
Moon Water Built Up Over Billions of Years, Not a One-Time Event
New analysis using NASA’s Lunar Reconnaissance Orbiter data shows that ice in permanently shadowed lunar craters accreted gradually over about 3 to 3.5 billion years from multiple sources—comet/asteroid deliveries, solar-wind interactions, and ancient volcanic activity—challenging the idea of a single Late Heavy Bombardment event. The oldest, most shadowed craters host the most ice, a result with strong implications for future Moon missions and in‑situ resource use, though direct sample analysis is needed to confirm the exact origins.











