Artistic concept of CoRaLS mission. Photo credit: A. Romero-Wolf, JPL |
A University of Hawaiʻi at Mānoa project to detect ice deposits below the surface of the Moon received a major boost from NASA. Five scientists in the Department of Physics and Astronomy and Hawaiʻi Institute of Geophysics and Planetology (HIGP) have been awarded a three-year, $2,945,704 grant to develop technology for the NASA Cosmic Ray Lunar Sounder (CoRaLS) mission, which was initiated by UH Mānoa and NASA’s Jet Propulsion Lab.
CoRaLS hopes to be the first mission to detect subsurface ice below the first meter, therefore having a unique opportunity to further lunar science and identify crucial resources for future manned and unmanned missions to the Moon.
History of ice deposits
Extensive ice deposits have been found in the permanently shadowed regions (PSRs) of Mercury, but so far only traces of ice have been found on the surface of lunar PSRs, and active radar measurements sensitive to the top meter or so of the regolith (5–10 meter layer of debris on the Moon’s surface) show no clear signal yet from extensive ice deposits.