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The utilization of analytical instruments for the detection and quantification of volatiles on the Moon is crucial for the development of in situ resource utilization technology. A test campaign under cryogenic conditions aimed to simulate the cold lunar environment of permanently shadowed regions (PSRs). The test campaign was performed in a Thermal Vacuum Chamber (TVAC) equipped with a bin of regolith simulant doped at three increasing water concentrations delineated at specific depths (Dry, 2.5, and 5 wt%, respectively). The average operating pressure of the chamber was 1.6×10 -6 Torr with an average regolith temperature of -178°C. Four holes were drilled into the regolith simulant bin using The Regolith and Ice Drill for Exploring New Terrain (TRIDENT) drill. The resulting cuttings-piles and their volatile activity were monitored via the Mass Spectrometer observing lunar operations (MSolo) instrument to determine the extent to which a mass spectrometer can monitor the release of volatiles during drilling activities in lunar-like environments. The results of this campaign helped to plan for the operation and subsequent data interpretation of the Polar Resources Ice Mining Experiment-1 (PRIME-1) mission on the Moon.
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Ayala et al. (2026) studied this question.
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