EGU26-17572, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-17572
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 17:35–17:45 (CEST)
 
Room 0.94/95
Lunar Surface Magnetic Field Investigation of the Chang'e-7 Mission: Scientific Objectives and Instrumentation
Yasong Ge1, Aimin Du1, Shuquan Sun1, Yiing Zhang1, Hao Luo1, Lin Zhao1, Zhi Li1, Can Huang1, Lican Shan1, Lei Wang1, Kuixiang Zhang1, Jinqiao Fan1, Tong Liu1, Lei Wang2, Hao Geng2, Yuesong Chen2, Changbin Xue2, Yongliao Zou2, Yongxin Pan1, and Qinyun Di1
Yasong Ge et al.
  • 1Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China
  • 2National Space Science Center, Chinese Academy of Sciences, , Beijing, China

The upcoming Chang'e-7 (CE-7) mission, targeting a launch in 2026, will perform unprecedented exploration of the lunar south pole. A key scientific objective is to investigate the origin and characteristics of lunar surface magnetic anomalies, which hold critical information about the Moon's internal thermal evolution and past dynamo activity.

To achieve high-precision measurements, a dual-sensor tri-axial fluxgate magnetometer has been developed for this mission. This instrument will be deployed on the CE-7 rover to conduct in-situ surveys. Its design focuses on achieving an ultra-low noise level, enabling the detection of weak magnetic fields with high sensitivity. This capability is essential for mapping the fine-scale structure of magnetic anomalies and distinguishing between remnant crustal magnetization and fields induced by other mechanisms.

The primary scientific goals are to: 1) map the spatial distribution of magnetic fields at the south pole with high resolution, constrain the intensity and temporal evolution of the Moon's paleomagnetic field by analyzing the remanent magnetism of surface materials; 2) probe the lunar internal structure by analyzing the induced magnetic field response generated by the changing interplanetary magnetic field penetrating the Moon, which can reveal the electrical conductivity distribution of the lunar crust and mantle; 3) study how local magnetic fields modulate the surface space environment, potentially forming "mini-magnetospheres" that influence solar wind bombardment and volatile preservation through jointed space-Moon observations by combining surface magnetic field data from the rover with measurements from the orbiter’s magnetometer.

The findings from this investigation are expected to provide groundbreaking insights into the lunar internal structure and the history of the core dynamo, directly addressing fundamental questions in planetary science.

How to cite: Ge, Y., Du, A., Sun, S., Zhang, Y., Luo, H., Zhao, L., Li, Z., Huang, C., Shan, L., Wang, L., Zhang, K., Fan, J., Liu, T., Wang, L., Geng, H., Chen, Y., Xue, C., Zou, Y., Pan, Y., and Di, Q.: Lunar Surface Magnetic Field Investigation of the Chang'e-7 Mission: Scientific Objectives and Instrumentation, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-17572, https://doi.org/10.5194/egusphere-egu26-17572, 2026.