How can there be ice on the Moon?


The Moon is about one-fourth the size of Earth. Credit: NASA

Curious Kids is a series for children of all ages. If you have a question you’d like an expert to answer, send it to curiouskidsus@theconversation.com.

“I have a question about ice on the Moon. How is this possible?”

— Olaf, age 9, Hillsborough, North Carolina

We’re lucky to live on a water world. More than 70% of the Earth’s surface is covered in water.

Earth is about 94 million miles from the Sun. That’s within the Goldilocks zone: the place in our solar system where a planet has just the right temperature for water to exist in oceans and rivers as a liquid and as ice in the north and south poles.

Earth also has an atmosphere more than 6,000 miles (9,650 kilometers) thick that’s filled with oxygen for us to breathe. This atmosphere, along with a huge magnet in the center of the Earth, helps protect us from the Sun’s harmful radiation, mostly solar wind and cosmic rays.

But the Moon hardly looks like a water world, or even a place with a few puddles. It has a worn-out internal magnet and an atmosphere so weak it’s virtually a vacuum. There are no clouds or rain or snow, just a sky that’s only the blackness of space, with a surface baked by the Sun. The Moon’s temperature reaches 273 degrees Fahrenheit (134 Celsius) by day and goes as low as -243 F (-153 C) at night.

But as scientists who study space and work to develop technologies that look for the water, we can definitively say: Yes, the Moon has water.

The discovery

For a long time, astronomers and other scientists thought Moon water was unlikely. After all, the Apollo astronauts brought back many rock samples from the Moon, and all were dry, with no detectable water.

But visits by recent spacecraft showed that some water is there. In 2009, NASA smashed a spacecraft – the Lunar Crater Observation and Sensing Satellite, or LCROSS – into the Moon’s surface, inside Cabeus crater. When that happened, water ice was ejected.

This confirmed to scientists that water ice was in the bottom of the craters. But determining how much water is there will be difficult. The 10,000 or so Moon craters are essentially big holes, with areas so shaded the Sun never shines inside. These places are really cold, well under -300 F (-184 C). Once these frozen water molecules get stuck in the craters, they pretty much stay forever, unless some heat or energy dislodges them. They are unlikely to naturally evaporate or sublimate as vapor – it’s just too cold in there.

But that doesn’t mean water is stored only in craters. In 2023, scientists using SOFIA, the Stratospheric Observatory for Infrared Astronomy, looked for water on the Moon’s surface in areas that were not as cold as the craters. And they found it – not on top of the soil, but probably inside the soil grains.

No one knows yet how much water the Moon has or how deep it goes. But one thing is certain: There’s much more than scientists first thought.

Water will be a critical need for astronauts living in Moon colonies. Credit: ESA/P. Carril

Comets and volcanoes

How did the Moon get its water? No one is certain yet, but there are some theories.

Eons ago, comets – which are basically frozen, dirty snowballs – crashed into Earth, leaving their comet water. That’s one of the ways Earth developed its oceans; perhaps that’s how the Moon got some of its water too.

Other scientists think ancient volcanoes on the Moon released water vapor when they erupted billions of years ago. Eventually, that vapor descended to the surface as frost. Over time, layers of that frost accumulated, particularly at the poles; much of it may have found its way inside lunar craters as ice.

Drinking water for astronauts

Water is heavy. Transporting it to the Moon by spacecraft would be costly. So it makes more sense for astronauts to figure out a way to use the water already on the Moon.

But Moon water is not drinkable as is; it would have small pieces of the lunar soil and possibly other molecules mixed with it. Astronauts living in Moon colonies would need to purify any water they collected. This is a tricky process that would require considerable effort and resources.

There is a plan to drill for the water and look for it, the way people hunted for underground gold during the 19th century gold rush. The analogy is not a bad one – water on the Moon might eventually be more valuable than gold on Earth.

And not just for drinking. Water, of course, is two parts hydrogen, one part oxygen; it can be split. This is a win-win: Astronauts can use the hydrogen for rocket fuel and the oxygen for breathable air. Using the Sun as a power source, the water splitting is probably doable.

Returning to the Moon and establishing a permanent base are enormous commitments requiring decades of work, billions of dollars, the cooperation of many nations, and many new technologies yet to be developed. But as the world enters this dramatic new chapter of space exploration, pioneers run the risk of destroying or polluting a unique environment that has been in existence for billions of years – and many scientists feel a deep obligation not to repeat the painful lesson we’re now learning here on Earth.

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This article is republished from The Conversation under a Creative Commons license.

Authors

  • Thomas Orlando

    Electron- and Photon-stimulated Interface and Surface Processes. Dr. Orlando's group utilizes state-of-the-art ultra-high vacuum (UHV) surface science systems equipped with UV-laser sources and low-energy electron beams to stimulate reactions (such as the production of hydrogen) on a variety of substrates and interfaces. Sensitive laser detection schemes (resonance-enhanced multiphoton ionization) are used to probe the reaction dynamics. Approaches based on quantum mechanical interference to control desorption and patterning of surfaces at the nano- and meso-scale are also being developed.

    Environmental Chemistry and Planetary Surface Science. Water is ubiquitous in terrestrial and planetary atmospheres and environments. Dr. Orlando's group studies "wet" interfaces using nanoscale films of ice grown in UHV. Radical and ion-molecule reactions are then initiated using electron- and photon-beam sources. These experiments are relevant to understanding the photochemistry of stratospheric cloud particles and magnetospheric processing of icy satellite surfaces in the Jovian system.

    Biophysical Chemistry. The mechanisms of DNA damage and repair have been studied extensively, though the role intrinsic waters of hydration play in initiating damage have not been elucidated. Dr. Orlando's group will carry out electron- and photon-irradiation studies of DNA:water interfaces to examine the importance of direct vs. indirect damage.

  • Frances Rivera-Hernández

    Dr. Frances Rivera-Hernández runs the PLANETAS group at the Georgia Institute of Technology (Georgia Tech). She is an Assistant Professor in the School of Earth & Atmospheric Sciences and Co-director of Georgia Tech’s Astrobiology Program. She is also Deputy PI for the new NASA SSERVI center at Georgia Tech: Center for Lunar Environment and Volatile Exploration Research (CLEVER). Her research is focused on characterizing sedimentary deposits and landforms to help interpret present and past surface conditions and habitability on Earth, Mars, Moon, and beyond! Outside of research, she remains active in several outreach and informal education projects to encourage students from underrepresented communities to pursue STEM careers.

    She is a native of Aguas Buenas, Puerto Rico (¡Wepa!) and has been in love with science for as long as she can remember. When she is not sciencing, she enjoys spending time with her family, traveling and walking in new cities, learning new languages, cooking, and trying new restaurants.

  • Glenn Lightsey

    Dr. Glenn Lightsey is the director of the Space Systems Design Lab and director of the Center for Space Technology And Research at Georgia Tech. His research program focuses on the technology of small satellites, including: guidance, navigation, and control systems; attitude determination and control; formation flying, satellite swarms, and satellite networks; cooperative control; proximity operations and unmanned spacecraft rendezvous; space based Global Positioning System receivers; radionavigation; visual navigation; propulsion; satellite operations; and space systems engineering. Dr. Lightsey has authored and co-authored more than 140 technical articles and publications, including four book chapters. He is an AIAA Fellow and a Founding Member of the AIAA Small Satellite Technical Committee. He is Associate Editor-in-Chief of the Journal of Small Satellites. Dr. Lightsey was previously employed at the University of Texas at Austin and NASA’s Goddard Space Flight Center.

    Prior to joining the faculty at the Daniel Guggenheim School of Aerospace Engineering, Dr. Lightsey held the position of Fellow of the W. R. Woolrich Professor in Engineering in the Department of Aerospace Engineering and Engineering Mechanics at The University of Texas at Austin. He also held the title of University Distinguished Teaching Professor, a position designated to less than 5% of the tenured faculty at The University of Texas. In 2011, Dr. Lightsey received the American Society for Engineering Education's John Leland Atwood Award for outstanding aerospace engineering education, and the William David Blunk Memorial Professorship for outstanding undergraduate teaching at the University of Texas at Austin.

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