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Ding L, Zhou R, Yu T, Yang H, He X, Gao H, Wang J, Yuan Y, Wang J, Wang Z, Qi H, Li J, Feng W, Li X, Liu C, Han S, Zeng X, Zhao YYS, Liu G, Wan W, Zhang Y, Wang S, Li L, Deng Z, Liu J, Hu G, Zhao R, Zhang K. Lunar rock investigation and tri-aspect characterization of lunar farside regolith by a digital twin. Nat Commun 2024; 15:2098. [PMID: 38459034 PMCID: PMC11258293 DOI: 10.1038/s41467-024-46233-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/08/2022] [Accepted: 02/20/2024] [Indexed: 03/10/2024] Open
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.
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Affiliation(s)
- Liang Ding
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.
| | - Ruyi Zhou
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Tianyi Yu
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Huaiguang Yang
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Ximing He
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Haibo Gao
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.
| | - Juntao Wang
- Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Science, Guiyang, 550081, China
- CAS Center for Excellence in Comparative Planetology, Hefei, 230026, China
| | - Ye Yuan
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Jia Wang
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Zhengyin Wang
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Huanan Qi
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Jian Li
- Beijing Aerospace Control Center, Beijing, 100094, China.
| | - Wenhao Feng
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Xin Li
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Chuankai Liu
- Beijing Aerospace Control Center, Beijing, 100094, China
- Key Laboratory of Science and Technology on Aerospace Flight Dynamics, Beijing, 100094, China
| | - Shaojin Han
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Xiaojia Zeng
- Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Science, Guiyang, 550081, China
- CAS Center for Excellence in Comparative Planetology, Hefei, 230026, China
| | - Yu-Yan Sara Zhao
- Research Center for Planetary Science, College of Earth Science, Chengdu University of Technology, Chengdu, 610059, China
| | - Guangjun Liu
- Department of Aerospace Engineering, Ryerson University, Toronto, ON, M5B 2K3, Canada
| | - Wenhui Wan
- State Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing, 100101, China
| | - Yuedong Zhang
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Saijin Wang
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Lichun Li
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Zongquan Deng
- State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China
| | - Jianzhong Liu
- Center for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Science, Guiyang, 550081, China.
- CAS Center for Excellence in Comparative Planetology, Hefei, 230026, China.
| | - Guolin Hu
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Rui Zhao
- Beijing Aerospace Control Center, Beijing, 100094, China
| | - Kuan Zhang
- Beijing Aerospace Control Center, Beijing, 100094, China
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Effect of Lunar Complex Illumination on In Situ Measurements Obtained Using Visible and Near-Infrared Imaging Spectrometer of Chang’E-4. REMOTE SENSING 2021. [DOI: 10.3390/rs13122359] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/17/2022]
Abstract
In-situ measurements of the spectral information on the lunar surface are of significance to study the geological evolution of the Moon. China’s Chang’E-4 (CE-4) Yutu-2 rover has conducted several in-situ spectral explorations on the Moon. The visible and near-infrared imaging spectrometer (VNIS) onboard the rover has acquired a series of in-situ spectra of the regolith at the landing site. In general, the mineralogical research of the lunar surface relies on the accuracy of the in-situ data. However, the spectral measurements of the Yutu-2 rover may be affected by shadows and stray illumination. In this study, we analyzed 106 CE-4 VNIS spectra acquired in the first 24 lunar days of the mission and noted that six of these spectra were affected by the shadows of the rover. Therefore, a method was established to correct the effects of the rover shadow on the spectral measurements. After shadow correction, the FeO content in the affected area is corrected to 14.46 wt.%, which was similar to the result calculated in the normal regolith. Furthermore, according to the visible images, certain areas of the explored sites were noted to be unusually bright. Considering the reflectance, geometric information, and shining patterns of the multi-layer insulation (MLI), we examined the influence of the specular reflection of the MLI on the bright spot regionsd, and found that the five sets of data were likely not affected by the specular reflection of the MLI. The results indicated that the complex illumination considerably influences the in situ spectral data. This study can provide a basis to analyze the VNIS scientific data and help enhance the accuracy of interpretation of the composition at CE-4 landing sites.
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Compact Matrix-Exponential-Based FDTD with Second-Order PML and Direct Z-Transform for Modeling Complex Subsurface Sensing and Imaging Problems. REMOTE SENSING 2020. [DOI: 10.3390/rs13010094] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 11/16/2022]
Abstract
To simulate complex subsurface sensing and imaging problems with both propagating and evanescent waves by the finite-difference time-domain (FDTD) method, the highly-accurate second-order perfectly matched layer (SO-PML) formulations based on the direct Z-transform (DZT) and the matrix exponential (ME) techniques are compactly and efficiently proposed for modeling open-domain problems. During mathematical deductions, several manipulations, for example, convolution computations, formulation reorganizations, or variable substitutions, can be circumvented due to the fact that the ME-based method shows a compact first-order differential matrix form. Besides, any material attributes can be completely circumvented because of using electric and magnetic flux densities, consequently, the proposed DZT-SO-PML could be applied without needing any alteration. Moreover, the DZT-SO-PML method can not only preserve better absorption accuracies, but also attain palpable improvements in computational efficiencies, even if the distance between the DSP-SO-PML truncation and the target becomes closer for modeling 3D open-domain subsurface sensing and imaging problems. Finally, numerical examples have been carried out to illustrate and validate these proposed formulations.
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