Résumé
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
Sujets)
Acides aminés/synthèse chimique , Exobiologie , Analyse spectrale RamanRésumé
Rocks, apart from being ancient records that enlighten us about the geological history of our planet, are dynamic repositories that support life forms central to the sustenance of our biosphere. It is the latter that our discussion will be largely focused on. Life associated with rocks has been documented as early as 1914 (Diels 1914), but it was in the 1960s that Friedmann and colleagues, with their extensive studies on rock-dwellers in hot and cold desert habitats, gave shape to this modern branch of geobiology. The presence of microscopic algae and bacteria was first demonstrated within exposed rocks from hot desert environments such as the Negev and the Sinai (Friedmann and Galun 1974) by electron microscopy and laboratory cultivation methods. Subsequent studies in ortho-quartzite rocks from the Dry Valley area of Antarctica also showed morphologically similar algae (related to the genus Gloeocapsa) to be colonizing areas ~1.5 mm wide parallel to and ~2 mm beneath the rock surface (Friedmann and Ocampo 1976). The results from the latter caught the attention of the scientific community as NASA had been testing their Voyager mission probes on the apparently lifeless cold deserts of Antarctica with the aim of studying a habitat analogous to Mars. In 2005, Walker and colleagues, through the use of culture-independent molecular methods, discovered the microbial colonization of rocks from the extremely acidic (pH~1) Yellowstone geothermal environment. By employing universal PCR primers that targeted 16S rRNA genes from all three domains of life, the authors were able to retrieve sequences phylogenetically related to extant red alga (Cyanidium sp.), bacteria (α-, β-, γ-Proteobacteria; Actinobacteria; Bacteroidetes and Firmicutes) and archaea (Euryarchaeota and Crenarchaeota). The astoundingly high diversity of microbial life forms present in such extreme habitats captured the imaginations of geo(micro)biologists, astrobiologists and microbial ecologists alike. Astrobiologists imagined that if rock interiors could support the major fraction of life in the harshest of environments on earth, then the same could be applicable to other planets such as Mars, and they sensed that there was a need to extend the scope of extraterrestrial life detection missions beyond the mere analysis of top soils. Microbial ecologists wondered if rock-associated life was ubiquitous in the biogeosphere, and geo(micro)biologists hypothesized that the rock micro-habitat offered life (a) protection from intense solar radiations, temperature and desiccation and (b) a supply of nutrients, moisture and growth surfaces. Today, with two dedicated international scientific journals – Geobiology and Geomicrobiology Journal and an ever growing number of papers dealing with rock-associated microbes in microbiological research journals, the concept of ‘life in/on the rocks’ has become as hardened as the rock itself. What is apparently lacking, however, is an understanding among the general public that a ‘dumblooking’ average rock in their gardens (on this planet and perhaps in the gardens of intelligent beings on other planets) could be home to a dynamic assortment of interesting yet diverse living organisms of inevitably microbial nature.
Résumé
This paper is an introduction to gravitational and space life sciences and a summary of key achievements in the field. Current global research is focused on understanding the effects of gravity/microgravity onmicrobes, cells, plants, animals and humans. It is now established that many plants and animals can progress through several generations in microgravity. Astrobiology is emerging as an exciting field promoting research in biospherics and fabrication of controlled environmental life support systems. India is one of the 14-nation International Space Exploration Coordination Group (2007) that hopes that someday humans may live and work on other planets within the Solar System. The vision statement of the Indian Space Research Organization (ISRO) includes planetary exploration and human spaceflight. While a leader in several fields of space science, India is yet to initiate serious research in gravitational and life sciences. Suggestions are made here for establishing a full-fledged Indian space life sciences programme.
Résumé
A vida é primeiramente reconhecida como tal com base em considerações subjetivas a priori. A riqueza das relações subjetivas complexas da vida conosco é a "bioassinatura" mais fundamental, que nos permite construir estratégias para a busca de vida no universo.
la vida se reconoce como tal según consideraciones subjetivas a priori. La riqueza de las relaciones subjetivas complejas con nosotros es la biofirma más fundamental, que nos permite construir estrategias para la búsqueda de la vida en el universo.
Life is primarily recognized as such based on priori subjective considerations. The richness of complex subjective exchanges with us is the most fundamental biosignature, which allows us to build strategies for the search of life in the universe.