Sylvain Blunier , Dimitrios Athanasopoulos , Clemens Dittmar , Freja Thoresen , Aidan Cowley , Anna Fogtman
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引用次数: 0
Abstract
Protecting astronauts from radiation is a critical challenge for extended missions on the lunar surface. To mitigate the risks from Galactic Cosmic Rays (GCR) and solar flares, future habitats must be designed with robust shielding against these hazards. Utilizing lunar regolith presents a promising solution, offering effective radiation protection to avoid transporting heavy, prefabricated materials. In this work, we simulated a two-layer lunar dome made of a thin aluminum-based alloy as an inner layer and an outer layer made of lunar regolith. Combined with an advanced mesh-type computerized human phantom, these simulations give a detailed insight into the radiation exposure of astronauts in such habitats. Using the ICRU (International Commission on Radiation Units) sphere as a simplified human phantom we computed the dose equivalent (DE) as a function of the thickness of the outer layer using the BON2020 GCR model. The simulation was repeated at different thicknesses using the ICRP 145 computerized female human phantom to characterize the impact on individual organs. Our study introduces a novel model giving the DE and effective dose equivalent (EDE) exposure experienced by astronauts within a regolith-made lunar dome under GCR during solar minimum conditions, contingent upon the dome's wall thickness. Our comprehensive analysis reveals a decrease in EDE when stacking regolith until 45 g·cm-2. Until 105 g·cm-2, the production of secondary particles would potentially induce more dose than it would protect. We observe rapid attenuation of heavy ions within 45 g·cm-2 of regolith thickness, while the presence of secondary neutrons produced by the interaction of primary protons and alphas with the regolith increases the impact on radiation exposure. Notably, the EDE behind a shield comprised of only 1.136 g·cm-2 of aluminum measures 291 mSv·y-1 with a body-averaged mean quality factor of 3.3, whereas adding 45 g·cm-2 of regolith reduces this exposure to 213 mSv·y-1 and the quality factor to 2.2. Our investigation identifies the skin, breasts, brain, and surface bones as the organs most affected by radiation exposure, with comparable magnitudes of impact across all organs. These findings also underscore the importance of considering organ-specific effects when assessing radiation hazards in space environments.
期刊介绍:
Planetary and Space Science publishes original articles as well as short communications (letters). Ground-based and space-borne instrumentation and laboratory simulation of solar system processes are included. The following fields of planetary and solar system research are covered:
• Celestial mechanics, including dynamical evolution of the solar system, gravitational captures and resonances, relativistic effects, tracking and dynamics
• Cosmochemistry and origin, including all aspects of the formation and initial physical and chemical evolution of the solar system
• Terrestrial planets and satellites, including the physics of the interiors, geology and morphology of the surfaces, tectonics, mineralogy and dating
• Outer planets and satellites, including formation and evolution, remote sensing at all wavelengths and in situ measurements
• Planetary atmospheres, including formation and evolution, circulation and meteorology, boundary layers, remote sensing and laboratory simulation
• Planetary magnetospheres and ionospheres, including origin of magnetic fields, magnetospheric plasma and radiation belts, and their interaction with the sun, the solar wind and satellites
• Small bodies, dust and rings, including asteroids, comets and zodiacal light and their interaction with the solar radiation and the solar wind
• Exobiology, including origin of life, detection of planetary ecosystems and pre-biological phenomena in the solar system and laboratory simulations
• Extrasolar systems, including the detection and/or the detectability of exoplanets and planetary systems, their formation and evolution, the physical and chemical properties of the exoplanets
• History of planetary and space research