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Humans are returning to the moon and understanding the toxicity of lunar dust is crucial for successful missions. Apollo mission reports suggest that lunar dust poses significant inhalation risks. Previous studies on lunar dust simulants have shown tissue and cellular damage in the lungs. This study focuses on two new simulants, LMS-1 and LHS-1, which closely replicate the lunar dust of the mare and highland regions of the moon. BEAS-2B and A549 cells were treated with unprocessed LMS-1 and LHS-1 (100µg/ml, 1000µg/ml and 5000µg/ml). The simulants were processed to isolate particles ≤2.5 µm, allowing a direct comparison to Earth dust (airborne particulate matter). BEAS-2B and A549 cells were treated with processed simulants and Earth dust (10µg/ml, 50µg/ml, and 100µg/ml) for 48 and 72 h. Inflammation was measured by measuring IL-6 and IL-8 using ELISA and cell viability was measured using a trypan blue exclusion test. A time- and dose-dependent increase in IL-8 and IL-6 production by LMS-1 and LHS-1 exposure was found only in BEAS-2B cells. A dose-dependent decrease in cell viability was found in both BEAS-2B and A549 cells with lunar dust simulant exposure. Particles ≤2.5 µms cause greater cell death than particles ≤1000µm. However, Earth dust induced greater cytokine release and was more toxic than lunar dust simulants. Lunar dust simulants did not increase SOD2 gene expression, indicating no increases in oxidative stress in either cell type. Therefore, our results suggest that lunar dust simulants are not highly toxic dusts, but rather a physical irritant. Future studies are needed to confirm the relative toxicity and irritant capacity of other lunar regions simulants.
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http://dx.doi.org/10.1016/j.lssr.2025.02.005 | DOI Listing |
Life Sci Space Res (Amst)
August 2025
Texas A&M School of Engineering Medicine, Bryan, TX, United States; Department of Ophthalmology, Baylor College of Medicine, Houston, TX, United States; Department of Ophthalmology, University of Texas Medical Branch, Galveston, TX, United States; Department of Ophthalmology, Blanton Eye Institute,
Ocular health is critical for overall astronaut health requirements given its essential role for mission performance and safety. The ocular surface is a vital structure to the visual system and is essential for ocular protection and the refraction of light for focused vision. Data from the 2024 NASA Lifetime Surveillance of Astronaut Health identified that Space Shuttle and International Space Station (ISS) astronauts (N = 257) queried during post-flight eye exams reported symptoms of eye irritation (34 %), dry eyes (14 %), and foreign body sensation (21 %).
View Article and Find Full Text PDFACS Appl Polym Mater
July 2025
School of Materials Science and Engineering, Georgia Institute of Technology, Atlanta, Georgia 30322, United States.
There is a critical need for new technologies to support lunar and Martian exploration efforts, particularly for flexible, durable, and environmentally stable materials that can weather challenging space conditions. Electrically conductive thin films are critical for numerous applications, including structural health monitoring, charge dissipation, micrometeoroid and orbital debris impact detection, and electrodynamic dust shielding. Surface-localized nanocomposites (SLNCs) offer a promising alternative to metallic and ceramic films as flexible, durable, thin film conductors.
View Article and Find Full Text PDFNat Commun
July 2025
Department of Mechanical Engineering, Johns Hopkins University, Baltimore, MD, USA.
From the crewed Apollo missions to the recent Chinese Chang'e landings, the interaction between spacecraft exhaust plumes and lunar soil produces dusty clouds with high-speed particle ejection. Despite varying landing sites, remarkably stable streak patterns were observed, raising questions about their origin. We solved this puzzle by showing that these patterns were driven by Görtler instability from the curved compressed shear layer of the supersonic but surprisingly laminar jet.
View Article and Find Full Text PDFNature
July 2025
California Institute of Technology, Pasadena, CA, USA.
Young exoplanets provide an important link between understanding planet formation and atmospheric evolution. Direct imaging spectroscopy allows us to infer the properties of young, wide-orbit, giant planets with high signal-to-noise ratio. This allows us to compare this young population with exoplanets characterized by transmission spectroscopy, which has indirectly revealed the presence of clouds, photochemistry and a diversity of atmospheric compositions.
View Article and Find Full Text PDFLangmuir
June 2025
School of Aerospace Engineering, Huazhong University of Science and Technology, Wuhan 430074, China.
To understand and prevent the toxic effects of lunar dust on astronauts' health in future manned lunar exploration missions, the translocation characteristics of paired nonspherical silica nanoparticles (P-NS-SiNPs) across a pulmonary surfactant (PS) monolayer are studied using a coarse-grained molecular dynamics method considering both ellipsoidal and cubic SiNPs with/without bugles. The key findings are as follows: (1) Compared with an individual SiNP, the translocation times for 4 and 6 nm ellipsoidal P-SiNPs decrease by 25-50% and 7.7-30.
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