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Water & Ice

Ice in the coldest places in the solar system

The Moon looks bone dry, but its poles hide craters that have not seen sunlight for billions of years, and some of them hold water ice. Here is how we found it and why every space agency wants it.

Mosaic of the Moon's south pole from above, with many craters whose floors stay in permanent shadow

NASA/GSFC/Arizona State University, LRO Wide Angle Camera (PIA13523). Public domain.

Craters where the Sun never shines

Earth's spin axis is tilted 23.4°, which gives us seasons. The Moon's axis is tilted only about 1.5° to its path around the Sun. So near the lunar poles the Sun always skims the horizon, and the floors of deep craters stay in shadow all year round, for billions of years.

These permanently shadowed regions (PSRs) are among the coldest places measured anywhere in the solar system. NASA's Lunar Reconnaissance Orbiter (LRO) has measured temperatures below about −240 °C (around 30 kelvin) on some crater floors near the poles, colder than the surface of Pluto.

At those temperatures, water molecules that wander in, from comet and asteroid impacts, volcanic gases or the solar wind reacting with the soil, freeze and stay put. The craters are cold traps.

Famous examples near the south pole include Shackleton, Cabeus, Haworth and Faustini. Near the north pole, Hermite holds the record for the coldest temperature measured on the Moon.

Illustration of frost in the floor of a permanently shadowed crater, lit faintly by a sunlit rim
AI-generated illustrationWhat it might be like on the floor of a permanently shadowed crater: lit only by light bounced from a sunlit rim far above.AI-generated illustration for BotBuhdy.

How we found water on the Moon

When Apollo samples came back bone dry in the 1970s, most scientists concluded the Moon had no water at all. That changed slowly, clue by clue:

Two views of the Moon side by side: a grey brightness map, and a dark map where blue colour marks the water and hydroxyl signal, strongest near the poles
Moon Mineralogy Mapper data: a normal brightness map (left) and the water and hydroxyl signal (right, blue), strongest near the poles.ISRO/NASA/JPL-Caltech/Brown Univ./USGS, Moon Mineralogy Mapper on Chandrayaan-1 (PIA12235), 2009.
Illustration of a plume of dust and ice rising from a dark polar crater after the LCROSS impact
AI-generated illustrationThe LCROSS impact in Cabeus crater threw a plume of dust and ice into sunlight, where instruments could measure it.AI-generated illustration for BotBuhdy.

Why lunar ice matters

Water is heavy and expensive to launch from Earth: every kilogram sent to the Moon costs a fortune. Finding it there changes what is possible:

  • Drinking water and water for growing food.
  • Oxygen to breathe, split from water with electricity from solar panels.
  • Rocket fuel: water can be split into hydrogen and oxygen, the same propellants many rockets burn. A lunar "filling station" could make deep-space missions cheaper.
  • Radiation shielding: water is good at blocking radiation around habitats.
  • Science: the ice is a frozen record of where the inner solar system's water came from, layer by layer over billions of years.

That is why the lunar south pole is the target for NASA's Artemis landings, India's Chandrayaan-3, China's Chang'e 7 and several private landers. See Future on the Moon for how it might be mined.

An engineer crouching on simulated grey lunar soil beside a test version of the VIPER rover in a slope laboratory
A test version of NASA's VIPER rover in a slope laboratory. VIPER was built to drive into shadowed areas and map the ice.NASA Glenn Research Center (GRC-2022-C-04467), VIPER mobility tests, 2022. Public domain.

What we still don't know

To work in the dark craters, NASA built ShadowCam, a super-sensitive camera on Korea's Danuri orbiter. Since 2023 it has been photographing the inside of permanently shadowed craters using the faint light reflected off nearby crater walls.

Quick answers

Is there water on the Moon?

Yes, but not liquid water. There is water ice in permanently shadowed craters near the poles, and tiny amounts of water and hydroxyl bound in soil and glass beads across the surface.

How was water ice found on the Moon?

Step by step: hydrogen detected by Lunar Prospector (1998), water signals from the Moon Mineralogy Mapper on India's Chandrayaan-1 (2009), and NASA's LCROSS impact into Cabeus crater in October 2009, which threw up a plume containing water.

Why is the lunar south pole important?

Because its permanently shadowed craters hold water ice, and nearby crater rims get sunlight for most of the year, ideal for solar power. That combination makes it the top target for future bases.

How cold are the shadowed craters?

Some are below about minus 240 degrees Celsius (around 30 kelvin), colder than the surface of Pluto.

Could astronauts drink Moon water?

In principle yes, after the ice is dug up, melted and cleaned of dust and other chemicals. Testing how easy that is remains a key goal of future missions.

Sources and credits

  1. NASA Science, Water on the Moon.
  2. Colaprete, A. et al. (2010), Detection of water in the LCROSS ejecta plume, Science 330, 463–468.
  3. Pieters, C. M. et al. (2009), Character and spatial distribution of OH/H2O on the surface of the Moon seen by M3 on Chandrayaan-1, Science 326, 568–572.
  4. Li, S. et al. (2018), Direct evidence of surface exposed water ice in the lunar polar regions, PNAS 115, 8907–8912.
  5. Honniball, C. I. et al. (2020), Molecular water detected on the sunlit Moon by SOFIA, Nature Astronomy 5, 121–127.
  6. He, H. et al. (2023), A solar wind-derived water reservoir on the Moon hosted by impact glass beads, Nature Geoscience 16, 294–300.
  7. NASA, LROC, Diviner and ShadowCam mission pages.

Photos credited to NASA, NOAA and other public-domain sources are used with thanks; BotBuhdy adds a small botbuhdy.com mark. Pictures labelled AI-generated illustration are artist-style illustrations made for this page, not photographs.