Entender como se originou a vida é um dos desafios propostos pela astrobiologia. Este trabalho busca compreender como argilas aniônicas do tipo hidróxidos duplos lamelares (LDH) interagem com alguns aminoácidos quando submetido a condições presentes no passado do nosso planeta. Para tanto, foi estudada a interação dos aminoácidos cisteína (cys), cistina (cyss) e ácido glutâmico (glu) com duas variações de LDHs: hidrotalcita, que consistem em um LDH de Mg e Al (LDHal), e as piroauritas, um LDH de Mg e Fe III (LDHfe). Os LDHs foram sintetizados com cada um dos três aminoácidos por coprecipitação (cop) e reconstrução (rec). Todos os compostos produzidos foram submetidos a irradiação com UV-C (254 nm), longa exposição à temperatura de 70 °C e ciclos de hidratação e dessecação a 70 °C, tentando simular condições próximas à Terra primitiva. Os resultados obtidos indicam que os aminoácidos estão presentes no espaço interlamelar dos LDHs. Sendo que os LDHfe e os LDHal_glu se mostraram mais inertes, não sofrendo variações significativas com as simulações prebióticas. Para os LDHal_cys ocorreu a formação de ligações do tipo S-S durante a síntese; a irradiação UV-C afetou de maneira distinta os LDHs cop e rec, sendo que apenas nos reconstruídos ocorreu a formação de SO4-2. A simulação de temperatura causou o rompimento das ligações S-S e a formação de ligações S-H, enquanto os ciclos de hidratação, ao que tudo indicam, acarretam a liberação da cisteína do meio interlamelar. Essas características presentes no LDHal_cys estão, em partes, também presentes para os LDHal_cyss. De maneira geral, os LDHs são eficientes na intercalação de aminoácidos e estáveis quanto à temperatura e, em alguns casos, a radiação UV-C. Desta forma os LDHs se mostram como um mineral que pode ter tido a sua importância na Terra prebiótica, sendo aptos a atuar na retenção de aminoácidos, resistência a algumas das condições presentes e com a possibilidade de liberar estas biomoléculas novamente no ambiente, tornando-as disponíveis para o aumento de complexidade química / Understanding how life originated is one of the challenges proposed by astrobiology. This work aims to understand how layered double hydroxides (LDH), a type of anionic clay, may interact with amino acids when submitted to conditions present in prebiotic Earth. It was studied the interaction between amino acids cysteine (cys), cystine (cyss) and glutamic acid (glu) with two LDHs variations: hydrotalcite, LDH of Mg and Al (LDHal), and pyroaurite, a LDH of Mg and Fe III (LDHfe). LDHs were synthesized with each of the three amino acids by coprecipitation (cop) and reconstruction (rec). All the LDHs produced were submitted to UV-C irradiation (254 nm), long exposure to the temperature of 70 °C and cycles of hydration and desiccation at 70 °C, trying to simulated the conditions presents in primordial Earth. The results indicate that amino acids are present in the interlayer region of LDHs. Since LDHfe and LDHal_glu were shown to be more inert, they did not undergo significant variations with the prebiotic simulations. For LDHal_cys the formation of S-S type bonds occurred during the synthesis; the UV-C irradiation differently affected the LDHs cop and rec, being that only in the reconstructed the formation of SO4-2 occurred. The temperature simulation induced breakage of the S-S bonds and formation of S-H bonds, whereas the hydration cycles leaded to the release of cysteine from the interlamellar space. These features present in LDHal_cys are, partially, also present for the LDHal_cyss. In general, LDHs are efficient in the intercalation of amino acids, stable in temperature and, in some cases, to UV-C radiation. In this manner, the LDHs may have been important minerals in the prebiotic Earth, being able to act in the retention of amino acids, resisting to some of the prevailing conditions and possibly releasing these biomolecules back into the environment, making them available for increasing chemical complexity

Esta tese se insere no contexto da química prebiótica, que estuda a evolução química que ocorreu antes do surgimento da vida na Terra. Tal área pertence ao ramo de pesquisa da Astrobiologia, que estuda o surgimento, a evolução, distribuição e futuro da vida na Terra ou em outro lugar do Universo. Dentre as várias hipóteses abordadas na química prebiótica, a hipótese mineral é foco de estudo deste trabalho, ou seja, se os minerais podem ter agido como preconcentradores ou protetores de moléculas biologicamente relevantes para a química prebiótica e como catalisadores de reações. A classe mineral de hidróxidos duplo lamelares (HDL) é estudada inicialmente considerando se sua síntese seria possível em um ambiente prebiótico. Desta forma, o HDL foi sintetizado por dois métodos de síntese (coprecipitação e reconstrução) e em quatro composições distintas de água do mar sintética, que mimetizam diferentes fases geológicas da Terra, os resultados mostraram a formação deste mineral em todas as composições de água do mar analisadas. Posteriormente, o estudo da interação de biomoléculas com HDL foi feito visando caracterizar se estas poderiam estar inseridas no espaço interlamelar deste mineral. O íon tiocianato, precursor de biomoléculas, e as bases nitrogenadas adenina, timina, e uracila mostraram-se presentes nas amostras de HDL sintetizadas pelos dois métodos, coprecipitação e reconstrução. As amostras foram caracterizadas por difratometria de raios X, análise termogravimétrica, análise elementar e por espectroscopia vibracional, Raman e no infravermelho. Embora os resultados iniciais indiquem que as biomoléculas possam estar interagindo com o mineral por adsorção e não necessariamente estejam intercaladas, estudos com lavagem das amostras com carbonato de sódio mostraram a troca iônica das biomoléculas pelo ânion inorgânico e sugerem que estas encontravam-se realmente no espaço interlamelar do mineral. Foram feitas então simulações de ambientes extremos nos sistemas HDL + biomoléculas para avaliar se a presença do mineral aumenta a estabilidade das biomoléculas frente a aquecimento, radiação UVC e radiação ionizante já que tais condições extremas estariam presentes na Terra primitiva / This thesis subject is related to prebiotic chemistry, which studies the chemical evolution that happened before the origin of life on Earth. This subject belongs to the Astrobiology research area, which studies the origin, evolution, distribution and future of life on Earth and elsewhere in the Universe. Among the many hypothesis that prebiotic chemistry encompass, the mineral hypothesis is the aim of this thesis, that is, if minerals could have had a role in preconcentrating and protecting molecules relevant to prebiotic chemistry, and also if they could have acted as catalists. The layered double hydroxide (LDH) minerals are studied and the first question is if they could have been synthetized in a prebiotic environment. Four different seawater compositions are analyzed, considering many geological periods of Earth, and two synthesis methods were studied: coprecipitation and reconstruction. The results showed that the LDHs are formed in all seawater types studied. Following these studies, we discuss whether biomolecules could be in the interlayer space of this mineral. Thiocyanate, a biomolecule precursor, and the nucleic acids adenine, thymine and uracil were present in the LDH samples synthetized either by coprecipitation and reconstruction, and they were characterized by X-Ray diffraction, thermogravimetric analysis, elemental analysis and by vibrational spectroscopy: IR and Raman. Although the preliminary results showed that the biomolecules are not necessarily intercalated, but may simply be adsorbed on the minerals, after washing with a sodium carbonate solution, the biomolecules were replaced by the inorganic anion, suggesting that the former was in fact intercalated in the mineral. Extreme conditions simulations were then performed on the LDH plus biomolecules systems to evaluate whether the mineral may act as a protector and stabilize the biomolecules when these were heated or irradiated with UV-C and ionizing radiation, since such scenarios would be common on early Earth

Entender como se originou a vida é um dos desafios propostos pela astrobiologia. Este trabalho busca compreender como argilas aniônicas do tipo hidróxidos duplos lamelares (LDH) interagem com alguns aminoácidos quando submetido a condições presentes no passado do nosso planeta. Para tanto, foi estudada a interação dos aminoácidos cisteína (cys), cistina (cyss) e ácido glutâmico (glu) com duas variações de LDHs: hidrotalcita, que consistem em um LDH de Mg e Al (LDHal), e as piroauritas, um LDH de Mg e Fe III (LDHfe). Os LDHs foram sintetizados com cada um dos três aminoácidos por coprecipitação (cop) e reconstrução (rec). Todos os compostos produzidos foram submetidos a irradiação com UV-C (254 nm), longa exposição à temperatura de 70 °C e ciclos de hidratação e dessecação a 70 °C, tentando simular condições próximas à Terra primitiva. Os resultados obtidos indicam que os aminoácidos estão presentes no espaço interlamelar dos LDHs. Sendo que os LDHfe e os LDHal_glu se mostraram mais inertes, não sofrendo variações significativas com as simulações prebióticas. Para os LDHal_cys ocorreu a formação de ligações do tipo S-S durante a síntese; a irradiação UV-C afetou de maneira distinta os LDHs cop e rec, sendo que apenas nos reconstruídos ocorreu a formação de SO4-2. A simulação de temperatura causou o rompimento das ligações S-S e a formação de ligações S-H, enquanto os ciclos de hidratação, ao que tudo indicam, acarretam a liberação da cisteína do meio interlamelar. Essas características presentes no LDHal_cys estão, em partes, também presentes para os LDHal_cyss. De maneira geral, os LDHs são eficientes na intercalação de aminoácidos e estáveis quanto à temperatura e, em alguns casos, a radiação UV-C. Desta forma os LDHs se mostram como um mineral que pode ter tido a sua importância na Terra prebiótica, sendo aptos a atuar na retenção de aminoácidos, resistência a algumas das condições presentes e com a possibilidade de liberar estas biomoléculas novamente no ambiente, tornando-as disponíveis para o aumento de complexidade química / Understanding how life originated is one of the challenges proposed by astrobiology. This work aims to understand how layered double hydroxides (LDH), a type of anionic clay, may interact with amino acids when submitted to conditions present in prebiotic Earth. It was studied the interaction between amino acids cysteine (cys), cystine (cyss) and glutamic acid (glu) with two LDHs variations: hydrotalcite, LDH of Mg and Al (LDHal), and pyroaurite, a LDH of Mg and Fe III (LDHfe). LDHs were synthesized with each of the three amino acids by coprecipitation (cop) and reconstruction (rec). All the LDHs produced were submitted to UV-C irradiation (254 nm), long exposure to the temperature of 70 °C and cycles of hydration and desiccation at 70 °C, trying to simulated the conditions presents in primordial Earth. The results indicate that amino acids are present in the interlayer region of LDHs. Since LDHfe and LDHal_glu were shown to be more inert, they did not undergo significant variations with the prebiotic simulations. For LDHal_cys the formation of S-S type bonds occurred during the synthesis; the UV-C irradiation differently affected the LDHs cop and rec, being that only in the reconstructed the formation of SO4-2 occurred. The temperature simulation induced breakage of the S-S bonds and formation of S-H bonds, whereas the hydration cycles leaded to the release of cysteine from the interlamellar space. These features present in LDHal_cys are, partially, also present for the LDHal_cyss. In general, LDHs are efficient in the intercalation of amino acids, stable in temperature and, in some cases, to UV-C radiation. In this manner, the LDHs may have been important minerals in the prebiotic Earth, being able to act in the retention of amino acids, resisting to some of the prevailing conditions and possibly releasing these biomolecules back into the environment, making them available for increasing chemical complexity

Desde o clássico experimento de Miller em 1953 evidenciando a formação de aminoácidos em condições de Terra primitiva, a química do período pré-biótico ainda é muito discutida. Cita-se, por exemplo, o papel da teoria sulfociânica, que descreve a origem de moléculas orgânicas a partir de compostos contendo enxofre, como o tiocianato de amônio (NH4SCN). Neste contexto, essa Tese aborda um estudo sobre a investigação do NH4SCN em condições pré-bióticas. Para isso, experimentos de oxidação eletroquímica e de irradiação ultravioleta (UV) em amostras contendo NH4SCN em diferentes condições experimentais foram conduzidos. Por eletroquímica acoplada à espectroscopia vibracional no infravermelho (FTIR in situ), identificou-se como o primeiro produto da oxidação do NH4SCN, o dímero tiocianogênio (SCN)2, que é um reconhecido precursor dos oligômeros do período pré-biótico. Em contrapartida, a irradiação UV do NH4SCN levou a formação de enxofre ortorrômbico (S8) e das bases nitrogenadas 4-(3H)-pirimidinona, citosina, purina e adenina, além de outras moléculas. Provavelmente, o cianeto de hidrogênio (HCN) é um dos precursores das biomoléculas supracitadas, contrariando uma possível rota via (SCN)2. Os resultados desse estudo também reforçam a hipótese de que não há formação direta de aminoácidos por irradiação do NH4SCN. Desta forma, propõe-se aqui que a formação dos blocos do DNA, as bases nitrogenadas, também possa ser inserida no contexto da teoria sulfociânica. / Since the classic Miller experiment in 1953 evidencing the amino acids formation under early Earth conditions, the chemistry of the prebiotic period is still very discussed. It is cited, for example, the role of sulfocyanic theory, which describes the origin of organic molecules from sulfur-containing compounds such as ammonium thiocyanate (NH4SCN). In this context, this thesis shows a study about the investigation of NH4SCN in prebiotic conditions. Thereby, experiments of electrochemical oxidation and ultraviolet (UV) irradiation were carried out with samples containing NH4SCN in different experimental conditions. By using electrochemistry coupled to Fourier transform infrared spectroscopy (FTIR in situ), the dimer thiocyanogen (SCN)2 was identified as the first oxidation product of NH4SCN, which is a recognized precursor of the oligomers from prebiotic period. In counterpart, UV irradiation of the NH4SCN led to the formation of orthorhombic sulfur (S8) and the nitrogenous bases 4-(3H)-pyrimidinone, cytosine, adenine and purine, besides other molecules. Probably, hydrogen cyanide (HCN) is one of the precursors of the biomolecules abovementioned, contradicting a possible route via (SCN)2. The results of this study also reinforce the hypothesis that there is no direct formation of amino acids by irradiation of NH4SCN. Thus, it is proposed here that the formation of DNA blocks, the nitrogenous bases, can also be inserted in the context of sulfocyanic theory.

El origen de la vida en la Tierra es una de las preguntas más difíciles presentadas a la ciencia. En los últimos 60 años, ha habido un progreso considerable en entender cómo moléculas relativamente sencillas, que son relevantes para la vida, pueden ser generadas espontáneamente o pueden llegar a la Tierra desde el espacio. Además, los análisis de la evolución de la historia de ácidos nucleicos, los cuales almacenan la información genética, apuntan a un ancestro común universal ya extinto. Los estudios del origen de la vida ofrecen muchas pistas que apuntan hacia un origen común, quizás no solo en el Tierra sino también en algún otro punto del sistema solar. Debido al largo tiempo transcurrido desde que la Tierra empezó a albergar vida, las pistas más antiguas de los primeros organismos se han perdido. Es muy poco probable encontrar exactamente cómo fue este primer organismo. Sin embargo, en los últimos años la biología sintética ha logrado progresar mucho en la modificación de biomoléculas, en particular, los ácidos nucleicos. Es posible que pronto podamos construir y comprender un sistema minimalista en el cual las moléculas puedan copiarse a sí mismas dentro de una célula rudimentaria. El estudio de un sistema así podría permitirnos develar el origen de los primeros organismos. / The origin of life on Earth is one of the most challenging questions in science. In the last 60 years, considerable progress has been made in understanding how simple molecules relevant to life can be generated spontaneously or are known to arrive to Earth from space. Additionally, analysis of the evolution history of nucleic acids, which are the repository of genetic information, points to a now extinct, universal common ancestor for all life on Earth. The studies of the origin of life offer many clues towards a common origin, perhaps not just on Earth but somewhere else in the solar system. However due to the length of time that the Earth has harbored life, the oldest clues of the first organisms are mostly gone. It is unlikely to find exactly what this first organism was like. Nevertheless, in the last few years, synthetic biology has made remarkable progress at modifying biomolecules, particularly nucleic acids. It is possible that soon we will be able to construct and understand a minimalistic system in which molecules can copy themselves in a protocell. The study of such systems could shed light into the origin of the first organisms.

L'élongation de peptides ou d'acides aminés N-acylés via une activation C-terminale (par exemple par un carbodiimide) est délaissée en synthèse peptidique à cause de l'épimérisation rapide des intermédiaires 5(4H)- oxazolones issus de cette activation. Au contraire, cela représente une voie prometteuse en chimie prébiotique où les substrats sont a priori racémiques, et où une étape d'épimérisation peut favoriser un scénario protométabolique / autocatalytique d'émergence de l'homochiralité. Partant de travaux récents qui montraient clairement que l'activation C-terminale de peptides en milieu aqueux procède surtout via une 5(4H)-oxazolone, nous avons étudié la stéréosélectivité des couplages peptidiques qui en résultent dans des conditions prébiotiques plausibles (milieu aqueux dilué à pH faiblement acide). Notre étude sur des peptides modèles (préparés par des méthodes classiques de synthèse peptidique et comportant un résidu tyrosine qui facilite l'analyse par HPLC) visait à évaluer l'effet de la configuration des résidus voisins ou des nucléophiles ; elle a montré la formation d'excès diastéréomériques significatifs en faveur de dérivés homochiraux, sous l'influence prépondérante de la chiralité du nucléophile.Nous avons ensuite étudié la réactivité de dipeptides libres dans les mêmes conditions, pour évaluer la formation compétitive de dicétopipérazine (DCP), qui est susceptible de bloquer l'élongation au-delà du dipeptide. La formation de DCP est prépondérante à partir de dipeptides faiblement activés, mais n'a pas lieu en présence d'agents d'activation de potentiel élevé (e.g. l'EDC) qui favorisent la formation plus rapide d'oxazolone et permet l'élongation peptidique ; ces derniers résultats soulignent l'importance prébiotique de potentiels d'activation élevés. / The elongation of peptides or N-acylamino acids through C-terminus activation is usually avoided in peptide synthesis, because of the fast epimerisation of 5(4H)-oxazolones intermediates resulting form such activation. Conversely, it represents a promising perspective in prebiotic chemistry where substrates are assumed to be racemic, and where an epimerisation step may favour a protometabolic / autocatalytic scenario of emergence of homochirality.Based on recent works which clearly showed that the C-terminus activation of peptides in aqueous media mostly proceed through a 5(4H)-oxazolone, we investigated the stereoselectivity of peptide couplings resulting therefrom under plausible prebiotic conditions (dilute aqueous medium at weakly acidic pH). Our study on model peptides (prepared by classical peptide synthesis methods, and bearing a tyrosine residue which facilitates HPLC analysis), aimed at assessing the influence of the configuration of the vicinal peptide residue or of the nucleophile; we observed significant diastereomeric excesses in favour of homochiral sequences, under the preponderant influence of the chirality of the nucleophile.Then we investigated the reactivity of free dipeptides under the same conditions, to assess the extent of diketopiperazine (DKP) formation, which may prevent further elongation beyond dipeptides. While DCP formation is preponderant from weakly activated peptides, id does not occur in the presence of high potential activation agents (e.g. EDC), which favour the faster formation of oxazolone and allow subsequent peptide eleongation; these last results undeline the prebiotic importance of high activation potentials.

Les surfaces minérales auraient eu un rôle important dans la chimie prébiotique, grace à leurs propriétés catalytiques, tel que le champ électrique de surface. Dans ce travail, le champ électrique à la surface de MgO et à l'interface MgO/eau est étudié en utilisant la dynamique moléculaire ab-initio. Ce champ est local et intense, de l'ordre de V/Å, même lorque la surface est recouverte d'eau. Une réaction prébiotique modèle est ensuite étudiée, à la surface de MgO : une molécule de monoxide de carbone et une molécule d'eau, donnant une molécule d'acide formique. En utilisant la métadynamique, et sans connaissance des états de transition en amont, des chemins de réaction sont trouvés et leurs profils d 'énergie libre sont calculés à 5 kcal/mol près, avec l'aide d'un échantillonage dans l'espace des configurations par « umbrella sampling ». La présence de la surface minérale stabilise l'acide formique d'au moins 15 kcal/mol par-rapport au cas en solution sans surface. La même réaction a aussi été étudiée sous un champ électrique homogène de 0,3 V/Å, afin de comparer l'effet de ce champ à l'effet du champ de surface sur le paysage d'énergie libre. Le champ homogène stabilise aussi le produit, et l'acide formique se trouve orienté dans la direction du champ électrique de surface ainsi que dans le champ électrique homogène. Ce travail montre que les conditions proche d'une surface minérale, même sans adsorption directe, peut modifier considerablement le paysage d'énergie libre de réactions chimiques, ce qui pourrait avoir de l'importance en chimie prébiotique. / Mineral surfaces are thought to be of importance to prebiotic chemistry due to their catalytic properties, which include a strong electric field at the interface. In this work the electric field at the surface of MgO and at the interface of MgO and water is studied through ab-initio molecular dynamics. The spontaneous electric field from the surface is found to be local and intense, on the order of V/Å, even when completely covered with water. A model prebiotic reaction is then studied on the model MgO surface : carbon monoxide and water yielding formic acid. Using metadynamics, reaction pathways were found with no a priori knowledge of the transition states, and umbrella sampling was then used to compute free energy landscapes to about 5 kcal/mol accuracy. The presence of the mineral surface was found to stabilise formic acid by at least 15 kcal/mol compared to the bulk case. The reaction was also studied in solution with an applied electric field of 0.3 V/Å, in order to estimate to impact of the surface electric field on the free energy landscape. The field is also found to stabilise the product, and formic acid is found to have a preferred orientation in the direction of both the applied electric field and the surface electric field. This work shows that near surface conditions (without direct adsorption) can significantly alter the free energy landscapes of chemical reactions, in a way which could be of importance for prebiotic chemistry.

Le développement d’outils de détection in situ (IDT) est indispensable pour rapporter entemps réel la présence d’une signature moléculaire spécifique. L’efficacité d’un IDT estliée à son affinité, à sa spécificité, mais aussi à son potentiel à opérer dans des conditionsimposées par le contexte d’application. Parmi les contraintes imposées, la variation detempérature, le pH et la présence de solvant d’extraction. Le but du projet est dedévelopper des aptamères capables d’opérer en présence de solvant organique ; à ceteffet, nous avons opté pour une sélection en présence de méthanol. La limitation decette stratégie est principalement liée à la nature chimique des acides nucléiques. Parconséquent, nous avons choisi d’utiliser une banque ADN incorporant le (5-(octa1,7-diynyl)-2’-deoxyuridine) dDOTP, au lieu du dTTP. Notre stratégie expérimentale aabouti à la sélection d’un aptamère qui lie spécifiquement l’adénine en présence de 25 %de méthanol. Nous avons montré que les dDOTP sont essentiels à l’interaction del’aptamère avec l’adénine ; l’aptamère sélectionné comporte un motif riche en G partagéavec l’aptamère anti-adénosine, cependant, l’aptamère sélectionné dans le méthanolcomporte un motif structural indispensable à l’interaction avec la cible en présence deméthanol. Par ailleurs, nous avons montré que l’aptamère sélectionné pourraitfonctionner comme un module de reconnaissance spécifique d’un biocapteur. / Development of in situ detection tools (IDT) is required for specific real time monitoringof chemical species. Efficient IDT is not only related to its affinity and ability todiscriminate between molecular variants, but moreover it must be adapted for operatingunder conditions imposed by the context of application. Among others, hightemperature, pH variation and presence of organic solvents may be mentioned. The aimof our project is to develop an aptamer operating in the presence of organic solvents. Forthis purpose, we opted for selection in presence of methanol. Limitations of this strategyare adaptability of SELEX technology and chemical diversity of nucleic acids. For thispurpose, we used library incorporating (5-(octa1,7-diynyl)-2’-deoxyuridine) dDOTPinstead of conventional thymine nucleotide. Our experimental strategy led to theselection of an aptamer that specifically recognises adenine in the presence of 25 % ofmethanol. dDOTP nucleotides are essential for adenine recognition; the selectedaptamer shares a purine rich motif with a previously described adenosine aptamer, butdisplays a specific structure motif, essential for operating in the presence of methanol.Furthermore, the ability of truncated variants of the selected aptamer to form arecognition module of biosensor was assessed in this study.

La vie a émergé sur Terre il y a probablement 3,8 milliards d'années, sur une planète largement recouverte d'eau. Ce travail porte sur la synthèse prébiotique de peptides, en particulier de peptides riches en thiol. Nous avons étudié les réactions des aminonitriles (les premiers produits de la réaction de Strecker) avec la cystéine et l'homocystéine. Elles conduisent à la formation de cycles à 5 ou 6 chaînons qui sont ensuite hydrolysés pour donner les dipeptides correspondants (aa-Cys ou aa-Hcy). Les dipeptides contenant un thiol obtenus sont capables de favoriser la formation de chaînes peptidiques plus longues via des liaisons thioesters et de favoriser la formation de certains hétérocycles. L'homocystéine nitrile se cyclise dans l'eau pour former l'homocystéine thiolactone, qui présente une double réactivité, la thiolactone est ouverte par des amines puis on observe une condensation de l'aminothiol ainsi formé avec les nitriles. Le nitrile de cystéine et le thioester de S-éthyle de la cystéine conduisent à la formation de polycystéine, tandis que les molécules de type Cys-aa-CN donnent des polypeptides linéaires et cycliques. Nos résultats soutiennent l’hypothèse que des peptides contenant des thiols auraient joué un rôle important dans les premiers stades du développement de la vie. / Life emerged on Earth probably about 3.8 billion years ago, on a planet that was largely covered by water. This work focuses on the prebiotic synthesis of peptides, especially thiol-rich ones. We studied the reactions of aminonitriles (the first products of the Strecker reaction) with cysteine and homocysteine. These reactions lead to the formation of 5- or 6-membered rings which are then hydrolysed to give the corresponding dipeptides (aa-Cys or aa-Hcy). The obtained thiol-containing dipeptides are able to promote the formation of longer peptide chains via thioesters bonds, and to promote the formation of some heterocycles. Homocysteine nitrile cyclizes in water to form homocysteine thiolactone, which shows a double reactivity, thiolactone opening by amines followed by aminothiol condensation reaction with nitriles. Cysteine nitrile and the S-ethyl thioester of cysteine lead to the formation of polycysteine, while Cys-aa-CN molecules gives linear and cyclic polypeptides. Our results support the hypothesis that thiol-containing peptides would have been important molecules in the early stages of life development.

Metabolism is a subset of chemistry that allows cells to defy thermodynamic equilibrium, a fundamental process that must have been in place from the very beginning of biology. Before evolution produced efficient catalysts in the form of complex protein machinery, short metal binding peptides might have preceded modern metalloproteins. Such prebiotic, metal-binding motifs have been hypothesized to have existed through analyses of extant protein sequences. However, it is unclear how metal-binding motifs might have evolved in the harsh prebiotic environment. Here, we show how certain environments, in particular seawater-like environments rich in divalent cations and especially Mg2+, support the survival of short peptides upon extreme temperatures as high as 150 °C. Moreover, while Mg2+ does not offer the same protection from UV light, peptides are protected from both heat and irradiation when bound to a metal ion. The results suggest that specific environments rich in metal ions may be better suited for the emergence of complex systems in the path toward life. Additionally, the conditional degradation of peptides depending on their ability of binding metals might have enabled a selection mechanism that would favor the survival of metal-binding motifs which resemble the motifs found in modern proteins. These short sequences could have acted as early, simple catalysts able to facilitate a restricted set of chemical reactions, which would shape the emergence and biology of the Last Universal Common Ancestor.