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The aim of this study was to evaluate the potential of 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. This acidic medium is ideal for bioleaching, a process that employs acidolysis and complexolysis to extract metals from rocks. Additionally, the strain synthesized siderophores, molecules capable of mobilizing metals from solid matrices, as verified by the blue CAS colorimetric test. The secretion of siderophores in the culture medium proved advantageous for biomining. The siderophores facilitated the leaching of metal ions, such as manganese, from the rock matrix into the acidified water solution. In addition, the susceptibility of the Martian regolith simulant to the biomining process was assessed by determining the particle size distribution, acid composition after treatment, and geochemical composition of the rock. Although the preliminary results demonstrate successful manganese extraction, further research is required to optimize the extraction technique. To conclude, the strain exhibits promising abilities in extracting metals from rocks through biomining. Its use could prove useful in future in situ mining operations and environmental remediation efforts. Further research is required to optimize the process and evaluate its feasibility on a larger scale.
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http://dx.doi.org/10.3390/jof9100976 | DOI Listing |
NPJ Microgravity
August 2025
Advanced Ceramics, University of Bremen, Bremen, Germany.
The long-term goal of establishing a sustained human presence on Mars requires the capacity to produce essential consumables on-site. To this end, we develop strategies for processing inorganic oxidic powders and biomass into highly particle-filled composites using direct ink writing (DIW) 3D printing. Our approach relies on a simulant of a Martian regolith unit rich in hydrated clay minerals and food-grade spirulina, used as proxies for local regolith and cyanobacterial biomass, respectively.
View Article and Find Full Text PDFPNAS Nexus
August 2025
Department of Biological and Environmental Engineering, College of Agriculture and Life Sciences, Cornell University, Ithaca, NY 14853, USA.
Clay minerals are well documented to facilitate the retention of water and organic matter in terrestrial soils, Martian regolith, and meteorites. Yet, the mechanisms underlying water trapping within these mineral-organic matter associations are poorly understood. Here, we investigate these mechanisms with montmorillonite, a smectite clay, populated with carbohydrates of different structures.
View Article and Find Full Text PDFEnviron Res
July 2025
Dept. of Biotechnology, Univ. of Verona, Italy.
The poor fertility of Martian regolith, due to its lack of organic matter (OM) and nitrogen (N), limits its suitability as a plant substrate. While compost amendment enhances short-term fertility, the mechanisms underlying long-term OM stabilization, particularly through interactions with iron (Fe) minerals, remain poorly understood. This study explores OM fractionation and Fe mineral transformations in Mojave Mars Simulant (MMS-1), both pure (R100) and amended with compost (R70C30), across two consecutive cropping cycles (potato followed by Vicia faba).
View Article and Find Full Text PDFProg Earth Planet Sci
July 2025
CNES, 18 Avenue Edouard Belin, 31401 Toulouse, France.
IDEFIX, the Martian Moons eXploration (MMX) mission Phobos rover, will be the first of its kind to attempt wheeled-locomotion on a low-gravity surface. The IDEFIX WheelCams, two cameras placed on the underside of the rover looking at the rover wheels, provide a unique opportunity to study the surface properties of Phobos, regolith behaviour on small-bodies and rover mobility in low-gravity. The information gained about Phobos' surface will be of high importance to the landing and sampling operations of the main MMX spacecraft, in addition to being valuable for understanding the surface processes and geological history of Phobos.
View Article and Find Full Text PDFDermatology
July 2025
Dr. Phillip Frost Department of Dermatology and Cutaneous Surgery, University of Miami Miller School of Medicine, Miami, Florida, USA.
Background: The complex interplay of the Martian environment, equipment, and difficulties of delivering care presents unique challenges for dermatology.
Summary: In this review, we sought to provide an overview of dermatological challenges associated with future human exploration of the surface of Mars and provide information on preventative strategies and treatment methods. Sources relevant to Martian dermatology were collated from a PubMed and Google Scholar relevant to dermatological conditions associated with Martian exploration.