Space radiation measurements during the Artemis I lunar mission.
basic_science · Level V
Where this comes from
- Record sourced from PubMed, PMID 39294379.
- Also identified by DOI 10.1038/s41586-024-07927-7 and PMC identifier 11446838.
- Licence recorded as CC BY.
- The licence permits redistribution, so the abstract is shown in full and the full text is available from the publisher.
Abstract
Space radiation is a notable hazard for long-duration human spaceflight<sup>1</sup>. Associated risks include cancer, cataracts, degenerative diseases<sup>2</sup> and tissue reactions from large, acute exposures<sup>3</sup>. Space radiation originates from diverse sources, including galactic cosmic rays<sup>4</sup>, trapped-particle (Van Allen) belts<sup>5</sup> and solar-particle events<sup>6</sup>. Previous radiation data are from the International Space Station and the Space Shuttle in low-Earth orbit protected by heavy shielding and Earth's magnetic field<sup>7,8</sup> and lightly shielded interplanetary robotic probes such as Mars Science Laboratory and Lunar Reconnaissance Orbiter<sup>9,10</sup>. Limited data from the Apollo missions<sup>11-13</sup> and ground measurements with substantial caveats are also available<sup>14</sup>. Here we report radiation measurements from the heavily shielded Orion spacecraft on the uncrewed Artemis I lunar mission. At differing shielding locations inside the vehicle, a fourfold difference in dose rates was observed during proton-belt passes that are similar to large, reference solar-particle events. Interplanetary cosmic-ray dose equivalent rates in Orion were as much as 60% lower than previous observations<sup>9</sup>. Furthermore, a change in orientation of the spacecraft during the proton-belt transit resulted in a reduction of radiation dose rates of around 50%. These measurements validate the Orion for future crewed exploration and inform future human spaceflight mission design.
Medical subject headings
- Cosmic Radiation
- Moon
- Radiation Monitoring
- Space Flight
- Spacecraft