According to new research from a Western University postdoctoral fellow, the early lunar crust that forms the Moon’s surface was significantly enriched in water more than 4 billion years ago, contrary to previously held beliefs. The discovery is described in a paper published today in Nature Astronomy.
Tara Hayden, a doctoral student at The Open University (U.K.), discovered the mineral apatite (the most prevalent phosphate) in a sample of early lunar crust while working with a meteorite she recognized as having come from the Moon.
The work provides fascinating new evidence that the Moon’s early crust held more water than previously assumed, potentially opening up new avenues for lunar history research.
“The discovery of apatite in the Moon’s early crust for the first time is incredibly exciting — as we can finally start to piece together this unknown stage of lunar history. We find the Moon’s early crust was richer in water than we expected, and its volatile stable isotopes reveal an even more complex history than we knew before,” said Hayden, currently working as a cosmochemist with planetary geologist Gordon “Oz” Osinski in Western’s department of Earth sciences.
The discovery of apatite in the Moon’s early crust for the first time is incredibly exciting — as we can finally start to piece together this unknown stage of lunar history. We find the Moon’s early crust was richer in water than we expected, and its volatile stable isotopes reveal an even more complex history than we knew before.
Tara Hayden
“Lunar meteorites are revealing new, exciting parts of the Moon’s evolution and expanding our knowledge beyond the samples collected during the Apollo missions. As the new stage of lunar exploration begins, I am eager to see what we will learn from the lunar far side,” said Hayden.
The Apollo samples were first assumed to be ‘volatile-poor’ upon their return from the Moon, leading to the wide-known description of the Moon as ‘bone dry.’
In 2008, Alberto Saal and other researchers discovered the presence of significant amounts of water and other volatiles in glass beads from the Apollo sample collection. This set forth fifteen years of re-analysis of the Apollo samples while newly found lunar meteorites have revealed the Moon had much more water across its surface.
“We know most about the history of water on the Moon from the Apollo samples, but those samples are thought to only represent about five percent of the entire Moon surface,” said Hayden. “Until we get more samples back in the upcoming Artemis missions, the only other samples from the surface we have are meteorites.”
Hayden made the discovery at The Open University during her PhD studies while verifying a rock sample for a collector as a lunar meteorite. Beyond its identification, the sample proved to be holding a key piece of data about water on the Moon.
“I was so lucky the meteorite not only came from the Moon but remarkably, featured chemistry so vital to our understanding about lunar water-bearing minerals,” said Hayden.
This research concentrated mostly on the mineral apatite, which contains volatile components in its crystalline structure. Apatite was detected in all lunar rock types except glass beads and ferroan anorthosites, which represent the Moon’s early crust. The Ferroan Anorthosite group is extremely old (4.5-4.3 billion years old) and is the only rock type known to have originated straight from the Lunar Magma Ocean, when the Moon was nearly completely molten.
The discovery of apatite in this rock type allowed for the first direct analysis of this hitherto unknown stage in lunar evolution.
“Unravelling the history of water in the earliest-formed lunar crust approximately 4.5 billion years ago is important for improving our understanding of the origin of water in the Solar System. Ancient rock samples from the Moon in the form of lunar meteorites provide an excellent opportunity for undertaking such investigations,” said Mahesh Anand, professor of planetary science and exploration at The Open University and Hayden’s formal lead supervisor.
Future Artemis missions
Hayden says the timing of the discovery is perfect as the NASA Artemis missions are preparing for launch and researchers, including her current supervisor, are developing programing and targets for the astronauts.
“It has been long believed the lunar surface has been dried out for thousands and even millions of years, but maybe there might be more water available than we thought on the surface of the Moon and we just need to find a way to extract it,” said Hayden.
Osinski is similarly thrilled about the potential applications of this new discovery. Last year, Osinski was named to the NASA geology team in charge of establishing the surface scientific plan for the first crewed lunar landing mission in over 50 years. He will work with his colleagues in mission control’s science backroom at NASA’s Johnson Space Center in Houston, providing support during the Artemis III mission.
“Tara’s discoveries are super exciting and will feed into our sampling strategy for the Artemis III mission where we hope to identify and sample some of the earliest crust on the Moon,” Osinski said in a statement.
Canadensys Aerospace is designing and building Canada’s first lunar rover, and Osinski is the primary investigator and scientific lead on the project.
