September 20, 2024

How Scientists Are Turning Moon Dust Into Drinking Water

How Scientists Are Turning Moon Dust Into Drinking WaterIn Situ Water Production on the Moon - How Scientists Are Turning Moon Dust Into Drinking Water
The strategy for in situ water production on the Moon through the reaction between lunar regolith and endogenous hydrogen. Credit: NIMTE

Researchers have developed a method to produce significant amounts of water on the Moon by reacting lunar regolith with hydrogen.

This innovative process could potentially yield over 50 kg of water from a ton of lunar soil, paving the way for sustainable human life and research stations on the Moon.

Lunar Water Extraction

Water plays a crucial role in human survival on the lunar surface, thus attracting extensive research attention. Prof. Junqiang Wang’s team at the Ningbo Institute of Materials Technology and Engineering (NIMTE) of the Chinese Academy of Sciences (CAS) has recently developed a new method of massive water production through reaction between lunar regolith and endogenous hydrogen.

Research results of previous lunar explorations, like the Apollo and Chang’E-5 missions, have revealed the widespread presence of water on the Moon. However, the water content in lunar minerals is extremely low, ranging from 0.0001% to 0.02%. It remains challenging to extract and utilize water in situ on the Moon.

Breakthrough in Lunar Hydrogen Utilization

“We used lunar regolith samples brought back by the Chang’E-5 mission in our study, trying to find a way to produce water on the Moon,” said Wang.

The study revealed that when the lunar regolith is heated above 1,200 K with concave mirrors, one gram of molten lunar regolith can generate 51–76 mg of water. In other words, one ton of lunar regolith could produce more than 50 kg of water, which is equal to about a hundred 500-ml bottles of drinking water. This would be enough drinking water for 50 people for one day.

Exploring Mineral Resources for Sustained Life on the Moon

In addition, lunar ilmenite (FeTiO3) was found to contain the highest amount of solar wind-implanted hydrogen among the five primary minerals in the lunar regolith, owing to its unique lattice structure with sub-nanometer tunnels.

In-situ heating experiments indicated that hydrogen in lunar minerals is a substantial resource for producing water on the Moon. Such water could be used both for drinking and irrigating plants. In addition it could be electrochemically decomposed into hydrogen and oxygen, with hydrogen being used for energy and oxygen being essential for breathing.

These discoveries provide pioneering insights into water exploration on the Moon and shed light on the future construction of lunar research stations.

The results of the study were published in the scientific journal The Innovation.

Reference: “Massive Water Production from Lunar Ilmenite through Reaction with Endogenous Hydrogen” by Xiao Chen, Shiyu Yang, Guoxin Chen, Weixu, Lijian Song, Ao Li, Hangbo Ce Yin, Weixing Xia, Meng Gao, Ming Li, Haichen Wu, Junfeng Cui, Lei Zhang, Lijing Miao, Xiaoxue Shui, Weiping Xie, Peiling Ke, Yongjiang Huang, Jianfei Sun, Bingnan Yao, Min Ji, Mingliang Xiang, Yan Zhang, Shaofan Zhao, Wei Yao, Zhigang Zou, Mengfei Yang, Weihua Wang, Juntao Huo, Jun-Qiang Wang and Haiyang Bai, 22 August 2024, The Innovation.
DOI: 10.1016/j.xinn.2024.100690