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Design for In-Situ Water Ice Analysis in the Lunar Polar Region
- LI Xiang1, WANG Xingping1, LU Wenzhen1, GUO Meiru2, HUANG Zhengxu3, ZHANG Xiaoping4, XU Zhenyu1, YAO Lu1, RUAN Jun1, KAN Ruifeng1, CAO Nailiang1
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1. Anhui Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, Hefei 230031, China;
2. Lanzhou Institute of Physics, China Academy of Space Technology, Lanzhou 730000, China;
3. Institute of Mass Spectrometry and Atmospheric Environment, JInan University, Guangzhou 510623, China;
4. State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, Macau 999078, China
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Received |
Revised |
Published |
28 Aug 2023 |
31 Oct 2023 |
25 Jan 2024 |
Issue Date |
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25 Jan 2024 |
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It is crucial to directly confirm the presence of water by detecting water ice and its content in the lunar polar region in situ. Spectroscopy and mass spectrometry are both important tools for identifying and quantifying material composition. They can complement each other to achieve comprehensive detection of water ice, volatile content, and H isotope abundance in the lunar polar region. The paper introduces the spectroscopy and mass spectrometry technique with Luna 25, Luna 27 and Viper as examples of typical in-situ detection applications. It includes the detection mechanism, operating mode and instrument functions, performance and applications. In last, we provided a brief introduction to the upcoming application of the “Chang’e-7” lunar polar region water molecule analyzer. This instrument comprises a laser absorption spectrometer, which is responsible for the in-situ analysis of H2O and HDO, and a time-of-flight mass spectrometer that enables the analysis of gas molecules with mass numbers < 200 amu, such as H2O and CH4. The scheme can support in-situ analysis of water ice for lunar south pole landing missions.
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