A recent study reveals that most of the moon's water is likely chemically bound in its deep interior. The findings, published on July 13, 2026, suggest significant implications for understanding the Earth-moon system's formation and evolutionary history.
New Discoveries About Lunar Water
For decades, scientists believed the moon was anhydrous, containing very little water. This perception shifted in 2009 when NASA's Lunar Crater Observation and Sensing Satellite (LCROSS) provided evidence of water ice in permanently shaded regions of the moon. However, the new research indicates that water is also present in the moon's interior, primarily as hydroxide (OH) bound to minerals.
Neil Bowles, a professor of planetary science at the University of Oxford, noted, "The Apollo samples appeared to be so dry, which was puzzling. This new understanding of water's presence in the moon's interior is crucial for understanding the initial water budget of our Earth-moon system, formed about 4.5 billion years ago after a Mars-sized impactor struck Earth."
The Role of Apatite in Water Retention
The study highlights the discovery of apatite, a mineral that can hold water within its crystal structure. Bowles explained, "Apatite shows that the moon had water and it's still present in the interior, basically bound to minerals." This contradicts earlier analyses that suggested the moon was extremely dry.





