Planetary Atmosphere and Surfaces Chamber (PASC): A Platform to Address Various Challenges in Astrobiology

The study of planetary environments of astrobiological interest has become a major challenge. Because of the obvious technical and economical limitations on in situ planetary exploration, laboratory simulations are one of the most feasible research options to make advances both in planetary science and in developing a consistent description of the origin of life. With this objective in mind, we applied vacuum technology to the design of versatile vacuum chambers devoted to the simulation of planetary atmospheres’ conditions. These vacuum chambers are able to simulate atmospheres and surface temperatures representative of the majority of planetary objects, and they are especially appropriate for studying the physical, chemical and biological changes induced in a particular sample by in situ irradiation or physical parameters in a controlled environment. Vacuum chambers are a promising potential tool in several scientific and technological fields, such as engineering, chemistry, geology and biology. They also offer the possibility of discriminating between the effects of individual physical parameters and selected combinations thereof. The implementation of our vacuum chambers in combination with analytical techniques was specifically developed to make feasible the in situ physico-chemical characterization of samples. Many wide-ranging applications in astrobiology are detailed herein to provide an understanding of the potential and flexibility of these experimental systems. Instruments and engineering technology for space applications could take advantage of our environment-simulation chambers for sensor calibration. Our systems also provide the opportunity to gain a greater understanding of the chemical reactivity of molecules on surfaces under different environments, thereby leading to a greater understanding of interface processes in prebiotic chemical reactions and facilitating studies of UV photostability and photochemistry on surfaces. Furthermore, the stability and presence of certain minerals on planetary surfaces and the potential habitability of microorganisms under various planetary environmental conditions can be studied using our apparatus. Therefore, these simulation chambers can address multiple different challenging and multidisciplinary astrobiological studies.The work performed at CAB was supported by the Instituto Nacional de Tecnica Aeroespacial and Ministerio de Economia y Competitividad (MINECO). We acknowledge funding through the Spanish research project MAT2010-17720. Thank you to PASC’s users to make possible such a wide range of astrobiological applications.We acknowledge support by the CSIC Open Access Publication Initiative through its Unit of Information Resources for Research (URICI)Peer reviewe

Analysis and adsorption-interaction of amino acids on basaltic mineral subjected to different simulated atmospheres

[EN] The research have been conducted in order to have a better understanding of amino acid adsorption on volcanic matrix surface subjected to different extreme environmental conditions (Martian surface environment, space environment, UV-environment, etc.) simulated by The Planetary Atmosphere and Surfaces Chamber (PASC) at the ”INTA-Centro de Astrobiogia”. The spectroscopic measurements were done by Raman and IR spectroscopy (at the Unidad Asociada Uva-CSIC at Centro de Astrobiología) taking into account the capabilities of the combined Raman-IR analyses for astrobiological target such as the detection of biomarkers on the future ESA-ExoMars Mission. Moreover, SEM-EDX analyses have been conducted in order to complement the spectroscopic results, which endeavour the use of spectroscopic systems for space missions. Conclusion: The L-aspartic acid shows to be the most suitable amino acid for this kind of experiment; the amino acid half–life is 104 seconds according to the reference; both spectroscopic techniques, working in synergy, have detected the amino acid degradation, but amino acid mineral interaction was not detected; the experiments have shown the versatility of the simulation chamber (PASC) to perform experiments under different planetary environments.[ES] Los experimentos se han realizado con el objectivo de tener un mejor entendimiento sobre aminoácidos inmovilizados sobre matrices de caracter volcánico y estos han sido sometidos a diferentes ambientes extremos (Ambiente marciano, ambiente espacial, ambiente de radiación UV, etc.) dentro de la Cámara de Simulación de atmosferas y superficies planetarias (PASC) en el Centro de Astrobiología- INTA. Los métodos espectroscópicos usados son la espectroscopía Raman e Infrarroja (en la Unidad Asociada Uva-CSIC al Centro de Astrobiología) teniendo en cuenta las capacidades combinadas de estos sistemas para objetivos astrobiológicos como la detección de biomarcadores en la futura misión ESAExoMars. Además, se realizaron medidas mediante microscopía electrónica (SEM-EDX) las cuales complementan los resultados espectroscópicos y refuerzan el uso de estos sistemas para misiones espaciales. Conclusiones: El ácido L-Aspartico demostró ser el más eficiente para este tipo de experimentos; la vida media de los aminoácido es de 104 teniendo en cuenta las referencias; ambos sistemas espectroscópicos Raman-IR, trabajando conjuntamente, detectaron la degradación de los aminoácidos, pero la interacción entre aminoácido-mineral no fue detectada; los experimentos demostraron la versatilidad de la Cámara de Simulación (PASC) en cuanto a la realizacion de experimentos en distintos ambientes planetarios.Peer reviewe

Spectroelectrochemical operando method for monitoring a phenothiazine electrografting process on amide functionalized C-nanodots/Au hybrid electrodes

Phenothiazine derivatives are extensively explored dye molecules, which present interesting electrochemical and optical properties. In recent years, the possibility of transforming some phenothiazines in their aryl diazonium salt derivatives has been proved, what allows them to be electrochemically reduced and electrografted onto conductive surfaces. This is a smart way to modify these surfaces and enable them with specific functionalities. In order to better comprehend the electrografting process and consequently have a higher control of it, in this work we have carried out an exhaustive study by operando UV–Vis spectroelectrochemistry of the electrografting of a phenothiazine aryl diazonium salt onto amide carbon nanodots. As a model of phenothiazine dye we have chosen Azure A. The electrografting onto carbon nanodots has been stablished by comparison with the results obtained on bare gold electrodes in this novel study. The presence of carbon dots improves the reversibility of the electrochemical process as derived from the results obtained by operando UV–Vis spectroelectrochemistry. In addition, to asses that the electrochemical process studied corresponds to the electrografting, the results have been compared to those obtained for the simple Azure A adsorption. This study shows the advantages of obtaining simultaneously the electrochemical and the spectroscopic evolution of an electron-transfer process in a single experiment, in a particular electrochemical reaction. This work could be the starting point for the study of the electrografting on other nanomaterialsFunding from the Spanish Ministerio de Ciencia, Innovación y Universidades (project: CTQ2017-84309-C2-1-R) and Comunidad Autónoma de Madrid (NANOAVANSENS Program) is acknowledged. IMDEA Nanociencia acknowledges support from the 'Severo Ochoa' Programme for Centres of Excellence in R&D (Ministerio de Ciencia, Innovación y Universidades, Grant SEV-2016-0686

Survival of Moss Reproductive Structures under Simulated Martian Environmental Conditions and Extreme Thermal Stress: Vibrational Spectroscopic Study and Astrobiological Implications

The principal goal of astrobiology is the search for extraterrestrial life forms. A key aspect is the study of the ability of different kinds of terrestrial organisms to support simulated extraterrestrial environmental conditions. Mosses are multicellular green plants, poorly studied from an astrobiological perspective. In this paper, we report experimental results obtained using two species of moss, which demonstrate that both the spores of the moss Funaria hygrometrica as well as the desiccated vegetative gametophyte shoots of the moss Tortella squarrosa (=Pleurochaete squarrosa) were capable of resisting Simulated Martian Environmental Conditions (SMEC): Mars simulated atmospheric composition 99.9% CO2, and 0.6% H2O with a pressure of 7 mbars, -73 ºC and UV irradiation of 30 mW cm-2 in a wavelength range of 200-400 nm under a limited short time of exposition of 2 hours. After being exposed to SMEC and then transferred to an appropriate growth medium, the F. hygrometrica spores germinated, producing typical gametophyte protonemal cells and leafy shoots. Likewise, detached leaves from SMEC-exposed gametophyte shoots of T. squarrosa retained the ability to produce new protonemata and shoots under suitable growth conditions. Furthermore, we studied the tolerance of these moss structures to a thermal stress of 100 °C for 1 h; in both cases the spores and shoots were capable of resisting this heat treatment. Our study using FT-Raman and FT-IR vibrational spectroscopy demonstrated that neither spores nor shoots apparently suffered significant damage in their biomolecular makeup after being subject to these stress treatments. The implications of these findings for the search of life on Mars are discussed

Home i natura a la Vall de Riells

Considerant l'absència d'estudis ambientals previs a la Vall de Riells (Bigues i Riells, Vallès Oriental), i l'evident necessitat de gestió de l'espai a causa de la sobrefreqüentació antròpica, s'ha realitzat aquesta diagnosi ambiental. En ella es descriuen de manera integrada els principals elements del medi físic, biòtic i socioeconòmic, per tal de proporcionar les eines necessàries per avaluar les problemàtiques de l'espai i fomentar la seva gestió i conservació.Considerando la ausencia de estudios ambientales previos en la Vall de Riells (Bigues i Riells, Vallès Oriental), y la evidente necesidad de gestión del espacio debido a la sobrefrecuentación antrópica, se ha realizado esta diagnosis ambiental. En ella se describen de forma integrada los principales elementos del medio físico, biótico y socioeconómico, para proporcionar las herramientas necesarias para evaluar las problemáticas del espacio y promover su gestión y conservación.As a result of the absence of previous environmental studies in Vall de Riells (Bigues i Riells, Vallès Oriental), and the evident need of management due to excessive anthropic presence, it has been realized this environmental diagnostic. It describes, in an integrated way, the main elements of geology, biology, economy and culture of Vall de Riells. This environmental analysis provides the necessary tools for the evaluation and the management of the space

Azure A embedded in carbon dots as NADH electrocatalyst: Development of a glutamate electrochemical biosensor

Carbon nanodots modified with azure A (AA-CDs) have been synthesized and applied as redox mediator of bioelectrocatalytic reactions. A deep characterization of AA-CDs nanomaterial has been carried out, proving the covalent attachment of azure A molecules into the carbon dots nanostructure. Disposable screen-printed carbon electrodes (SPCE) have been modified with AA-CDs, through the action of chitosan polymer (Chit-AA-CDs/SPCE). The Chit-AA-CDs/SPCE electrocatalytic activity towards the oxidation of NADH has been proved, obtaining excellent results regarding the low oxidation potential achieved (−0.15 V vs. Ag) and low detection and quantification limits (LOD and LOQ) for NADH, 16 and 53 µM, respectively. The developed electrochemical platform has been applied for the construction of a glutamate biosensor by immobilizing L-glutamic dehydrogenase (GLDH/Chit-AA-CDs/SPCE). The morphology of GLDH/Chit-AA-CDs/SPCE platform was analysed by AFM at each different step of the electrode modification process. The resulting biosensing platform is capable of detect NADH enzymatically generated by GLDH in the presence of glutamate and NAD+. Good analytical parameters were obtained for glutamate analysis using GLDH/Chit-AA-CDs/SPCE, as LOD and LOQ of 3.3 and 11 µM, respectively. The biosensor has been successfully applied to the analysis of food and biological samplesThis work has been supported by the Spanish Ministerio de Ciencia e Innovacion (PID2020–116728RB-I00) and Comunidad Autonoma de Madrid (SI3/PJI/2021–00341, P2018/NMT-4349 TRANSNANOAVANSENS Program

Carbon nanodots modified-electrode for peroxide-free cholesterol biosensing and biofuel cell design

The determination of cholesterol is greatly important because high concentrations of this biomarker are associated to heart disease. Moreover, cholesterol can be used as a fuel in enzymatic fuel cells operating under physiological conditions. Here, we present a cholesterol biosensor and a peroxide-free biofuel cell based on the electrocatalytic oxidation of the NADH generated during the enzymatic reaction of cholesterol dehydrogenase (ChDH) as an alternative to the H2O2 biosensing strategies used with cholesterol oxidase-bioelectrodes. Azure A functionalized-carbon nanodots were used as NADH oxidation electrocatalysts and for ChDH covalent immobilization. The biosensor responded linearly to cholesterol concentrations up to 1.7 mM with good sensitivity (4.50 mA cm−2 M−1) and at a low potential. The ChDH bioelectrode was combined with an O2-reducing bilirubin oxidase cathode to produce electrical energy using cholesterol as fuel and O2 as oxidant. Furthermore, the resulting enzymatic fuel cell was tested in human serum naturally containing free cholesterolA.L.DL. and M.P. thank MCIU/AEI/FEDER, EU for funding project RTI2018–095090-B-I00. M.B. acknowledges funding from the European Union’s Horizon 2020 Research and Innovation Program under the Marie Skłodowska-Curie grant agreement No. 713366. This work was also supported by Talent Attraction Project from CAM (SI3/PJI/ 2021–00341 and 2021–5A/BIO-20943), Spanish Ministerio de Ciencia e Innovacion (PID2020–116728RB-I00) and TRANSNANOAVANSENSCAM Program (S2018/NMT-4349

Rapid SARS-CoV-2 sensing through oxygen reduction reaction catalysed by Au@Pt/Au core@shell nanoparticles

The development of rapid, accurate, sensitive, and low-cost diagnostic methods for COVID-19 detection in real-time is the unique way to control infection sources and monitor illness progression. In this work, we propose an electrochemical biosensor for the rapid and accuracy diagnosis of COVID-19, through the determination of ORF1ab specific sequence. The biosensor is based on the immobilization of a thiolated sequence partially complementary (domain 1) to ORF1ab on gold screen-printed electrodes and the use of bifunctional Au@Pt/Au core@shell nanoparticles modified with a second thiolated sequence partially complementary to ORF1ab (domain 2) as electrochemical indicator of the hybridization of DNA sequences. The synthesized Au@Pt/Au nanoparticles consist of an Au core, a shell of Pt (Au@Pt NPs), that provides an excellent electrocatalytic activity toward the oxygen reduction reaction (ORR) even after formation of hybrid biomaterials by modification, through the Au protuberances growth on the NPs surface, with an oligonucleotide with recognition ability. The ORR electrochemical activity, enhanced by the label element (Au@Pt/Au NPs), has been employed, for the first time, as indicator of the hybridization event. Based on this strategy, target sequences of the SARS-CoV-2 virus have been detected with a detection limit of 32 pM. The selectivity of the biosensor was confirmed by analysing ORF1ab sequence in the presence of DNA sequences from other viruses. The biosensor has been successfully applied to the direct detection of the virus in non-amplified samples of nasopharyngeal swabs from infected and non-infected patients. Results compare well with those obtained through RT-qPCR but our method is more rapid since does not need any amplification processPID2020-116728RB-I00, PID2020-115204RB-I00, PID2022-140180OB-C22, PID2022-142262OA-I00, TED2021-129738B–I00, RED2022-134120-T, S2018/NMT-4349 TRANSNANOAVANSENS-CM, SI3/PJI/2021–0034

Constraining the preservation of organic compounds in Mars analog nontronites after exposure to acid and alkaline fluids

The presence of organic matter in lacustrine mudstone sediments at Gale crater was revealed by the Mars Science Laboratory Curiosity rover, which also identified smectite clay minerals. Analogue experiments on phyllosilicates formed under low temperature aqueous conditons have illustrated that these are excellent reservoirs to host organic compounds against the harsh surface conditions of Mars. Here, we evaluate whether the capacity of smectites to preserve organic compounds can be influenced by a short exposure to different diagenetic fluids. We analyzed the stability of glycine embedded within nontronite samples previously exposed to either acidic or alkaline fluids (hereafter referred to as “treated nontronites”) under Mars-like surface conditions. Analyses performed using multiple techniques showed higher photodegradation of glycine in the acid-treated nontronite, triggered by decarboxylation and deamination processes. In constrast, our experiments showed that glycine molecules were preferably incorporated by ion exchange in the interlayer region of the alkali-treated nontronite, conferring them a better protection against the external conditions. Our results demonstrate that smectite previously exposed to fluids with different pH values influences how glycine is adsorbed into their interlayer regions, affecting their potential for preservation of organic compounds under contemporary Mars surface conditionsEuropean Commission | Ref. FP7 n. 307496European Commission | Ref. H2020 n. 818602Ministerio de Economía | Ref. MDM-2017-0737Ministerio de Economía | Ref. ESP2017-89053-C2-1-