenesis, and its metabolism changed from anaerobic and autotrophic to aerobic and heterotrophic.The 1,089 acquisitions include genes for catabolic carbon metabolism, membrane transporters, menaquinone biosynthesis, and complexes I–IV of the eubacterial respiratory chain that functions in the haloarchaeal membrane consisting of diphytanyl isoprene ether lipids. LGT on a massive scale transformed a strictly anaerobic, chemolithoautotrophic methanogen into the heterotrophic, oxygen-respiring, and bacteriorhodopsin-photosynthetic haloarchaeal common ancestor.
We propose that RNA is well suited for a world evolving at acidic pH. This is supported by the enhanced stability at acidic pH of not only the RNA phosphodiester bond but also of the aminoacyl-(t)RNA and peptide bonds. Examples of in vitro-selected ribozymes with activities at acid pH have recently been documented. The subsequent transition to a DNA genome could have been partly driven by the gradual rise in ocean pH, since DNA has greater stability than RNA at alkaline pH, but not at acidic pH.
The discovery of numerous riboswitch classes reveals that many of these RNA structures regulate gene expression in response to the selective binding of coenzymes and signaling molecules derived from RNA monomers or their precursors. It has been proposed that many coenzymes might be of ancient origin, based on their universal distribution in biology and their RNA-like chemical composition. In this Review, which includes four figures and 103 references, we discuss the findings that support the hypothesis that common RNA-derived signaling compounds are ancient and speculate on the possible complexity of the chemical language that might have been used by life-forms long before proteins emerged.
We present a molecular-level model for the origin and evolution of the translation system, using a 3D comparative method. In this model, the ribosome evolved by accretion, recursively adding expansion segments, iteratively growing, subsuming, and freezing the rRNA. Functions of expansion segments in the ancestral ribosome are assigned by correspondence with their functions in the extant ribosome. The model explains the evolution of the large ribosomal subunit, the small ribosomal subunit, tRNA, and mRNA. Prokaryotic ribosomes evolved in six phases, sequentially acquiring capabilities for RNA folding, catalysis, subunit association, correlated evolution, decoding, energy-driven translocation, and surface proteinization. Two additional phases exclusive to eukaryotes led to tentacle-like rRNA expansions. In this model, ribosomal proteinization was a driving force for the broad adoption of proteins in other biological processes. The exit tunnel was clearly a central theme of all phases of ribosomal evolution and was continuously extended and rigidified. In the primitive noncoding ribosome, proto-mRNA and the small ribosomal subunit acted as cofactors, positioning the activated ends of tRNAs within the peptidyl transferase center. This association linked the evolution of the large and small ribosomal subunits, proto-mRNA, and tRNA.
Interestingly, considering a metal-catalysed origin of metabolism gives rise to an attractive hypothesis about how the first enzymes could have formed: simple RNA or (poly)peptide molecules could have bound the metal ions, and thus increased their solubility, concentration and accessibility. In a second step, this would have allowed substrate specificity to evolve.
Not just the Earth, but also elsewhere in the Universe, like early Mars and the interiors of he larger icy moons of the outer planets.The synthesis of amino acids in the Miller-Urey spark-discharge experiments in the early 1950s inspired a strong interest in experimental studies of prebiotic organic chemistry that continues today. Over the years, many of the basic building blocks of life as we know it have been synthesized in the laboratory from simple ingredients, including amino acids, sugars, nucleobases, and membrane-forming lipids. Questions remain, however, concerning whether the conditions that allow synthesis of these compounds in the laboratory accurately simulate those that might have been present on the early Earth, and a closer convergence between plausible prebiotic conditions and laboratory simulations remains a challenge for experimentalists.
So hydrothermal vents are good places for prebiotic synthesis.Organic compounds which are obviously synthesized from inorganic precursors (e.g., CO) by hydrothermal activity are currently a research topic in prebiotic chemistry leading to the origin of life. However, such de novo products would be overwhelmed in present Earth environments, by an excess of thermal alteration (pyrolysis) products formed from contemporary life (e.g., hydrocarbons, alkanoic acids, etc.). Thus, organic syntheses must be demonstrated and distinguished from organic matter alteration initially in the laboratory and then in the field. Organic synthesis under hydrothermal conditions is theoretically possible and various established industrial processes are used to synthesize organic compounds from inorganic substrates with the aid of catalysts. A set of Strecker-type synthesis experiments has been carried out under hydrothermal conditions (150 °C), producing various amino acids. The formation of lipid compounds during an aqueous organic synthesis (Fischer–Tropsch-type) reaction was reported, using solutions of oxalic acid (also formic acid) as the carbon and hydrogen sources, and heating at discrete temperatures (50° intervals) from 100 to 400 °C. The maximum lipid yield, especially for oxygenated compounds was in the window of 150–250 °C. The compounds range from C6 to >C33, including n-alkanols, n-alkanoic acids, n-alkyl formates, n-alkanones, and n-alkanes, all with no carbon number preferences. These lipid compounds, especially the acids, can form lipid bilayers or micelles, potential precursors for membranes. Reductive condensation (i.e., dehydration) reactions also occur under simulated hydrothermal conditions and form amide, nitrile and ester bonds. The chemistry and kinetics of the condensation reactions are under further study and have the potential for oligomerization of acid-amides in aqueous medium. Abiotic organic compounds are not biomarkers per se because they do not originate from biosynthesis. Thus, they should be regarded as a distinctly separate group, termed prebiotic or synthetic organic compounds, in explorations for evidence of life.
Ferrous iron: Fe++ or Fe II.The action of an electric discharge on reduced gas mixtures such as H2O, CH4 and NH3 (or N2) results in the production of several biologically important organic compounds including amino acids. However, it is now generally held that the early Earth’s atmosphere was likely not reducing, but was dominated by N2 and CO2. The synthesis of organic compounds by the action of electric discharges on neutral gas mixtures has been shown to be much less efficient. We show here that contrary to previous reports, significant amounts of amino acids are produced from neutral gas mixtures. The low yields previously reported appear to be the outcome of oxidation of the organic compounds during hydrolytic workup by nitrite and nitrate produced in the reactions. The yield of amino acids is greatly increased when oxidation inhibitors, such as ferrous iron, are added prior to hydrolysis. Organic synthesis from neutral atmospheres may have depended on the oceanic availability of oxidation inhibitors as well as on the nature of the primitive atmosphere itself. The results reported here suggest that endogenous synthesis from neutral atmospheres may be more important than previously thought.
Here is the Citric acid cycle. Biochemists often like to use -ate instead of -ic acid in the names of acids. Thus, acetate instead of acetic acid.
That's a reasonable position to take in the context of biochemistry, which mostly occurs in highly impure aqueous solutions where multiple anions (and cations) are present. When the cation is the important group, as is invariably the case when discussing acids (H+ being the most common and least interesting of the possible anions in an acid solution, by definition), and several anions are present in solution (most biological contexts have plenty of K+, Na+ and often Mg2+ and Ca2+ present as well as the ubiquitous H+), there is no good reason to specify the anion, and the use of the '-ic acid' suffix might be taken as implying that it is specifically and exclusively H+.
Biochemists and organic chemists have a habit of ignoring H+ ions, and even covalently bonded H, as it is just assumed to be there by default if no other group or anion is specified.
LUCApediaKEGG (Kyoto Encyclopedia of Genes and Genomes) is a database resource that integrates genomic, chemical and systemic functional information. In particular, gene catalogs from completely sequenced genomes are linked to higher-level systemic functions of the cell, the organism and the ecosystem.
eQuilibrator: The Biochemical Thermodynamics CalculatorLUCApedia is a unified framework containing multiple datasets related to the Last Universal Common Ancestor (LUCA) and its predecessors. The database can be searched by protein name or Uniprot ID. Text and MySQL datafiles are also available on the download page.
Iron-sulfur groups likely go back to the origin of life, while copper use likely only goes back to the presence of atmospheric oxygen, starting around 2.5 billion years ago.An evolutionary tree of key enzymes from the Complex-Iron-Sulfur-Molybdoenzyme (CISM) superfamily distinguishes “ancient” members, i.e. enzymes present already in the last universal common ancestor (LUCA) of prokaryotes, from more recently evolved subfamilies. The majority of the presented subfamilies and, as a consequence, the Molybdo-enzyme superfamily as a whole, appear to have existed in LUCA. The results are discussed with respect to the nature of bioenergetic substrates available to early life and to problems arising from the low solubility of molybdenum under conditions of the primordial Earth.
CISM = Complex-Iron-Sulfur-MolybdoenzymeWhat then of the availability of these two transition metals? W occurs in both acid and alkaline solutions and was thus available to emerging life, whereas Mo is relatively insoluble in reduced and neutral waters, but does occur in mixed valence sulfide and selenide and/or oxide complexes in alkaline solutions. Mo's insolubility at neutral pH values, exacerbated by an anoxic atmosphere, suggested a low bioavailability of this element for early life. Mo-isotope analyses on samples from the Archaean era indeed show substantially lower levels than during Phanerozoic times. Two scenarios can reconcile the results of molecular phylogeny and paleogeochemistry. (i) The ancestral CISM enzyme exclusively used W which was later replaced by Mo. (ii) CISM-catalyzed reactions in early life used Mo supplied by alkaline hydrothermal vents, proposed as cradles for life. The exclusiveness for Mo of many CISM-members as well as findings that primary productivity involving Mo has been comparable to the present since the geological record began at 3.8 Ga lead us to favor the second scenario.
https://www.nature.com/articles/s41467-021-21218-z said:Water radiolysis continuously produces H2 and oxidized chemicals in wet sediment and rock. Radiolytic H2 has been identified as the primary electron donor (food) for microorganisms in continental aquifers kilometers below Earth’s surface. Radiolytic products may also be significant for sustaining life in subseafloor sediment and subsurface environments of other planets. However, the extent to which most subsurface ecosystems rely on radiolytic products has been poorly constrained, due to incomplete understanding of radiolytic chemical yields in natural environments. Here we show that all common marine sediment types catalyse radiolytic H2 production, amplifying yields by up to 27X relative to pure water. In electron equivalents, the global rate of radiolytic H2 production in marine sediment appears to be 1-2% of the global organic flux to the seafloor. However, most organic matter is consumed at or near the seafloor, whereas radiolytic H2 is produced at all sediment depths. Comparison of radiolytic H2 consumption rates to organic oxidation rates suggests that water radiolysis is the principal source of biologically accessible energy for microbial communities in marine sediment older than a few million years. Where water permeates similarly catalytic material on other worlds, life may also be sustained by water radiolysis.