Nature Communications (Mar 2024)

Lunar rock investigation and tri-aspect characterization of lunar farside regolith by a digital twin

  • Liang Ding,
  • Ruyi Zhou,
  • Tianyi Yu,
  • Huaiguang Yang,
  • Ximing He,
  • Haibo Gao,
  • Juntao Wang,
  • Ye Yuan,
  • Jia Wang,
  • Zhengyin Wang,
  • Huanan Qi,
  • Jian Li,
  • Wenhao Feng,
  • Xin Li,
  • Chuankai Liu,
  • Shaojin Han,
  • Xiaojia Zeng,
  • Yu-Yan Sara Zhao,
  • Guangjun Liu,
  • Wenhui Wan,
  • Yuedong Zhang,
  • Saijin Wang,
  • Lichun Li,
  • Zongquan Deng,
  • Jianzhong Liu,
  • Guolin Hu,
  • Rui Zhao,
  • Kuan Zhang

DOI
https://doi.org/10.1038/s41467-024-46233-8
Journal volume & issue
Vol. 15, no. 1
pp. 1 – 15

Abstract

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Abstract Yutu-2 rover conducted an exciting expedition on the 41st lunar day to investigate a fin-shaped rock at Longji site (45.44°S, 177.56°E) by extending its locomotion margin on perilous peaks. The varied locomotion encountered, especially multi-form wheel slippage, during the journey to the target rock, established unique conditions for a fin-grained lunar regolith analysis regarding bearing, shear and lateral properties based on terramechanics. Here, we show a tri-aspect characterization of lunar regolith and infer the rock’s origin using a digital twin. We estimate internal friction angle within 21.5°−42.0° and associated cohesion of 520-3154 Pa in the Chang’E-4 operational site. These findings suggest shear characteristics similar to Apollo 12 mission samples but notably higher cohesion compared to regolith investigated on most nearside lunar missions. We estimate external friction angle in lateral properties to be within 8.3°−16.5°, which fills the gaps of the lateral property estimation of the lunar farside regolith and serves as a foundational parameter for subsequent engineering verifications. Our in-situ spectral investigations of the target rock unveil its composition of iron/magnesium-rich low-calcium pyroxene, linking it to the Zhinyu crater (45.34°S, 176.15°E) ejecta. Our results indicate that the combination of in-situ measurements with robotics technology in planetary exploration reveal the possibility of additional source regions contributing to the local materials at the Chang’E-4 site, implying a more complicated geological history in the vicinity.