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CHEN Guanyu, MA Tao, ZHANG Yongqiang, ZHANG Yan, HUANG Yongyi, WU Kefan. Geant4 Simulation on Lunar Surface Water Content Inversion Using the Chang’E-7 Neutron and Gamma-ray Spectrometer (in Chinese). Chinese Journal of Space Science, 2026, 46(2): 1-8 doi: 10.11728/cjss2026.02.2025-0144
Citation: CHEN Guanyu, MA Tao, ZHANG Yongqiang, ZHANG Yan, HUANG Yongyi, WU Kefan. Geant4 Simulation on Lunar Surface Water Content Inversion Using the Chang’E-7 Neutron and Gamma-ray Spectrometer (in Chinese). Chinese Journal of Space Science, 2026, 46(2): 1-8 doi: 10.11728/cjss2026.02.2025-0144

Geant4 Simulation on Lunar Surface Water Content Inversion Using the Chang’E-7 Neutron and Gamma-ray Spectrometer

doi: 10.11728/cjss2026.02.2025-0144 cstr: 32142.14.cjss.2025-0144
  • Received Date: 2025-08-05
  • Rev Recd Date: 2025-11-11
  • Available Online: 2026-02-24
  • The Chang’E-7 lunar mission, scheduled for launch in 2026, has the primary scientific objective of detecting water-ice deposits within the Permanently Shadowed Regions (PSRs) at the lunar south pole. Understanding the distribution and concentration of lunar water ice is crucial for both fundamental science and future In-situ Resource Utilization (ISRU). In this study, we developed a high-fidelity model of the Chang’E-7 Lunar Neutron and Gamma-ray Spectrometer (LNGS) payload using the Geant4 toolkit (Version 10.07.p02) and established a quantitative inversion relationship between lunar surface water content and epithermal neutron count rates. The LNGS model, constructed by importing a detailed CAD model into Geant4, was rigorously validated against neutron beam calibration experiments conducted at the China Spallation Neutron Source (CSNS) Back-n facility. The results are as follows. The detector model shows excellent agreement with experimental data across the 0.4 eV to 1000 eV energy range, with a relative error of less than 6%, confirming the accuracy of the mass modeling and simulation setup. LNGS exhibits significant capability in discriminating soils with varying water content, as evidenced by both simulation and ground-based validation experiments using layered soil and water samples. Within the water-ice content range of 0.01% to 20%, simulations of galactic cosmic ray (GCR) bombardment and subsequent neutron transport show that the epithermal neutron (400~700 keV) count rate decreases significantly with increasing hydrogen abundance. This relationship follows a modified Lawrence model with an exceptional coefficient of determination (R2 = 0.9993). The slight parameter differences compared to the original Lawrence model are attributed to the different simulation tools, lunar regolith composition models, and distinct detector designs and energy responses between LNGS and the Lunar Prospector neutron spectrometer. This study provides a robust theoretical framework and a specific, validated inversion model for interpreting Chang’E-7 orbital neutron data, directly enabling the mapping of hydrogen concentrations from measured count rates. It establishes fundamental technical support for the development of in-situ resource utilization technologies on the Moon and paves the way for high-precision assessment of water ice resources in the lunar polar regions.

     

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