Mapping Water on the Moon and Mars using a Muon Tomograph

The search for water on the Lunar and Martian surfaces is a fundamental aspect of space exploration, contributing to the understanding of the history and evolution of these celestial bodies. However, the current understanding of the distribution, concentration, origin, and migration of water on these surfaces is limited. Moreover, there is a need for more detailed data on these aspects of Lunar and Martian water. The natural flux of cosmic-ray muons, capable of penetrating the planetary surface, offers a method to study the water-ice content, composition, and density of these surfaces. In this paper, the author presents a novel approach to address these knowledge gaps by employing cosmic-ray muon detectors and backscattered radiation. The study describes a cutting-edge muon tracking system developed by GScan and highlights the results of preliminary simulations conducted using GEANT4. These findings suggest that muon tomography could be a potential tool for investigating water-ice content on the Lunar and Martian surfaces, pointing to new avenues for space science exploration.