Formamide is a solvent of great interest to prebiotic chemists because it is liquid over a wide range, it is less volatile than either water or HCN, and it possesses a versatile reactivity. When formamide is heated in the presence of minerals or inorganic catalysts, a variety of products including purine nucleobases are generated. Irradiation of formamide reaction solutions with ultraviolet light increases the yield and diversity of products, and eliminates the need for a mineral catalyst. We have also performed formamide reactions in the presence of pyrite, a mineral which is likely to have been available on the primordial Earth, under a variety of atmospheric conditions. Our results indicate the greatest yield and diversity of products result from the combination of a pyrite mineral catalyst, heat, UV irradiation, and a carbon dioxide atmosphere. Purine nucleobases are simple to synthesize in model reactions and they stack well in aqueous solution; it has been hypothesized that the first nucleic acids were composed of only purine bases, and that water-soluble, cationic, aromatic molecules with large stacking surfaces (“”molecular midwives””) may have aided the assembly of the earliest nucleic acid analogs. We have characterized the interactions of various intercalators with a standard DNA duplex as well as with an antiparallel homopurine DNA duplex and have determined that molecules which possess four or more rings and a curved shape interact selectively with all-purine DNA; such molecules can serve as models for putative prebiotic midwives.

This dissertation has investigated the adsorption, thermal behavior, and radiation (both photon and electron) processing of prebiotically-relevant ices and surfaces. A custom ultra-high vacuum (UHV) chamber has been built that is coupled with a Fourier Transform-Infrared (FT IR) spectrometer and a Temperature Programmed Desorption (TPD) system that utilizes Quadrupole Mass Spectrometry (QMS) to study selected organic:surface systems. Formamide (HCONH₂) has been studied in two related but distinct studies relevant to primitive Earth and interstellar chemistry. First, in collaboration with a theory group, formamide’s interaction with kaolinite (Al6Si6O36H30), a clay mineral relevant to early Earth chemistry, has been studied experimentally and theoretically. Experimental infrared results are compared with calculated infrared frequencies obtained by our collaborators. TPD analysis is compared with the calculated values of adsorption energy, and the optimal kaolinite termination site for adsorption is reported. Second, the first thermal and radiation damage study of pure formamide and HCONH₂:H₂O mixed ices on an interstellar icy grain analog (SiO₂) is reported. A discussion of the pure formamide ice phases identified with FT-IR upon warm-up, as well as the TPD binding energies of HCONH₂ on SiO₂, is presented. The observed Lyman-alpha photochemical products and proposed formation mechanisms from pure formamide ice is reported and discussed. In addition, results of Lyman alpha processing of mixed HCONH₂:H₂O ices are provided. Low-energy electron irradiation of pure HCONH₂ and HCONH₂:H₂O mixed ices has also been reported for the first time. A third investigation has studied acetylene (C₂D₂) and acetonitrile (CH₃CN) interactions and radiation stability in mixed low-temperature ices to simulate possible prebiotic reactions that may occur on Saturn’s moon, Titan. This investigation contributes to understanding the possible consumption, trapping, and degradation of these species on the surface of Titan.

The origin of the first RNA polymers is central to most current theories regarding the origin of life. However, difficulties associated with the prebiotic formation of RNA have lead many researchers to conclude that simpler polymers, or proto-RNAs, preceded RNA. These earlier polymers would have been replaced by RNA over the course of evolution. A remaining difficulty for this theory is that the de novo synthesis of a feasible proto-RNA has not yet been demonstrated by plausible prebiotic reactions. This thesis focuses on two problems associated with prebiotic proto-RNA synthesis: The formation of nucleosides and the necessity of reversible backbone linkages for error correction in nucleic acid polymers. "The Nucleoside Problem", or the lack of success in forming pyrimidine nucleosides by plausible prebiotic reactions, represents a significant stumbling block to the RNA world hypothesis. Nearly four decades ago Orgel and coworkers demonstrated that the purine nucleosides adenosine and inosine are synthesized by heating and drying their respective bases and ribose in the presence of magnesium, but these reaction conditions do not yield the pyrimidine nucleosides uridine or cytidine from their respective bases. In this thesis a potential solution to The Nucleoside Problem is hypothesized based upon a proposed chemical mechanism for nucleoside formation. This hypothesis is supported by the successful synthesis of 2-pyrimidinone nucleosides by a plausible prebiotic reaction in good yield, demonstrating that pyrimidine nucleosides could have been available in the prebiotic chemical inventory, but that uridine and cytidine were likely not abundant. Reversible backbone linkages are necessary to provide a mechanism for error correction in non-enzymatic template-directed syntheses of proto-RNAs. In this thesis, acetals are explored as low-energy, reversible linkage groups for nucleosides in polymers. The synthesis of glyoxylate-acetal nucleic acids (gaNAs) through simple heating-drying reactions from neutral aqueous solutions is demonstrated, and these linkages are shown to be hydrolytically stable under a considerable range of solution conditions. Computational models demonstrate that the glyoxylate linkage is an excellent electronic and isosteric replacement for phosphate. Molecular dynamics simulations also indicate that a gaNA duplex would have structural properties that closely match a phosphate-linked RNA helix, suggesting the possibility for cross-pairing between gaNAs and RNAs, allowing for sequence transfer and genetic continuity through the evolution from proto-RNAs to RNA. The principles illustrated in this thesis by 2-pyrimidinone nucleoside and gaNA synthesis can be extended to other prebiotic condensation reactions. Factors affecting condensation yield, such as thermodynamics, kinetics, reactant solubility, and salt effects, are summarized herein.

La biogenèse du ribosome est un processus complexe et dynamique qui nécessite de nombreuses étapes de maturation et de modification des ARNr ainsi que l’assemblage et le transport des RNPs précurseurs. Un ribosome mature contient une centaine de pièces, ARN et protéines confondus, mais son assemblage requiert l’intervention de plus de 400 facteurs de synthèse. De part le coût énergétique important de ce processus, plusieurs voies de régulation interviennent pour contrôler la biogenèse des ribosomes en fonction des conditions nutritives. L’une des voies les plus connue est la voie TOR (Target of rapamycin). Cette voie de régulation agît principalement au niveau de la transcription des différents intervenants de la biogenèse :les ARNr, les protéines ribosomiques mais aussi les facteurs de synthèse. Ces facteurs, ayant une action transitoire dans la maturation des ribosomes, sont, par économie, recyclés pour la synthèse de nouveaux ribosomes. Nous nous sommes donc intéressés au devenir de ces facteurs, plus particulièrement de ceux intervenants dans la biogenèse de la petite sous unité, lorsque les conditions environnementales sont inadaptées à la croissance cellulaire. Ainsi, nous avons pu montré, pour quatre facteurs particuliers :Dim2, Rrp12, Hrr25 et Fap7, que leur localisation est dépendante de la synthèse ribosomique. Ainsi, lors de carence en sources nutritives, l’inhibition de la synthèse et de l’activité ribosomique entraîne un confinement de ces facteurs ribosomiques dans le nucléole ou dans des corps cytoplasmiques. En outre, la localisation particulière des facteurs ribosomiques Hrr25 et Fap7 dans les P-bodies en phase de croissance saturée laisse penser que ces corps cytoplasmiques sont le lieu de dégradation des pré-ribosomes lorsque les carences nutritives perdurent. / Doctorat en Sciences / info:eu-repo/semantics/nonPublished

Chirality is the property of objects, including molecules, which are not superimposable on their materialized mirror image. Chiral molecules are omnipresent in living organisms and the constituents of biological macromolecules (proteins and nucleic acids) are chiral. Amino-acids (constituting proteins), ribose and 2-deoxy-ribose (the only chiral constituent of RNA and DNA nucleotides respectively) are furthermore generally present in living organisms only under one of their enantiomeric forms. This is referred to as the homochirality of the living world. The origin of this homochirality is still unexplained, even if many partial scenarios have been proposed in the literature. All scenarios involve the creation of a small enantiomeric excess for certain molecules, amplification of this excess and chirality transfer to other chiral molecules. The origin of homochirality on Earth is closely related to the origin of life, and is currently supposed to have preceded life. As no-one will ever be able to directly observe the phenomena which lead to homochirality, and life, on our planet, the only scientific approach to try and help explain how this occurred is to build scenarios, and test them taking into account all available information on the physical and chemical conditions on the primitive Earth (Earth before life appeared). In our work, we investigated three scenarios related to the origin of homochirality on Earth. One of these scenarios also relates to a very precise step of the origin of life: the selection of beta-d-ribofuranose as component of RNA nucleotides.<p><p>Enantiomeric excesses (up to 15 %) of alpha-methylated alpha-amino-acids have been detected in meteorites which fell on Earth during the 20th century. No enantiomeric excess is detected for the corresponding alpha-hydroxy-acids in the same meteoritic samples and small (2% at most) or no enantiomeric excesses have been measured for non-methylated alpha-amino-acids. In the first part of our work, we investigated if photolysis by circularly polarized light (CPL) in space could be at the origin of the presence (or absence) of an enantiomeric excess for these compounds. Experiments to reproduce UV-CPL photolysis are difficult to undertake: they require high-energy circularly polarized photons, hence the use of a synchrotron. In our work, we used quantum mechanical calculations to obtain the electronic circular dichroïsm (ECD) spectra of two -methylated -amino-acids, their corresponding alpha-hydroxy-acids and one non-methylated alpha-amino-acid. Differences are observed between these spectra, and we propose a scenario to explain the experimental measurements reported here above: the enantioselective photolysis, in the gas phase at low temperatures (20K at most), of the alpha-amino-acids by UV-CPL with lambda>210 nm. Under these conditions no photolysis of the alpha-hydroxy-acids would occur. This scenario concerns the first step in the origin of homochirality on Earth: the creation of a small enantiomeric excess for some chiral molecules.<p><p>The second scenario that we investigated relates to the enantiomeric amplification step of the origin of homochirality on Earth, for which the role of the alpha-amino-acid serine has been suggested in the literature. Serine clusters have been observed in the gas phase by mass spectrometry. Among these clusters the octamer has been shown to be a magic number cluster and to have a preference for homochirality. An enantiomeric amplification via cycles of formation and dissociation of the octamer has been suggested. No complete scenario has however been proposed in the literature to explain how this could have occurred on the primitive Earth, but any scenario would most probably include an aqueous phase. We aimed at determining if the homochiral preference of serine octamers also exists in solution and therefore we first investigated if serine octamers exist in solution. For this study, we used nuclear magnetic resonance and infrared spectroscopies, which are well-adapted to the study of molecular assemblies in solution. We were able to demonstrate that most probably serine clusters are not present in solution, and if they are it could only be in extremely low concentration. The scenario suggested in the literature is discussed in the light of our results and of literature data on serine clusters.<p><p>As last hypothesis, we investigated a possible scenario for the selection of beta-d-ribofuranose as component of RNA nucleotides. The currently known prebiotic synthesis pathways to ribose also lead to the formation of many other carbohydrates, and ribose is only a minor product of these syntheses. Our hypothesis is that beta-d-ribofuranose could have been selected through favorable interactions with alpha-amino-acids already present on the primitive Earth under one enantiomeric form. Indeed, it is plausible that a peptidic world emerged before the presence of RNA and that homochiral alpha-amino-acids were present on Earth when RNA was synthesized. Under this hypothesis, we investigated the role that alpha-l-amino-acids could have played in the selection of alpha-d-ribofuranose as component of RNA nucleotides. This work is related to the last step of the origin of homochirality: chirality transfer. Our scenario was investigated via nuclear magnetic resonance studies of the interaction between alpha-amino-acids and carbohydrates. We were able to show that, in the systems that we studied, when an interaction occurs it is very weak (affinity constant less than 1M−1) and non enantioselective. Our results most probably discard the role that alpha-amino-acids alone could have played in the selection of beta-d-ribofuranose as component of RNA nucleotides, but does not discard the role that peptides could have played in this selection. / Doctorat en Sciences de l'ingénieur / info:eu-repo/semantics/nonPublished