One Small Grain of Moon Dust, One Giant Leap for Lunar Studies

A full Moon.
Scientists found a new way to analyze the chemistry of the Moon’s soil using a single grain of Moon dust. Their technique can help us learn more about conditions on the surface of the Moon and the formation of precious resources like water and helium there. (Image: via Pixabay)

Back in 1972, NASA sent their last team of astronauts to the Moon in the Apollo 17 mission. These astronauts brought Moon dust and rocks back to Earth so scientists could continue to study lunar soil in their labs.

Since we haven’t returned to the Moon in almost 50 years, every lunar sample is precious. We need to make them count for researchers now and in the future. In a new study in Meteoritics & Planetary Science, scientists found a new way to analyze the chemistry of the Moon’s soil using a single grain of dust.

Their technique can help us learn more about conditions on the surface of the Moon and the formation of precious resources like water and helium there. Jennika Greer, the paper’s first author and a Ph.D. student at the Field Museum and University of Chicago, said:

Philipp Heck, a curator at the Field Museum, associate professor at the University of Chicago and co-author of the paper, said:

The technique is called atom probe tomography (APT), and it’s normally used by materials scientists working to improve industrial processes like making steel and nanowires. But its ability to analyze tiny amounts of materials makes it a good candidate for studying lunar samples. The Apollo 17 sample contains 111 kilograms (245 pounds) of lunar rocks and soil — in the grand scheme of things, not a whole lot, so researchers have to use it wisely. Greer’s analysis only required one single grain of soil, about as wide as a human hair.

A tiny grain of lunar soil brought back by Apollo 17, magnified under a scanning electron microscope.
A tiny grain of lunar soil brought back by Apollo 17, magnified under a scanning electron microscope. (Image: Jennika Greer via Field Museum)

In that tiny grain, she identified products of space weathering, pure iron, water, and helium that formed through the interactions of the lunar soil with the space environment. Extracting these precious resources from lunar soil could help future astronauts sustain their activities on the Moon. To study the tiny grain, Greer used a focused beam of charged atoms to carve a tiny, super-sharp tip into its surface. This tip was only a few hundred atoms wide — for comparison, a sheet of paper is hundreds of thousands of atoms thick. Philipp Heck said:

Once the Moon dust sample was inside the atom probe at Northwestern University, Greer zapped it with a laser to knock atoms off one by one. As the atoms flew off the sample, they struck a detector plate. Heavier elements, like iron, take longer to reach the detector than lighter elements, like hydrogen. By measuring the time between the laser firing and the atom striking the detector, the instrument is able to determine the type of atom at that position and its charge. Finally, Greer reconstructed the data in three dimensions, using a color-coded point for each atom and molecule to make a nanoscale 3D map of the Moon dust.

A tiny, sharped piece of a grain of moon dust, only a few hundred atoms wide.
A tiny, sharpened piece of a grain of Moon dust, only a few hundred atoms wide. (Image: Jennika Greer via Field Museum)

It’s the first time scientists have been able to see both the type of atoms and their exact location in a speck of Moon dust. While APT is a well-known technique in material science, nobody had ever tried using it for lunar samples before. Greer and Heck encourage other cosmochemists to try it out. Greer said:

Studying Moon dust gives insights into space weathering

Studying soil from the Moon’s surface gives scientists insight into an important force within our Solar System: space weathering. Space is a harsh environment, with tiny meteorites, streams of particles coming off the Sun, and radiation in the form of solar and cosmic rays. While Earth’s atmosphere protects us from space weathering, other bodies like the Moon and asteroids don’t have atmospheres. As a result, the soil on the Moon’s surface has undergone changes caused by space weathering, making it fundamentally different from the rock that the rest of the Moon is composed of. It’s kind of like a chocolate-dipped ice cream cone: the outer surface doesn’t match what’s inside.

Apollo 17 astronaut and geologist Harrison Schmitt in 1972 collecting samples of lunar soil that would later be used in this study.
Apollo 17 astronaut and geologist Harrison Schmitt in 1972 collecting samples of lunar soil and Moon dust that would later be used in this study. (Image: via NASA)

With APT, scientists can look for differences between space-weathered surfaces and unexposed Moon dust in a way that no other method can. By understanding the kinds of processes that make these differences happen, they can more accurately predict what’s just under the surface of moons and asteroids that are too far away to bring to Earth. Because Greer’s study used a nanosized tip, her original grain of Moon dust is still available for future experiments. This means new generations of scientists can make new discoveries and predictions from the same precious sample. Heck stated:

Greer and Heck emphasize the need for missions where astronauts bring back physical samples because of the variety of terrains in outer space. Greer added:

We don’t yet know what surprises we might find from space weathering. Greer explained:

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  • Troy Oakes

    Troy was born and raised in Australia and has always wanted to know why and how things work, which led him to his love for science. He is a professional photographer and enjoys taking pictures of Australia's beautiful landscapes. He is also a professional storm chaser where he currently lives in Hervey Bay, Australia.

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