A recent study based on data from the Indian Space Research Organisation's (ISRO) Chandrayaan-2 mission has revealed compelling evidence of subsurface ice located beneath some of the coldest craters in the Moon's south polar region. Conducted by scientists from the Physical Research Laboratory in Ahmedabad, the research focused on nine doubly shadowed craters within Faustini, Haworth, and Shoemaker craters. Utilizing the Chandrayaan-2 orbiter's dual frequency synthetic aperture radar (DFSAR), researchers were able to capture detailed images of the lunar landscape. The findings suggest that these permanently shadowed regions (PSRs) maintain extremely low temperatures, around 25 K (-248°C), which are conducive to preserving water-ice over extended geological periods. This discovery holds significant implications for future lunar exploration, as the presence of ice could facilitate in-situ resource utilization, enabling astronauts to convert ice into drinking water, breathable oxygen, and rocket propellant. Such resources are vital for sustaining human life on the Moon and supporting long-term exploration missions.