#NASA discovers the Moon is wet — now scientists want to go back

Understanding how much water is present, and its location, is also incredibly useful for planning human missions to the Moon and beyond. Water represents a key resource that can be used for life-support purposes – but it can also be split apart into its constituent elements and put to other uses. Oxygen could replenish air supplies, or be used in simple chemical reactions at the lunar surface to extract other useful resources from the regolith (soil composed of small grains). Water could also be used as rocket fuel in the form of liquid hydrogen and liquid oxygen.

This means that the Moon has great potential to become a refueling base for space missions further into the Solar System or beyond. Its lower gravity and lack of atmosphere means it would require less fuel to launch from there than from Earth. So when space agencies talk of in-situ resource utilization at the Moon, water is front and centre of their plans, making the new papers extremely exciting.

New research

Instruments on board various spacecraft have previously measured “reflectance spectra” (light broken down by wavelength) from the Moon. These detect light coming from a surface to measure how much energy it reflects at a specific wavelength. This will differ based on what the surface consists of. Because it has water, the Moon’s surface absorbs light at 3?m wavelengths (0.000003 meters). However, absorptions at this wavelength cannot distinguish between molecular water and hydroxyl compounds.

Using the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA) telescope, flown at 43,000 feet, the team behind one of the new papers observed sunlit sections of the Moon’s surface in wavelengths of 5-8?m. H₂O results in a characteristic peak in the spectrum at 6?m, and by comparing a near-equatorial area as a baseline (thought to have almost no water) with an area near the south pole, this study reports the first unequivocal observations of molecular water under ambient conditions at the lunar surface at an abundance of 100-400 parts per million.

This is several orders of magnitude too large for most of the water to be adsorbed onto regolith grain surfaces. Instead, the authors suggest that the water they have observed must be locked up inside glass formed by tiny meteorites impacting and melting already hydrated regolith grains. Alternatively, it could be present in voids between grain boundaries, which would make it easier to extract. Where exactly this water is sited would be of extreme interest for future explorers as it would dictate the processes and energy required to extract it.

Luckily, the other paper used new theoretical models, based on temperature data and higher resolution images from the Lunar Reconnaissance Orbiter, to refine predictions of where conditions are right for molecular water to be trapped as ice.

Previous research has shown already that there are such kilometers-wide “cold traps” in permanently shadowed areas near the poles, where water ice may be present. Evidence from orbiting spacecraft, however, was inconclusive about this being molecular water or hydroxyl. The new study finds that there are also abundant small cold traps where conditions permit water ice to accumulate – on the scale of centimeters or decimeters. In fact, such traps should be hundreds to thousands of times more numerous than larger cold traps.

The team calculates that 0.1% of the total lunar surface is cold enough to trap water as ice, and that the majority of these icy cold traps are at high latitudes (> 80°). This is particularly near to the lunar south pole, narrowing down the choice of future landing sites with the highest chance of finding trapped water ice. However, it is important to realize that the two studies investigated areas at different latitudes (55°-75°S vs >80°S) and therefore cannot be compared directly.

Nevertheless, these latest discoveries further enhance our understanding of the history of water on our nearest neighbor. They will undoubtedly strengthen plans for a return to the Moon. Instruments such as the European Space Agency’s (PROSPECT payload on Luna 27) will be able to make measurements on the Moon to “ground-truth” these tantalizing glimpses of the wealth of information yet to be discovered.

This article is republished from The Conversation  James Mortimer, Postdoctoral researcher in Planetary Science and Exploration, The Open University and Mahesh Anand, Professor of Planetary Science and Exploration, The Open University under a Creative Commons license. Read the original article.