Where’s the water? Two resource-hunting tools for the Moon’s surface
(11 March 2019 - NASA Ames) We already know that the Moon is a complex world full of familiar minerals and gases. It even holds reserves of water ice in some craters at its poles.
Measurements from spacecraft orbiting the Moon tell us there is also material spread across the lunar surface that could be more water or a closely related resource, hydroxyl. What those orbiters found is actually the element hydrogen, which could turn out to be in the form of water – the familiar H2O – or hydroxyl, which is just one hydrogen and one oxygen atom, or OH.
Two tools from NASA’s Ames Research Center, in California’s Silicon Valley, will be delivered to the Moon, perhaps as soon as 2020, to find out more. Through the Commercial Lunar Payload Services contract, commercial partners are building lunar landers to carry NASA experiments like these to the surface. The measurements taken on the lunar surface will help researchers understand what form the Moon’s hydrogen takes and how it behaves in the lunar environment.
The Neutron Spectrometer System
Sensing the amount of hydrogen around is the job of the Neutron Spectrometer System, or NSS. It can measure the total volume present, up to three feet below the surface. NSS works by measuring changes in the number and energy of particles called neutrons that are always coming from the Moon. When these tiny particles strike something that’s about their size – like a hydrogen atom – they lose a lot of their energy. That’s a change that NSS can detect and use to infer the presence of hydrogen.
Components of the Neutron Spectrometer System undergo testing on the vibration table. The blue cables are sensors that monitor the forces experienced by the instrument during the test. (courtesy: NASA)
The Near-Infrared Volatiles Spectrometer System
The second tool can’t see underground. Instead, the superpower of the Near-Infrared Volatiles Spectrometer System, or NIRVSS (pronounced “nervous”), is the ability to tell the nature of the hydrogen it encounters. It could belong to water molecules or to hydroxyl or just exist as hydrogen atoms – any of which could be a useful resource, for tasks such as making fuel for space exploration.
NIRVSS features a spectrometer, a device that looks at light emitted or absorbed by materials to help identify their composition. In the lunar soil, that will mean detecting the different types of minerals and ices present – including frozen carbon dioxide, ammonia and methane, scientists expect – and differentiating between water and hydroxyl. Two other instruments on NIRVSS will reveal the precise characteristics of the locations it studies. The Spectrometer Context Imager is like a broad-spectrum camera that yields a nine-color image revealing the composition of the soil in fine resolution. The Longwave Calibration Sensor gives surface temperature at very small scales.
The Near-Infrared Volatiles Spectrometer System, or NIRVSS, looks at light emitted or absorbed by materials to help identify their composition. When it is delivered to the Moon, NIRVSS will detect the different types of minerals and ices present in the soil, including water. (courtesy: NASA)
Does Moon Water Move?
Scientists also have big questions about the mobility of lunar water. This isn’t flowing liquid water, but individual water molecules. Heated by the energy of sunlight, they could be shot upward like tiny cannonballs, until gravity pulled them back to the surface. The Moon’s delicate atmosphere is so thin that the water molecules would never actually bump into each other as they flew on these trajectories over the surface. Some researchers think that, through this random movement, water could hop across the surface, with some landing in ultra-cold craters at the poles, where it would freeze out into the lunar soil and remain stuck as ice crystals. In craters where the sun never shines, a reserve of ice could have built up this way over billions of years.
Scientists don’t know if this process is actually at work on the Moon, but orbiting spacecraft observations suggest the amount of water or hydroxyl across the surface is rising and falling, making scientists think water molecules may be moving around. If the lunar water really is that mobile, then those polar ice reserves may be building up, even today. If it’s not, another possible explanation could be that this water is ancient. It could have come from volcanic activity very early in the Moon’s history, or may have been deposited on the Moon long ago by one or two large comet impacts, then buried, stirred up and redistributed by subsequent smaller impacts in the billions of years since.
From their perches aboard the new lunar landers, NSS and NIRVSS will complement each other in tracking how hydrogen levels change both at the surface and deeper down, and help solve the mystery of whether water is still being supplied to the Moon’s poles.
Mapping the Moon’s Resources
Current plans for these instruments are for delivery to the lunar surface via non-mobile landers. However, in the future NSS and NIRVSS could be put to work aboard a rover crisscrossing the surface. NSS could make measurements nearly the whole time as it moved over the lunar landscape and sense hydrogen buried below the surface. By locating promising sites, it could tell a prospecting rover where to drill into the ground, bring up a soil sample and take a closer look. NIRVSS could then identify the components that make up that soil and evaluate different samples for further exploration.
Together on a rover, these tools for lunar prospecting could provide the data needed to create maps of resources awaiting human explorers on the Moon and identify hot spots of critical materials. The ability to harvest the ingredients to make products and fuel directly at deep space locations will be an important step in truly pioneering space, from the Moon to Mars and beyond.
February 2019: NASA selects both NSS and NIRVSS for delivery to the Moon – perhaps as early as 2020 – by commercial partners providing lunar payload delivery services.
The Neutron Spectrometer System was jointly developed by NASA’s Ames Research Center and Lockheed Martin Advanced Technology Center, in Palo Alto, California.
For the Near-Infrared Volatiles Spectrometer System, NASA Ames partnered with the Brimrose Corporation, in Sparks, Maryland, to develop the spectrometer.