
The hidden water reservoirs uncovered in Black Beauty reshape our view of early Martian habitability and validate neutron CT as a vital tool for analyzing pristine planetary samples.
Neutron computed tomography, unlike conventional X‑ray CT, leverages the deep‑penetrating power of neutrons to highlight light elements such as hydrogen. This capability makes it uniquely suited for planetary science, where detecting water‑bearing phases in dense, mineral‑rich rocks is essential. By pairing neutron scans with traditional X‑ray imaging, researchers can generate complementary density and compositional maps without cutting or crushing precious samples, preserving their scientific integrity for future investigations.
Applying this dual‑modal approach to Black Beauty uncovered microscopic clasts of hydrogen‑rich iron oxyhydroxide, a mineral assemblage previously invisible to standard techniques. Though these clasts occupy only 0.4 % of the examined volume, they store about 11 % of the meteorite’s total water, pushing the overall water estimate to roughly 6,000 ppm. This concentration rivals the hydrated minerals identified by NASA’s Perseverance rover at Jezero crater, reinforcing the hypothesis that liquid water once covered large swaths of the Martian surface billions of years ago.
The broader implication is clear: non‑destructive CT methods can become the workhorse for the upcoming Mars Sample Return campaign and other extraterrestrial sample‑return missions. By imaging through titanium containment vessels, neutron and X‑ray CT can assess sample composition, guide extraction strategies, and even prioritize specimens for detailed laboratory analysis. As international efforts, such as China’s planned sample‑return mission, move forward, these imaging tools will enable scientists to maximize scientific return while safeguarding the pristine nature of the most valuable planetary materials.
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