15 Combinatorial chemistry in the prebiotic environment

The pathway leading to the origin of life presumably included a process by which polymers were synthesized abiotically from simpler compounds on the early Earth, then encapsulated to form protocells. Previous studies have reported that mineral surfaces can concentrate and organize activated mononucleotides, thereby promoting their polymerization into RNA-like molecules. However, a plausible prebiotic activation mechanism has not been established, and minerals cannot form cellular compartments. We are exploring ways in which nonactivated mononucleotides can undergo polymerization and encapsulation. We found that small yields of RNA-like molecules are synthesized by a condensation reaction when mixtures of amphiphilic lipids and mononucleotides are exposed to cycles of dehydration and rehydration. The lipids concentrate and organize the monomers within multilamellar liquid-crystalline matrices that self-assemble in the dry state. The chemical potential driving the polymerization reaction is supplied by the anhydrous conditions in which water becomes a leaving group, with heat providing activation energy. Significantly, the polymeric products are encapsulated in trillions of microscopic compartments upon rehydration. Each compartment is unique in its composition and contents, and can be considered to be an experiment in a natural version of combinatorial chemistry that would be ubiquitous in the prebiotic environment. A successful experiment would be a compartment that captured polymers capable of catalyzing their own replication. If this can be reproduced in the laboratory, it would represent a significant step toward understanding the origin of cellular life.     

Prebiotic phosphate: a problem insoluble in water ? ]

It is well-known that in water phosphate readily reacts with calcium, precipitating as insoluble apatite. How phosphorus could have been available for prebiotic reactions is still an open problem. We suggest that phosphorus-containing compounds might have accumulated in a hydrophobic medium, since the absence of calcium ions would have prevented them from precipitating as apatite. Hydrophobic compounds may have been synthesized on the early Earth through the polymerization of methane or through Fischer-Tropsch-type reactions. Moreover, hydrophobic compounds would have been delivered to the early Earth by extraterrestrial infall. In previous articles (Morchio and Traverso [1999], Morchio et al. [2001]) we suggested that such hydrophobic material would have formed a hydrophobic layer on the surface of the sea, which would have provided an environment thermodynamically more suitable than water for the concentration and polymerization of organic molecules fundamental to life, particularly amino acids and (pyrimidine) bases. It may be hypothesized that elemental phosphorus or phosphorus-containing compounds (such as phosphite) deriving from volcanic eruptions would have ended up raining down into the hydrophobic layer, accumulating due to the absence of calcium ions, in an environment protected against hydrolysis. Phosphorus-containing compounds might have interacted with hydrophobic molecules in the layer giving rise to polymers. In particular, phosphite might have reacted with the hydrophobic amino acids, giving rise to phosphoamino acids, which, in turn, might have interacted with pyrimidine bases (relatively abundant in the layer) giving rise to peptides and oligonucleotide-like polymers. Indeed, it has been experimentally shown (Zhou et al. [1996]) that, in an anhydrous organic medium (pyridine), dialkilphosphite reacts with amino acids to form phosphoamino acids, which interact with pyrimidine nucleosides to give nucleotides, short oligonucleotides and phosphoryl peptides.     

Self-assembly processes in the prebiotic environment

An important question guiding research on the origin of life concerns the environmental conditions where molecular systems with the properties of life first appeared on the early Earth. An appropriate site would require liquid water, a source of organic compounds, a source of energy to drive polymerization reactions and a process by which the compounds were sufficiently concentrated to undergo physical and chemical interactions. One such site is a geothermal setting, in which organic compounds interact with mineral surfaces to promote self-assembly and polymerization reactions. Here, we report an initial study of two geothermal sites where mixtures of representative organic solutes (amino acids, nucleobases, a fatty acid and glycerol) and phosphate were mixed with high-temperature water in clay-lined pools. Most of the added organics and phosphate were removed from solution with half-times measured in minutes to a few hours. Analysis of the clay, primarily smectite and kaolin, showed that the organics were adsorbed to the mineral surfaces at the acidic pH of the pools, but could subsequently be released in basic solutions. These results help to constrain the range of possible environments for the origin of life. A site conducive to self-assembly of organic solutes would be an aqueous environment relatively low in ionic solutes, at an intermediate temperature range and neutral pH ranges, in which cyclic concentration of the solutes can occur by transient dry intervals.     

The Lipid World

The continuity of abiotically formed bilayer membraneswith similar structures in contemporary cellular life,and the requirement for microenvironments in whichlarge and small molecules could be compartmentalized, support the idea that amphiphilic boundary structurescontributed to the emergence of life. As an extensionof this notion, we propose here a `Lipid World'scenario as an early evolutionary step in theemergence of cellular life on Earth. This conceptcombines the potential chemical activities of lipidsand other amphiphiles, with their capacity to undergospontaneous self-organization into supramolecularstructures such as micelles and bilayers. Inparticular, the documented chemical rate enhancementswithin lipid assemblies suggest that energy-dependentsynthetic reactions could lead to the growth andincreased abundance of certain amphiphilic assemblies.We further propose that selective processes might acton such assemblies, as suggested by our computersimulations of mutual catalysis among amphiphiles. Asdemonstrated also by other researchers, such mutualcatalysis within random molecular assemblies couldhave led to a primordial homeostatic system displayingrudimentary life-like properties. Taken together,these concepts provide a theoretical framework, andsuggest experimental tests for a Lipid World model forthe origin of life.     

Arginine cofactors on the polymerase ribozyme

The RNA world hypothesis states that the early evolution of life went through a stage in which RNA served both as genome and as catalyst. The central catalyst in an RNA world organism would have been a ribozyme that catalyzed RNA polymerization to facilitate self-replication. An RNA polymerase ribozyme was developed previously in the lab but it is not efficient enough for self-replication. The factor that limits its polymerization efficiency is its weak sequence-independent binding of the primer/template substrate. Here we tested whether RNA polymerization could be improved by a cationic arginine cofactor, to improve the interaction with the substrate. In an RNA world, amino acid-nucleic acid conjugates could have facilitated the emergence of the translation apparatus and the transition to an RNP world. We chose the amino acid arginine for our study because this is the amino acid most adept to interact with RNA. An arginine cofactor was positioned at ten different sites on the ribozyme, using conjugates of arginine with short DNA or RNA oligonucleotides. However, polymerization efficiency was not increased in any of the ten positions. In five of the ten positions the arginine reduced or modulated polymerization efficiency, which gives insight into the substrate-binding site on the ribozyme. These results suggest that the existing polymerase ribozyme is not well suited to using an arginine cofactor.     

Prebiotic chemistry in clouds

Summary In the traditional concept for the origin of life as proposed by Oparin and Haldane in the 1920s, prebiotic reactants became slowly concentrated in the primordial oceans and life evolved slowly from a series of highly protracted chemical reactions during the first billion years of Earth's history. However, chemical evolution may not have occurred continuously because planetesimals and asterioids impacted the Earth many times during the first billion years, may have sterilized the Earth, and required the process to start over. A rapid process of chemical evolution may have been required in order that life appeared at or before 3.5 billion years ago. Thus, a setting favoring rapid chemical evolution may be required. A chemical evolution hypothesis set forth by Woese in 1979 accomplished prebiotic reactions rapidly in droplets in giant atmospheric reflux columns. However, in 1985 Scherer raised a number of objections to Woese's hypothesis and concluded that it was not valid. We propose a mechanism for prebiotic chemistry in clouds that satisfies Scherer's concerns regarding the Woese hypothesis and includes advantageous droplet chemistry.Prebiotic reactants were supplied to the atmosphere by comets, meteorites, and interplanetary dust or synthesized in the atmosphere from simple compounds using energy sources such as ultraviolet light, corona discharge, or lightning. These prebiotic monomers would have first encountered moisture in cloud drops and precipitation. We propose that rapid prebiotic chemical evolution was facilitated on the primordial Earth by cycles of condensation and evaporation of cloud drops containing clay condensation nuclei and nonvolatile monomers. For example, amino acids supplied by, or synthesized during entry of, meteorites, comets, and interplanetary dust would have been scavenged by cloud drops containing clay condensation nuclei. Polymerization would have occurred within cloud systems during cycles of condensation, freezing, melting, and evaporation of cloud drops. We suggest that polymerization reactions occurred in the atmosphere as in the Woese hypothesis, but life originated in the ocean as in the Oparin-Haldane hypothesis. The rapidity with which chemical evolution could have occurred within clouds accommodates the time constraints suggested by recent astrophysical theories.     

Signature of a Primitive Genetic Code in Ancient Protein Lineages

The genetic code is the syntactic foundation underlying the structure and function of every protein in the history of the biological world. Its highly ordered degenerate complexity suggests an incremental evolution, the result of a combination of selective, mechanistic, and random processes. These evolutionary processes are still poorly understood and remain an open question in the study of early life on Earth. We perform a compositional analysis of ribosomal proteins and ATPase subunits in bacterial and archaeal lineages, using conserved positions that came and remained under purifying selection before and up to the most recent common ancestor. An observable shift in amino acid usage at these conserved positions likely provides an untapped window into the history of protein sequence space, allowing events of genetic code expansion to be identified. We identify Cys, Glu, Phe, Ile, Lys, Val, Trp, and Tyr as recent additions to the genetic code, with Asn, Gln, Gly, and Leu among the more ancient. Our observations are consistent with a scenario in which genetic code expansion primarily favored amino acids that promoted an increase in polypeptide size and functionality. We propose that this expansion would have been critical in the takeover of many RNA-mediated processes, as well as the addition of novel biological functions inaccessible to an RNA-based physiology, such as crossing lipid membranes. Thus, expansion of the genetic code likely set the stage for the transition from RNA-based to protein-based life. Electronic supplementary material The online version of this article (doi:) contains supplementary material, which is available to authorized users.     

Preparation and characterization of long chain amino acid and peptide vesicle membranes

Four amino acid dicarboxylic amphiphiles which contain cysteine or homocysteine were synthesized. Each forms synthetic bilayer membranes upon hydration. Extensive sonication above the lipid phase transition temperature, 61 to 82 degrees C, produced 1000 A diameter vesicles. Treatment of the vesicles with water-soluble carbodiimides during and after sonication induced oligopeptide formation at the vesicle surface with retention of vesicle size and shape. Size exclusion chromatography indicates the products are predominantly di- to decapeptides. The permeability characteristics of the amino acid and peptide vesicles to [3H]glucose and 6-carboxyfluorescein are reported. The amino acid vesicles are among the least permeable nonpolymerized bilayer vesicles described in the literature to date. Formation of the peptide vesicles increases the membrane permeability, whereas in other polymerizable lipid vesicles the permeability decreases upon polymerization. The amino acid vesicles can be immobilized on Sephadex beads by reaction with carbodiimide. The impermeability, biodegradability, and ease of immobilization make this class of vesicles attractive materials for the encapsulation of reagents.     

Chiral Polymerization in Open Systems From Chiral-Selective Reaction Rates

We investigate the possibility that prebiotic homochirality can be achieved exclusively through chiral-selective reaction rate parameters without any other explicit mechanism for chiral bias. Specifically, we examine an open network of polymerization reactions, where the reaction rates can have chiral-selective values. The reactions are neither autocatalytic nor do they contain explicit enantiomeric cross-inhibition terms. We are thus investigating how rare a set of chiral-selective reaction rates needs to be in order to generate a reasonable amount of chiral bias. We quantify our results adopting a statistical approach: varying both the mean value and the rms dispersion of the relevant reaction rates, we show that moderate to high levels of chiral excess can be achieved with fairly small chiral bias, below 10%. Considering the various unknowns related to prebiotic chemical networks in early Earth and the dependence of reaction rates to environmental properties such as temperature and pressure variations, we argue that homochirality could have been achieved from moderate amounts of chiral selectivity in the reaction rates.     

Permeability of membranes to amino acids and modified amino acids: Mechanisms involved in translocation

Summary The amino acid permeability of membranes is of interest because they are one of the key solutes involved in cell function. Membrane permeability coefficients (P) for amino acid classes, including neutral, polar, hydrophobic, and charged species, have been measured and compared using a variety of techniques. Decreasing lipid chain length increased permeability slightly (5-fold), while variations in pH had only minor effects on the permeability coefficients of the amino acids tested in liposomes. Increasing the membrane surface charge increased the permeability of amino acids of the opposite charge, while increasing the cholesterol content decreased membrane permeability. The permeability coefficients for most amino acids tested were surprisingly similar to those previously measured for monovalent cations such as sodium and potassium (approximately 10^–12–10^–13 cm · s^–1). This observation suggests that the permeation rates for the neutral, polar and charged amino acids are controlled by bilayer fluctuations and transient defects, rather than partition coefficients and Born energy barriers. Hydrophobic amino acids were 10² more permeable than the hydrophilic forms, reflecting their increased partition coefficient values.External pH had dramatic effects on the permeation rates for the modified amino acid lysine methyl ester in response to transmembrane pH gradients. It was established that lysine methyl ester and other modified short peptides permeate rapidly (P = 10^–2 cm · s^–1) as neutral (deprotonated) molecules. It was also shown that charge distributions dramatically alter permeation rates for modified di-peptides. These results may relate to the movement of peptides through membranes during protein translocation and to the origin of cellular membrane transport on the early Earth.Abbreviations DCP dicetylphosphate - DMPC dimyristoyl phosphatidylcholine - EPC egg phosphatidylcholine - LUV large unilamellar vesicle - MLV multilamellar vesicle - PLM planar lipid membrane - SUV small unilamellar vesicle - pH transmembrane pH gradient     

Trimetaphosphate Activates Prebiotic Peptide Synthesis across a Wide Range of Temperature and pH

The biochemical activation of amino acids by adenosine triphosphate (ATP) drives the synthesis of proteins that are essential for all life. On the early Earth, before the emergence of cellular life, the chemical condensation of amino acids to form prebiotic peptides or proteins may have been activated by inorganic polyphosphates, such as tri metaphosphate (TP). Plausible volcanic and other potential sources of TP are known, and TP readily activates amino acids for peptide synthesis. But de novo peptide synthesis also depends on pH, temperature, and processes of solvent drying, which together define a varied range of potential activating conditions. Although we cannot replay the tape of life on Earth, we can examine how activator, temperature, acidity and other conditions may have collectively shaped its prebiotic evolution. Here, reactions of two simple amino acids, glycine and alanine, were tested, with or without TP, over a wide range of temperature (0–100 °C) and acidity (pH 1–12), while open to the atmosphere. After 24 h, products were analyzed by HPLC and mass spectrometry. In the absence of TP, glycine and alanine readily formed peptides under harsh near-boiling temperatures, extremes of pH, and within dry solid residues. In the presence of TP, however, peptides arose over a much wider range of conditions, including ambient temperature, neutral pH, and in water. These results show how polyphosphates such as TP may have enabled the transition of peptide synthesis from harsh to mild early Earth environments, setting the stage for the emergence of more complex prebiotic chemistries.     

Chemical Evolution and Meteorites: An Update

Carbonaceous chondrites are a primitive group of meteorites, which contain abundant organic material and provide a unique natural record of prebiotic chemical evolution. This material comprises a varied suite of soluble organic compounds that are similar, sometimes identical, to those found in the biosphere, such as amino acids, carboxylic acids, and sugar derivatives. Some amino acids of this suite also show L-enantiomeric excesses, and suggest the possibility they may have contributed to terrestrial homochirality by direct input of meteoritic material to the early Earth. This optical activity appears to be limited to the subgroup of alpha-methyl amino acids which, although not common in the extant biosphere, would have been well suited to provide the early earth with both enantiomeric excesses and means for their amplification by subsequent chemical evolution. We can also envision this exogenous delivery of carbonaceous material by meteorites and comets as having coincided with the endogenous formation of prebiotic precursors and influenced their evolution by complementary reactions or catalysis.     

Products of the reaction of HOCl with tryptophan protect LDL from atherogenic modification

Hypochlorite (HOCl) attacks amino acid residues in LDL making the particle atherogenic. Tryptophan is prone to free radical reactions and modification by HOCl. We hypothesized, that free tryptophan may quench the HOCl attack therefore protecting LDL. Free tryptophan inhibits LDL apoprotein modification and lipid oxidation. Tryptophan-HOCl metabolites associate with LDL reducing its oxidizability initiated by endothelial cells, Cu(2+) and peroxyl radicals. One tryptophan-HOCl metabolite was identified as 4-methyl-carbostyril which showed antioxidative activity when present during Cu(2+) mediated lipid oxidation, but did not associate with LDL. Indole-3-acetaldehyde, a decomposition product of tryptophan chloramine (the product of the tryptophan-HOCl reaction) was found to associate with LDL increasing its resistance to oxidation. Myeloperoxidase treatment of LDL in the presence of chloride, H(2)O(2) and tryptophan protected the lipoprotein from subsequent cell-mediated oxidation. We conclude that, in vivo, the activated myeloperoxidase system can generate antioxidative metabolites from tryptophan by the reaction of hypochlorite with this essential amino acid.     

Catalytic effects of Murchison Material: Prebiotic Synthesis and Degradation of RNA Precursors

Mineral components of the Murchison meteorite were investigated in terms of potential catalytic effects on synthetic and hydrolytic reactions related to ribonucleic acid. We found that the mineral surfaces catalyzed condensation reactions of formamide to form carboxylic acids, amino acids, nucleobases and sugar precursors. These results suggest that formamide condensation reactions in the parent bodies of carbonaceous meteorites could give rise to multiple organic compounds thought to be required for the emergence of life. Previous studies have demonstrated similar catalytic effects for mineral assemblies likely to have been present in the early Earth environment. The minerals had little or no effect in promoting hydrolysis of RNA (24mer of polyadenylic acid) at 80°C over a pH range from 4.2 to 9.3. RNA was most stable in the neutral pH range, with a half-life ~5 h, but at higher and lower pH ranges the half-life decreased to ~1 h. These results suggest that if RNA was somehow incorporated into a primitive form of RNA-based thermophilic life, either it must be protected from random hydrolytic events, or the rate of synthesis must exceed the rate of hydrolysis.     

Lipid domain boundaries as prebiotic catalysts of peptide bond formation

To address central problems in the origin of life such as the formation of linear polymers composed of only a small number of types of molecules, we have modeled the distribution of peptides in lipid monolayers. We show that short peptides and amino acids accumulate at the boundary between lipid domains, and that the concentration towards the boundary is higher the longer the peptide. We invoke a constraint on diffusion to one dimension as well as on orientation to suggest that polymerization of peptides is more likely to occur at the domain boundary than within domains or in the bulk phase. In a simple model, in which polymerization is taken to occur only at the boundary, we show that the equilibrium distribution of polymer lengths is shifted towards longer peptides. Since the reaction is occurring in a partially non-aqueous environment, hydrolysis is reduced and condensation increased to yield a significant polymerization. We show also that the free energy change from the redistribution of peptides within domains is sufficient to drive the formation of the peptide bond.     

Eutectic phase in water-ice: a self-assembled environment conducive to metal-catalyzed non-enzymatic RNA polymerization

Information and catalytic polymers play an essential role in contemporary cellular life, and their emergence must have been crucial during the complex processes that led to the assembly of the first living systems. Polymerization reactions producing these molecules would have had to occur in aqueous medium, which is known to disfavor such reactions. Thus, it was proposed early on that these polymerizations had to be supported by particular environments, such as mineral surfaces and eutectic phases in water-ice, which would have led to the concentration of the monomers out of the bulk aqueous medium and their condensation. This review presents the work conducted to understand how the eutectic phases in water-ice might have promoted RNA polymerization, thereby presumably contributing to the emergence of the ancient information and catalytic system envisioned by the 'RNA-World' hypothesis.     

Site of Inhibition of Peptidoglycan Biosynthesis During the Stringent Response in Escherichia coli

The site of inhibition of peptidoglycan synthesis during the stringent response in Escherichia coli was determined in strains which were auxotrophic for both lysine and diaminopimelic acid (DAP). Cells were labeled with [(3)H]DAP for 30 to 60 min in the presence and absence of required amino acids, and the cellular distribution of [(3)H]DAP was determined. In both stringent (rel(+)) and relaxed (relA) strains, amino acid deprivation did not inhibit the incorporation of [(3)H]DAP into the nucleotide precursor and lipid intermediate fractions. The amount of [(3)H]DAP incorporated into the peptidoglycan fraction by the amino acid-deprived relA strain was over 70% of the amount incorporated in the presence of required amino acids. In contrast, the amounts of labeled peptidoglycan in amino acid-deprived rel(+) strains were only 20 to 44% of the amounts synthesized in the presence of amino acids. These results indicate that a late step in peptidoglycan synthesis is inhibited during the stringent response. The components of the lipid intermediate fraction synthesized by rel(+) strains in the presence and absence of required amino acids were quantitated. Amino acid deprivation did not inhibit the synthesis of either the monosaccharide-pentapeptide or the disaccharide-pentapeptide derivatives of the lipid intermediate. Thus, the reaction which is most likely inhibited during the stringent response is the terminal one involving the incorporation of the disaccharide-pentapeptide into peptidoglycan.     

A New Pathway to Aspartic Acid from Urea and Maleic Acid Affected by Ultraviolet Light

The photochemistry of a mixture of ureaand maleic acid, which are thought to have been widelypresent on the primitive Earth, was studied in order toexamine a possibility of the formation of amino acids. When an aqueous solution of urea and maleic acid wasirradiated with an ultraviolet light of wavelength 172 nm,urea was revealed to be rather resistant to photochemicaldecomposition. In contrast, maleic acid was completelydecomposed within 4 h, reflecting the reactivity of a C-Cdouble bond in the molecule. In the reaction mixture, 2-isoureidosuccinic acid was detected. The acid wasconsidered to be formed by addition of an isoureido radicalwhich had been produced from urea by the action of ahydroxyl radical, to a C-C double bond of maleic acid. Theisoureido group of the product was revealed to undergothermal rearrangement to afford 2-ureidosuccinic acid (N-carbamoylaspartic acid). The result suggested a novelpathway leading to the formation of aspartic acid from non-amino acid precursors, possibly effected by UV-light on theprimitive Earth. The formation of ureidocarboxylic acidsis of another significance, since they are capable ofundergoing thermal polymerization, resulting in formationof polyamino acids.     

A secondary isotope effect in the lipoxygenase reaction

Fatty acids containing a prochiral tritium label have often been used in the study of enzymatic reactions which involve an obligatory step of hydrogen abstraction. In the lipoxygenase reaction, the primary isotope effect associated with this approach is detected as an isotopic enrichment of the substrate. Herein we characterize a previously unrecognized secondary isotope effect which changes the specific activity of both the substrate and product. The 12-lipoxygenase of human platelets removes the 10-LS hydrogen of arachidonic acid in the formation of 12-hydroperoxyeicosatetraenoic acid. We studied the specific activity changes associated with conversion of the enantiomerically labeled [10-DR-3H]arachidonic acid to 12-[10-3H]hydroxyeicosatetraenoic acid in aspirin-treated platelets. [3-14C]Arachidonic acid served as internal standard. The most pronounced change in 3H/14C ratio in the early stages of reaction was a 15-20% deficiency of tritium in the product. Later, the remaining arachidonate showed a marked increase in 3H/14C ratio. The changes in specific activity closely matched those predicted for a secondary isotope effect. Comparison of these data with the theoretical equations for a secondary isotope effect indicated the 10-DR-3H substrate reacted at about 84% of the rate of unlabeled molecules. Interestingly, this secondary isotope effect is similar in magnitude to the secondary isotope effect in autoxidation reactions, a finding compatible with a basic similarity in reaction mechanisms in enzymatic and non-enzymatic oxygenation of lipids.