Apollo 17 geologist and astronaut Harrison Schmitt
next to a large bolder on the Taurus-Littrow landing site on the
Moon.
NASA
NASA is joining international partners to hunt for ice on the
Moon in support of future human exploration. The agency
is providing a water-detecting instrument, the Neutron
Spectrometer System (NSS), to the Lunar Polar Exploration
(LUPEX) mission led by JAXA (Japan Aerospace Exploration Agency) and ISRO
(Indian Space Research Organisation).
The instrument, which detects ice
under the lunar surface, will be installed on
LUPEX’s lunar rover planned to arrive at the
Moon no earlier than 2028. NASA’s support of LUPEX is part
of an ongoing effort to identify and
characterize lunar water and other materials that
easily evaporate near the Moon’s South Pole.
Water is a
critical material for NASA’s plans to develop an
enduring presence on the Moon. Instead of relying solely
on resources carried from Earth, astronauts could use the
Moon’s water for breathable air, rocket fuel, and more.
The first step is to find deposits of meaningful
quantities of water close to the surface to
mark potential landing areas for future astronauts. The water on
the Moon is mostly found as molecules within lunar regolith, the dusty and
rocky material that covers the Moon’s surface, but there may be ice
deposits below the surface of the lunar South Pole. Once we better
understand the quantity and quality of the available resources, we can learn
how to harness it for exploration.
“There is currently a gap in our
understanding of how lunar ice is distributed at small scales,
from 10s of centimeters up to 10s of kilometers,” said Rick Elphic,
NSS lead at NASA’s Ames Research Center in California’s Silicon Valley, where
the instrument was developed in collaboration with Lockheed Martin
Advanced Technology Center in Palo Alto, California. “The only way to
understand the ‘where’ and ‘how much’ of lunar ice is by exploring on the
surface at these scales.”
How neutrons signal water
NASA’s Neutron Spectrometer System instrument will
search for signs of water ice on the Moon’s surface aboard a lunar rover
belonging to the Lunar Polar Exploration (LUPEX) mission led by JAXA (Japan
Aerospace Exploration Agency) and ISRO (Indian Space Research Organisation).
NASA/Warren Davis
Scientists can search for water on
the Moon without drilling into the surface. Instead, they hunt for
concentrations of hydrogen, the H in H₂O. Past missions in lunar
orbit have found signs of water at the Moon’s poles,
but ground missions are needed to build detailed maps of
location and quantity.
Instruments like NSS can infer the
presence of hydrogen by detecting interactions with
particles called neutrons. Neutrons are constantly rattling around in
the lunar soil, and they’re about the same size as hydrogen atoms.
When these two particles interact, fewer medium-energy neutrons
are ejected from the soil. The absence of medium-energy neutrons suggests
more of the particles are interacting with hydrogen underground, a deficit that
can be measured with the right tools.
The NSS instrument uses a “gas
proportional counter” to detect neutrons bouncing out of the lunar
soil. It features two tubes that contain a rare gas called
helium-3 that is very sensitive to neutrons. When
neutrons strike the helium-3 gas atoms, the
gas produces electrical pulses that can be counted to infer the
presence and quantity of hydrogen up to three
feet underground.
Series
of water-hunters
Ongoing investigation of the
Moon’s water will inform how astronauts might
access it in the future. To that end, NASA researchers
at Ames have developed a series of NSS instruments intended
to ride aboard different missions to investigate sites at
the Moon’s South Pole.
The
first Moon-bound NSS instrument in the series was
carried aboard Astrobotic’s Peregrine lander, Astrobotic Peregrine Mission One, which launched in January 2024. That mission came to an
end without touching down on the lunar surface, but the NSS
aboard powered on and operated on multiple days over the course
of the 10-day mission. These operations successfully captured data about the
particle background of deep space, which strongly supported NSS operations on
future missions.
NASA’s VIPER (Volatiles Investigating Polar
Exploration Rover) mission, part of the agency’s
Artemis campaign, will carry another NSS. As part of NASA’s ongoing Commercial Lunar Payload
Services effort, a fourth NSS instrument
will ride aboard the MoonRanger “micro rover” developed by Carnegie
Mellon University in Pittsburgh.
“The three upcoming NSS rover
expeditions will tell us what kinds of places on the Moon are most likely to
host ice,” Elphic said. “Missions to the lunar surface can then be
planned to similar sites where ice can be found.”
The Neutron Spectrometer System was jointly developed by NASA’s Ames Research Center and Lockheed Martin Advanced Technology Center in Palo Alto, California.
For more information on the science of water on the Moon, visit: https://science.nasa.gov/moon/moon-water-and-ices
Karen Fox
/ Molly Wasser
Headquarters, Washington
Source: NASA’s Water-Hunting Tool Will Help Scout Moon’s South Pole - NASA


