Líquenes y su importancia en la exploración del Sistema Solar

The exploration for life outside our planet is one of the main objectives proposed by astrobiology. Many international space missions have been launched and the most important have been focused on the planet Mars. Although many enigmas have been solved from the results of these missions, a large part of the research carried out in the field of astrobiology is developed at laboratories placed on Earth and through terrestrial areas that have been recognized as planetary analogues characterized by extreme habitability conditions. For the study of the evolution of life under these conditions, lichens have proven to be model organisms to know the limits of life in space and other planets. The main conclusion of the experiments on these organisms shows that they are able to survive in space.La búsqueda de la vida fuera de nuestro planeta es uno de los objetivos que se propone la astrobiología. Para ello se han llevado a cabo multitud de misiones espaciales de carácter internacional estando muchas de ellas centradas en el planeta Marte. Aunque a partir de los resultados de estas misiones se han resuelto muchos enigmas, también se desarrollan investigaciones en el campo de la astrobiología en laboratorios ubicados en la Tierra y en zonas terrestres que han sido reconocidas como análogos planetarios, caracterizadas por unas condiciones de habitabilidad extrema. Para el estudio de la evolución de la vida en estas condiciones, los líquenes han demostrado ser unos organismos especialmente idóneos para conocer los límites de la vida en el espacio y sobre otros planetas. Las conclusiones de los experimentos con estos organismos demuestran que son capaces de sobrevivir en el espacio

Insight of lichens as ideal models for astrobiological studies analyzed by Raman spectroscopy

Exposure experiments of different species to space conditions are essential because real space conditions with different radiation sources like ionizing radiation, UV-radiation, X-rays, gamma-ray from even galactic radiation, vacuum and space weathering by micro-dust cannot simultaneously be simulated in parallel even in our best simulation chambers on Earth. We need results from experiments under real space conditions to enable the development of appropriate predictions about the stability of organisms and their constituent organic parts. The extremophile lichen Circinaria gyrosa is one of the selected species within the BIOMEX (Biology and Mars Experiment) experiment and in this work we compare the previous Raman results obtained in this lichen [1] with the corresponding Raman results on the lichen Xanthoparmelia hueana. Both species have been exposed to space and simulated Mars-like conditions in planetary chambers and we have studied and identified possible degradation process in different layers and biomarkers. The analysis by Raman spectroscopy of simulated Space and Mars exposed samples confirm alterations and damages of the photobiont part of the lichen and changes related to the molecular structure of whewellite. The conclusions of this work will be important to understand what are the effects to consider when biological systems are exposed to space or Mars-like conditions and to expand our knowledge of how life survives in most extreme conditions that is a prerequisite in future planetary exploration projects.Acknowledgment Support for this work was provided by the Spanish Ministry of Economy, Industry and Competitiveness (MINECO), by the project BIOindicadores en MARTE y Espacio (BIOMARSS) (PID2019-109448RB-I00) and by INTA. References [1] M.R. Lopez Ramirez, L.G Sancho, J. P. de Vera, M. Baqué, U. Böttcher, E. Rabbow, J. Martínez-Frías, R. de la Torre Noetzel. Spectrochimica Acta, Part A. 261 (2021) 120046.Universidad de Málaga. Campus de Excelencia Internacional Andalucía Tec

The BIOMEX experiment on-board the International Space Station: limits of life and detection of biomarkers after exposure to space- and to Mars-like conditions

To explore the limits of terrestrial life in space, we have to understand the effects of the space environment on unprotected biological and chemical material, and on the degradation of organic molecules or biomarkers. The exposure platform EXPOSE-R2 on the ISS offer a suitable facility for the exposure of samples of the astrobiological model lichen Circinaria gyrosa, included in the BIOMEX experiment (Biology and Mars Experiment, ESA). During 18 months (2014-2016), the lichens lived in a latent state at space and at simulated Mars-like conditions, to study Mars’ habitability and resistance to space conditions. After the return of the samples in June 2016, initial analysis showed rapid recovery of photosystem II (PSII) activity in the samples exposed exclusively to space vacuum and to Mars-like atmosphere. In contrast, the samples directly exposed to solar UV radiation showed a slow and a lower recovery, in reference to their observed original activity. This tendency was corroborated with the complementary morphological/ultrastructural and biomolecular analyses. Complementary, the biogeochemical variations have been examined with Raman spectroscopy to assess the possible degradation of cell surfaces and pigments which were in contact with terrestrial rocks, and Martian analogue regolith. Identification of the biomarker whewellite (calcium oxalate) and other organic compounds and mineral products of the biological activity of Circinaria gyrosa were detected by Raman Laser. These findings contribute to answer questions on the habitability of Mars, the likelihood of the Lithopanspermia Hypothesis, the capability to detect biomolecules exposed to an extraterrestrial environment by life-detection instruments and will be of relevance for planetary protection issues

The BIOMEX Experiment on-board the International Space Station: Biomolecular- and Bio-geochemical changes of lichens exposed to space- and to Mars-like conditions

Exploration of the solar system is a priority research area of the AstRoMap European Astrobiology Roadmap (Horneck et al., 2015) [1], focused on various research topics, one of them is “Life and Habitability” and an other one is “Biomarkers for easy the detection of life”. Therefore “space platforms and laboratories” are necessary, such as EXPOSE, to gain more knowledment of space- and extraterrestrial habitats, eventually for human interplanetary exploration (Space, Moon, Mars, Encedalus, Titan, Europa). At the exposure platform EXPOSE-R2 on ISS (2014-2016), samples of the astrobiological model system Circinaria gyrosa gyrosa [3,4,5,6], belonging to the BIOMEX experiment [2], (Biology and Mars Experiment, ESA), were exposed during 18 months to space and to a Mars simulated environment, to study Mars habitability and resistance to space conditions. The data obtained by the investigation on biomarkers after being exposed to Mars-like conditions will support the analysis of data obtained during future instrumental detection operations in future space missions on Mars (i.e. ExoMars). After the return of the samples in June 2016, the first preliminary analysis showed a quick and complete recovery of metabolic activity of the control samples exposed to space vacuum and Mars-like atmosphere. In contrast, the samples directly exposed to extraterrestrial UV solar radiation showed slow recovery, in reference to their observed original activity. Here we expose the last results that show the biomolecular changes of the DNA analized by PCR and complementary sequencing techniques, in correlation with the previous results supporting changes in metabolic activity, and changes in viability (Electron- and fluorescence microscopy techniques), as well as in morphology/ultrastructure due to space vacuum and Mars atmosphere. Additionaly, the biogeochemical variations have been examined with spectroscopic analyses (Raman) to look for possible degradation of cell surfaces and pigments which were in contact with terrestrial rocks, and Martian analogue regolith. Moreover, differences were observed between samples irradiated with extraterrestrial UV solar radiation and samples positioned below defined as dark-control samples. These experiments will contribute to answer questions on the habitability of Mars, on the likelihood of the Lithopanspermia Hypothesis and will be of relevance for planetary protection issues

Limits of Life and the Habitability of Mars: The ESA Space Experiment BIOMEX on the ISS

BIOMEX (BIOlogy and Mars EXperiment) is an ESA/Roscosmos space exposure experiment housed within the exposure facility EXPOSE-R2 outside the Zvezda module on the International Space Station (ISS). The design of the multiuser facility supports—among others—the BIOMEX investigations into the stability and level of degradation of space-exposed biosignatures such as pigments, secondary metabolites, and cell surfaces in contact with a terrestrial and Mars analog mineral environment. In parallel, analysis on the viability of the investigated organisms has provided relevant data for evaluation of the habitability of Mars, for the limits of life, and for the likelihood of an interplanetary transfer of life (theory of lithopanspermia). In this project, lichens, archaea, bacteria, cyanobacteria, snow/permafrost algae, meristematic black fungi, and bryophytes from alpine and polar habitats were embedded, grown, and cultured on a mixture of martian and lunar regolith analogs or other terrestrial minerals. The organisms and regolith analogs and terrestrial mineral mixtures were then exposed to space and to simulated Mars-like conditions by way of the EXPOSE-R2 facility. In this special issue, we present the first set of data obtained in reference to our investigation into the habitability of Mars and limits of life. This project was initiated and implemented by the BIOMEX group, an international and interdisciplinary consortium of 30 institutes in 12 countries on 3 continents. Preflight tests for sample selection, results from ground-based simulation experiments, and the space experiments themselves are presented and include a complete overview of the scientific processes required for this space experiment and postflight analysis. The presented BIOMEX concept could be scaled up to future exposure experiments on the Moon and will serve as a pretest in low Earth orbit