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Artemis II and the invisible hazard on the way to the Moon

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Why This Matters

The Artemis II mission marks a pivotal step in human space exploration by providing critical data on space radiation exposure, which is essential for ensuring astronaut safety on future lunar and Mars missions. Understanding and mitigating radiation risks will influence spacecraft design, mission planning, and long-term human presence beyond Earth. This mission's findings will shape the future of deep-space travel, benefiting both the tech industry developing space habitats and consumers interested in sustainable space exploration.

Key Takeaways

The most important data from NASA’s first crewed Artemis II mission may not be its photographs, but the radiation measurements that will shape how humans work and survive beyond travel farther from Earth’s magnetic shelter safely.

Artemis II science operations will lay the foundation for safe and efficient human exploration of the Moon and Mars.

The investigations will encompass human health, lunar science, CubeSats, Science Operations and Space weather.

Caption: “Hello, World.” Commander Reid Wiseman, Nikon D5, mission day one. The Sun is hidden behind Earth, and the globe is lit mainly by moonlight from the nearly full Moon behind the spacecraft. Around both poles the faint green auroras are visible, where electrons guided by Earth’s magnetic field excite oxygen high in the atmosphere. Hugging the day–night boundary is a razor-thin glowing shell: the upper atmosphere seen edge-on, its airglow (including light from a narrow sodium layer around 80–100 km up) intensified into a bright band. Stretching away from Earth is a soft triangular wedge of zodiacal light, produced as sunlight scatters off interplanetary dust from comets and asteroids that orbit the Sun. Down in the lower right, we can even spot Venus, shining as a brilliant spot against the dark of space. Credit: NASA/Reid Wiseman

One of ANSTO's radiation dosimetry experts, Dr Mitra Safavi Naeini (pictured left) explored the approach undertaken by NASA.

When NASA launched Artemis II on 1 April 2026, sending Reid Wiseman, Victor Glover, Christina Koch and Jeremy Hansen on a 10-day lunar flyby, it sent humans beyond low Earth orbit and back into the deep-space radiation environment for the first time since the Apollo program.

Radiation is one of the mission’s core scientific and operational questions. Along with four astronauts went cabin monitors, crew-worn dosimeters, an upgraded German heavy-ion detector, organ chits, saliva and blood sampling, and performance studies. The flight is testing the Orion and the Space Launch System with a crew aboard, but it is also characterising the radiation field inside the spacecraft, measuring how that environment field changes with trajectory and shielding, and linking those physical measurements to biomarkers, performance data and biological experiments.

The radiation environment

The first thing to get right is that 'radiation level' is not a single number. Beyond Earth orbit, astronauts face three overlapping hazards: trapped particles in the Van Allen belts, solar particle events from the Sun, and galactic cosmic rays from outside the solar system. The belts are intense but brief—the spacecraft crosses them quickly. Solar particle events are intermittent and operationally urgent; they can raise dose rates sharply over hours. Galactic cosmic rays are the chronic background: a low-dose-rate field of very high-energy particles, mostly protons but also heavy ions, present all the time and notoriously difficult to shield against.

NASA astronaut Christina Koch reads on a tablet in the dimly lit Orion crew capsule in this April 3, 2026, photo. To the right of the image’s center, CSA (Canadian Space Agency) astronaut Jeremy Hansen is seen in profile peering out of one of Orion’s windows. Lights are turned off to avoid glare on the windows. Credit: NASA

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