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81“…These findings improve our understanding of the limitations of microbial life in saline environments, which provides a basis for better evaluation of the habitability of extraterrestrial environments such as Martian cryobrines.…”
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82“…Here, we report the production of a polymer-based oxygen delivery system that supports the germination and growth of cress seeds (Lepidium sativum) in a martian regolith simulant under a martian atmosphere at 101 kPa. …”
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83“…Here, we make use of recent advances in the field of bioinspired chitinous manufacturing to develop a manufacturing technology to be used within the context of a minimal, artificial ecosystem that supports humans in a Martian environment.…”
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84por Katzer, Jacek, Suchocki, Czesław, Błaszczak-Bąk, Wioleta, Damięcka-Suchocka, Marzena“…In authors’ opinion quick, precise and remote measuring technique will be essential for successful development of lunar and Martian construction projects. One of such techniques is terrestrial laser scanning (TLS). …”
Publicado 2021
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85“…We demonstrate that Microbial Induced Calcite Precipitation (MICP) can be utilized for creation of consolidates of Martian Simulant Soil (MSS) and Lunar Simulant Soil (LSS) in the form of a ‘brick’. …”
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86por Ruan, Tao, Young, R. M. B., Lewis, S. R., Montabone, L., Valeanu, A., Read, P. L.“…A new dust data assimilation scheme has been developed for the UK version of the Laboratoire de Météorologie Dynamique Martian General Circulation Model. The Analysis Correction scheme (adapted from the UK Met Office) is applied with active dust lifting and transport to analyze measurements of temperature, and both column‐integrated dust optical depth (CIDO), τ ( ref ) (rescaled to a reference level), and layer‐integrated dust opacity (LIDO). …”
Publicado 2021
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87“…In this paper the concept for in-situ search of water in the Martian soil by applying neutron spectroscopy is examined. …”
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88“…On average, the Martian crust is 51–71 km thick with a southern crust thicker by 18–28 km than the northern one. …”
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89por Vezzola, Michele, Tosi, Solveig, Doria, Enrico, Bonazzi, Mattia, Alvaro, Matteo, Sanfilippo, Alessio“…The aim of this study was to evaluate the potential of Aspergillus tubingensis in extracting metals from rocks simulating Martian regolith through biomining. The results indicated that the fungal strain produced organic acids, particularly oxalic acid, in the first five days, leading to a rapid reduction in the pH of the culture medium. …”
Publicado 2023
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90“…Similar metabolic flexibility for Martian methanotrophs would mean that the same microbial groups could inhabit a diverse set of Martian mineralogical crustal environments. …”
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91“…Here, we present a comprehensive approach for creating robust, elastic, designer Lunar and Martian regolith simulant (LRS and MRS, respectively) architectures using ambient condition, extrusion-based 3D-printing of regolith simulant inks. …”
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92por Goesmann, Fred, Brinckerhoff, William B., Raulin, François, Goetz, Walter, Danell, Ryan M., Getty, Stephanie A., Siljeström, Sandra, Mißbach, Helge, Steininger, Harald, Arevalo, Ricardo D., Buch, Arnaud, Freissinet, Caroline, Grubisic, Andrej, Meierhenrich, Uwe J., Pinnick, Veronica T., Stalport, Fabien, Szopa, Cyril, Vago, Jorge L., Lindner, Robert, Schulte, Mitchell D., Brucato, John Robert, Glavin, Daniel P., Grand, Noel, Li, Xiang, van Amerom, Friso H. W.“…The Mars Organic Molecule Analyzer (MOMA) instrument onboard the ESA/Roscosmos ExoMars rover (to launch in July, 2020) will analyze volatile and refractory organic compounds in martian surface and subsurface sediments. In this study, we describe the design, current status of development, and analytical capabilities of the instrument. …”
Publicado 2017
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94por Borykov, Timur, Mège, Daniel, Mangeney, Anne, Richard, Patrick, Gurgurewicz, Joanna, Lucas, Antoine“…No distinguishable difference is observed between the behaviour of terrestrial and Martian landslides. ELECTRONIC SUPPLEMENTARY MATERIAL: The online version of this article (10.1007/s10346-019-01140-8) contains supplementary material, which is available to authorized users.…”
Publicado 2019
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95por Murri, Mara, Domeneghetti, Maria C., Fioretti, Anna M., Nestola, Fabrizio, Vetere, Francesco, Perugini, Diego, Pisello, Alessandro, Faccenda, Manuele, Alvaro, Matteo“…Due to its thickness and petrological similarities, the pyroxenitic layer of the 120m-thick magmatic pile Theo’s Flow (Archean Abitibi greenstone belt Ontario, Canada), has always been regarded as the terrestrial analogue for Martian nakhlites. However, its origin and cooling history and, as a consequence those of nakhlites, have always been a matter of vigorous debate. …”
Publicado 2019
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96“…However, global dust variability within a sol (Martian day) is still poorly understood. Although short-term dynamic processes are crucial, detailed comparisons of simulated diurnal variations are limited by relatively sparse observations. …”
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97por Semple, Carson, Riveros, Daniela, Nagy, Janice A., Rutkove, Seward B., Mortreux, Marie“…Therefore, we exposed adult female rats to 2 weeks of partial weight-bearing at either 100% of their normal loading (PWB100) or 40% of their normal loading (PWB40), corresponding to Martian gravity-analog, and assess muscle function, force and histomorphometry. …”
Publicado 2020
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98por Sobrado, Jesús Manuel“…We performed the simulations with the design and development of different tools that recreate Martian weather in the MARTE simulation chamber.…”
Publicado 2020
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99“…The Sun’s luminosity was ~30% lower 4 Ga ago; thus, most martian climate models struggle to elevate the mean surface temperature past the melting point of water. …”
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100por Harris, Rachel L., Schuerger, Andrew C., Wang, Wei, Tamama, Yuri, Garvin, Zachary K., Onstott, Tullis C.“…Observations of trace methane (CH(4)) in the Martian atmosphere are significant to the astrobiology community given the overwhelming contribution of biological methanogenesis to atmospheric CH(4) on Earth. …”
Publicado 2021
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