Evidence map›Paper›PMID 38459034›Full record

ArticleNature communications2024

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 and 18 more

Abstract read
In one paragraph

Article in Nature communications, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

2 citing papers in PubMed.

  1. Article
  2. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

28 authors.

Liang Ding *State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China. liangding@hit.edu.cn.ORCID http://orcid.org/0000-0002-8351-5178
Ruyi Zhou *State Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.ORCID http://orcid.org/0000-0002-1854-9451
Tianyi Yu *Beijing Aerospace Control Center, Beijing, 100094, China.ORCID http://orcid.org/0000-0001-5017-4920
Huaiguang YangState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.ORCID http://orcid.org/0000-0001-6747-0988
Ximing HeBeijing Aerospace Control Center, Beijing, 100094, China.
Haibo GaoState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China. gaohaibo@hit.edu.cn.ORCID http://orcid.org/0000-0002-6501-656X
Juntao WangCenter for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Science, Guiyang, 550081, China.ORCID http://orcid.org/0000-0002-2837-6822
Ye YuanState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.ORCID http://orcid.org/0000-0002-8690-5913
Jia WangBeijing Aerospace Control Center, Beijing, 100094, China.ORCID http://orcid.org/0000-0003-0713-8830
Zhengyin WangState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.ORCID http://orcid.org/0000-0002-2418-6167
Huanan QiState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.ORCID http://orcid.org/0000-0002-1707-7122
Jian LiBeijing Aerospace Control Center, Beijing, 100094, China. lisirjian@163.com.
Wenhao FengState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.
Xin LiBeijing Aerospace Control Center, Beijing, 100094, China.
Chuankai LiuBeijing Aerospace Control Center, Beijing, 100094, China.
Shaojin HanBeijing Aerospace Control Center, Beijing, 100094, China.
Xiaojia ZengCenter for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Science, Guiyang, 550081, China.ORCID http://orcid.org/0000-0002-6536-779X
Yu-Yan Sara ZhaoResearch Center for Planetary Science, College of Earth Science, Chengdu University of Technology, Chengdu, 610059, China.ORCID http://orcid.org/0000-0003-2551-5425
Guangjun LiuDepartment of Aerospace Engineering, Ryerson University, Toronto, ON, M5B 2K3, Canada.
Wenhui WanState Key Laboratory of Remote Sensing Science, Aerospace Information Research Institute, Chinese Academy of Sciences, Beijing, 100101, China.
Yuedong ZhangBeijing Aerospace Control Center, Beijing, 100094, China.
Saijin WangBeijing Aerospace Control Center, Beijing, 100094, China.
Lichun LiBeijing Aerospace Control Center, Beijing, 100094, China.
Zongquan DengState Key Laboratory of Robotics and System, Harbin Institute of Technology, Harbin, 150080, China.
Jianzhong LiuCenter for Lunar and Planetary Sciences, Institute of Geochemistry, Chinese Academy of Science, Guiyang, 550081, China. liujianzhong@vip.gyig.ac.cn.
Guolin HuBeijing Aerospace Control Center, Beijing, 100094, China.
Rui ZhaoBeijing Aerospace Control Center, Beijing, 100094, China.
Kuan ZhangBeijing Aerospace Control Center, Beijing, 100094, China.

Funding

Heilongjiang Postdoctoral Science Foundation LBH-Z20136National Natural Science Foundation of China (National Science Foundation of China) 51822502National Natural Science Foundation of China (National Science Foundation of China) 52205011National Natural Science Foundation of China (National Science Foundation of China) 91948202Natural Science Foundation of Heilongjiang Province LH2022E054
6 · The paper itself

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.

Identifiers

PMID38459034
PMCPMC11258293

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