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Crewed Missions to Mars: Modeling the Impact of Astrophysical Charged Particles on Astronauts and Their Health

1 Pith paper cite this work, alongside 1 external citations. Polarity classification is still indexing.

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abstract

The impact of exposure to astrophysical ionizing radiation on astronaut health is one of the main concerns in planning crewed missions to Mars. Astronauts will be exposed to energetic charged particles from Galactic and Solar origin for a prolonged period with little protection from a thin spacecraft shield in transit and from the rarefied Martian atmosphere when on the surface. Adverse impacts on astronaut health include, for example, Acute Radiation Syndrome, damage to the nervous system, and increased cancer risk. We rely on medical studies to assess the impact of enhanced radiation dose levels on various physiological systems and the overall health of astronauts. Using a combination of radiation measurements and numerical modeling with the GEANT4 package, we calculate the distribution of radiation dose in various human body organs for various expected scenarios simulated with a model human phantom. We suggest mitigation strategies, such as improved ways of shielding and dietary supplements, and make recommendations for the safety of astronauts in future crewed missions to Mars.

fields

astro-ph.EP 1

years

2026 1

verdicts

UNVERDICTED 1

representative citing papers

Stellar impact on exoplanetary atmospheric evolution and habitability

astro-ph.EP · 2026-07-29 · unverdicted · novelty 2.0

An expert review asserting that exoplanet habitability is set by the star's full evolutionary history — XUV fluence, spin-down, wind, particles — plus planetary outgassing and magnetic history, not by today's insolation.

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Showing 1 of 1 citing paper.

  • Stellar impact on exoplanetary atmospheric evolution and habitability astro-ph.EP · 2026-07-29 · unverdicted · none · ref 63 · internal anchor

    An expert review asserting that exoplanet habitability is set by the star's full evolutionary history — XUV fluence, spin-down, wind, particles — plus planetary outgassing and magnetic history, not by today's insolation.