Discovery of water in lunar samples and on the lunar surface has opened a new chapter in lunar exploration. In addition to their potential utility, water and other volatile compounds can record a vast amount of information about the evolution of the Moon and migration of material throughout the Solar System. This chapter centers on volatile species (H2O, OH, CO2, Ar, etc.) identified and theorized in the upper microns to meters of the lunar surface. While volatiles are generally thought of as residing within the cold, permanently shadowed regions (PSR) near the lunar poles, volatiles also...

You do not have access to this content, please speak to your institutional administrator if you feel you should have access.