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Background: On a future lunar habitat, acquiring needed resources in situ will inevitably come from the Lunar regolith. Biomining, i.e. the use of microorganisms to extract metals from the regolith, is sustainable and energy-efficient, making it highly promising for space exploration applications. Given the extensive use of filamentous fungi in industrial biotechnology, we investigated the ability of the fungus Penicillium simplicissimum to extract metals from the European Astronaut Centre lunar regolith simulant 1 (EAC-1 A), which will be used as the analogue soil at the European Lunar Exploration Laboratory (LUNA) facility at the European Space Agency (ESA) and German Aerospace Centre (DLR) site.
Results: Biocompatibility tests demonstrated P. simplicissimum tolerance to high concentrations of EAC-1 A lunar regolith simulant (up to 60%), both on Earth gravity and Lunar simulated gravity via clinorotation. We reveal that a fungal bioleaching setup using low nutrient medium (20% PDB) enables P. simplicissimum to extract metals from EAC-1 A regolith over the course of 2 weeks at room temperature. Inductively coupled plasma mass spectrometry (ICP-MS) analysis of the leachate revealed the extraction of magnesium (up to 159 mg/L), calcium (151 mg/L), iron (68 mg/L), aluminium (32 mg/L), manganese (3 mg/L) as well as traces of titanium (0.02 mg/L). The recovered metal oxide powder from the leachate, obtained via centrifugation (14,500 g, 4,000 rpm), followed by filtration (0.22 μm) and drying at 60 °C overnight, achieved a promising average of 10 ± 3 g/L. Further analysis via SEM/EDS and XRD confirmed the presence of aluminium [as boehmite (AlO(OH))], magnesium, and iron [possibly as haematite (FeO)] and magnetite [possibly as (FeO)].
Conclusion: Our study demonstrates successful fungal biomining of lunar regolith simulant EAC-1 A and emphasizes the utilization of fungal-based approaches as promising ISRU technologies in future space exploration missions.
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http://dx.doi.org/10.1186/s40694-025-00201-z | DOI Listing |
Research (Wash D C)
July 2025
China Academy of Space Technology, Beijing 100094, P. R. China.
Water extraction from lunar regolith is one of the critical techniques for in situ resource utilization on the Moon. Traditional conductive heating methods show low efficiencies for massive water production from lunar regolith due to the low heat conductivity of lunar regolith and the inherent harsh lunar environment. To enhance the effectiveness of massive water production and reduce energy cost, microwave heating method is used in this study to extract water from icy lunar regolith at an initial cryogenic temperature of -80 °C.
View Article and Find Full Text PDFCommun Earth Environ
July 2025
Institute of Applied Physics, TU Wien, Vienna, Austria.
Important aspects concerning the origin and formation of the Moon's exosphere, its tenuous gas envelope, remain puzzling with uncertainties regarding the importance of different effects. Two competing processes - micrometeoroid impact vaporization and solar wind ion sputtering - are considered key contributors to the ejection of particles into the exosphere. Here we present direct, high-precision yield measurements of solar wind ion sputtering using real lunar samples (Apollo 16 sample 68501), combined with advanced 3D simulations of regolith erosion.
View Article and Find Full Text PDFSci Rep
July 2025
Brunel University London, Kingston Lane, Bragg Building 015, London, UB8 3PH, England, UK.
The prospect of establishing a human presence on the Moon has transitioned from the realm of science fiction to an achievable goal. The long-term objective of the Artemis program is to establish a habitat on the Moon that would enable crews to remain on the lunar surface for extended periods. The developmental pathway for such facilities culminates in structures that are manufactured and constructed predominantly from materials sourced on the lunar surface, in alignment with the In-Situ Resource Utilization (ISRU) concept.
View Article and Find Full Text PDFACS Sens
June 2025
Anhui Institute of Optics Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, P. R. China.
Distinguishing the origin of lunar water ice requires in situ isotopic measurements with high sensitivity and robustness under extreme lunar conditions; however, challenges such as uncertain water contents and isotopic fractionation induced by regolith particles restrict isotopic analysis. Herein, we present a miniaturized tunable diode laser absorption spectrometer (TDLAS) developed as the core prototype for the Chang'E-7 Lunar Soil Water Molecule Analyzer (LSWMA). The wavelength range of the instrument is 3659.
View Article and Find Full Text PDFMaterials (Basel)
May 2025
Faculty of Materials Science and Engineering, Warsaw University of Technology, Wołoska 141, 02-507 Warsaw, Poland.
This paper concerns the assessment of the lunar regolith ability to consolidate in the presence of liquid water and develop and sustain cohesion after drying. This type of cohesion originates from interparticle adhesion and can be potentially improved through grading modification. The research was conducted using the lunar regolith simulant (EAC-1A) reproducing the PSD of real lunar soil delivered from the Moon.
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