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Journal articles on the topic 'Chang'e-5'

Author: Grafiati

Published: 4 June 2025

Last updated: 1 August 2025

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1

Yuqi, Qian, Xiao Long, Wang Qian, et al. "China's Chang'e-5 landing site: Geology, stratigraphy, and provenance of materials." Earth and Planetary Science Letters 561 (June 22, 2021): 116855. https://doi.org/10.5281/zenodo.5346571.

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<strong>Data for:</strong> China’s Chang’e-5 landing site: Geology, stratigraphy, and provenance of materials <strong>Data List: </strong> [1] "CE5_Geologic Map_4244N5053W_Qian2021.7z" for<strong> Figure 5 (Geological map of the CE-5 landing site)</strong> [2] "CE5_Crater Counts_Landing Site.7z" for <strong>Figure 6 (CSFD measurements of the CE-5  landing site)</strong> [3] "CE5_Distal Ejecta Distribution.7z" for <strong>Figure 7 (Ejecta distribution of major source craters in the Northern Oceanus Procellarum)</strong> <strong>Reference<

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2

Jia, Bojun, Wenzhe Fa, Mingwei Zhang, et al. "On the provenance of the Chang'E-5 lunar samples." Earth and Planetary Science Letters 596 (October 2022): 117791. http://dx.doi.org/10.1016/j.epsl.2022.117791.

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3

Li, Linxi, Hejiu Hui, Sen Hu, et al. "Discovery of carbonaceous chondritic fragment in Chang'e-5 regolith samples." Icarus 429 (March 2025): 116454. https://doi.org/10.1016/j.icarus.2025.116454.

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4

Feng, Jianqing, Yan Su, Chunlai Li, Shun Dai, Shuguo Xing, and Yuan Xiao. "An imaging method for Chang'e−5 Lunar Regolith Penetrating Radar." Planetary and Space Science 167 (March 2019): 9–16. http://dx.doi.org/10.1016/j.pss.2019.01.008.

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5

Qian, Yuqi, Long Xiao, Qian Wang, et al. "China's Chang'e-5 landing site: Geology, stratigraphy, and provenance of materials." Earth and Planetary Science Letters 561 (May 2021): 116855. http://dx.doi.org/10.1016/j.epsl.2021.116855.

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6

Ji, Jianglong, Huicun He, Sen Hu, et al. "Magmatic chlorine isotope fractionation recorded in apatite from Chang'e-5 basalts." Earth and Planetary Science Letters 591 (August 2022): 117636. http://dx.doi.org/10.1016/j.epsl.2022.117636.

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7

Zhang, Yue, Hejiu Hui, Sen Hu, et al. "Extremely large Cl isotopic fractionation in Chang'e-5 impact glass beads." Earth and Planetary Science Letters 644 (October 2024): 118933. http://dx.doi.org/10.1016/j.epsl.2024.118933.

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8

Yan, Pan, Zhiyong Xiao, Yanxue Wu, et al. "Submicroscopic iron-rich grains throughout impact glasses in Chang'E-5 regolith." Icarus 410 (March 2024): 115920. http://dx.doi.org/10.1016/j.icarus.2023.115920.

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9

WANG, ShaSha, LinXi LI, HeJiu HUI, and Bo WAN. "Geochemical characteristics of minerals and glass in Chang'e-5 breccia fragments." Acta Petrologica Sinica 41, no. 4 (2025): 1135–48. https://doi.org/10.18654/1000-0569/2025.04.02.

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10

Cao, Zhi, Xi Wang, Yun Chen, et al. "Nature of space-weathered rims on Chang'e-5 lunar soil grains." Earth and Planetary Science Letters 658 (May 2025): 119327. https://doi.org/10.1016/j.epsl.2025.119327.

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11

Shen, ShaoXiang, Bin Zhou, YuXi Li, et al. "The Design of Payload Lunar Regolith Penetrating Radar on Chang'E-5 Lander." IEEE Aerospace and Electronic Systems Magazine 36, no. 2 (2021): 4–16. http://dx.doi.org/10.1109/maes.2020.3033439.

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12

Wang, Siyuan, Mingjing Jiang, Tao Zhao, and Anning Shi. "Analyzing strain localization of Chang'E-5 lunar regolith through discrete element analysis." Powder Technology 448 (December 2024): 120293. http://dx.doi.org/10.1016/j.powtec.2024.120293.

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13

Yue, Zongyu, Kaichang Di, Gregory Michael, Sheng Gou, Yangting Lin, and Jianzhong Liu. "Martian surface dating model refinement based on Chang'E-5 updated lunar chronology function." Earth and Planetary Science Letters 595 (October 2022): 117765. http://dx.doi.org/10.1016/j.epsl.2022.117765.

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14

Zhang, Di, Bin Su, Yi Chen, Wei Yang, Qian Mao, and Li-Hui Jia. "Titanium in olivine reveals low-Ti origin of the Chang'E-5 lunar basalts." Lithos 414-415 (April 2022): 106639. http://dx.doi.org/10.1016/j.lithos.2022.106639.

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15

Di, K., M. Jia, X. Xin, et al. "HIGH RESOLUTION SEAMLESS DOM GENERATION OVER CHANG'E-5 LANDING AREA USING LROC NAC IMAGES." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLII-3 (April 30, 2018): 271–76. http://dx.doi.org/10.5194/isprs-archives-xlii-3-271-2018.

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Chang’e-5, China’s first sample return lunar mission, will be launched in 2019, and the planned landing area is near Mons Rümker in Oceanus Procellarum. High-resolution and high-precision mapping of the landing area is of great importance for supporting scientific analysis and safe landing. This paper proposes a systematic method for large area seamless digital orthophoto map (DOM) generation, and presents the mapping result of Chang’e-5 landing area using over 700 LROC NAC images. The developed method mainly consists of two stages of data processing: stage 1 includes subarea block adjustment

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16

Qiu, Mengfan, Sen Hu, Huicun He, et al. "Discovery of a highly shocked alkali suite clast in the Chang'e-5 lunar soils." Icarus 429 (March 2025): 116448. https://doi.org/10.1016/j.icarus.2024.116448.

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17

Qian, Yuqi, Long Xiao, James W. Head, Carolyn H. van der Bogert, Harald Hiesinger, and Lionel Wilson. "Young lunar mare basalts in the Chang'e-5 sample return region, northern Oceanus Procellarum." Earth and Planetary Science Letters 555 (February 2021): 116702. http://dx.doi.org/10.1016/j.epsl.2020.116702.

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18

Zhang, Xuhang, Fei Su, Guillaume Avice, et al. "Presence of non-solar derived krypton and xenon unveiled by Chang'e-5 lunar soils." Earth and Planetary Science Letters 637 (July 2024): 118725. http://dx.doi.org/10.1016/j.epsl.2024.118725.

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19

Wu, Bo, Jun Huang, Yuan Li, Yiran Wang, and Jin Peng. "Rock Abundance and Crater Density in the Candidate Chang'E-5 Landing Region on the Moon." Journal of Geophysical Research: Planets 123, no. 12 (2018): 3256–72. http://dx.doi.org/10.1029/2018je005820.

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20

Zhao, Weijie, and Chi Wang. "China's lunar and deep space exploration: touching the moon and exploring the universe." National Science Review 6, no. 6 (2019): 1274–78. http://dx.doi.org/10.1093/nsr/nwz120.

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Abstract The Chinese lunar probe Chang'e-4 (CE-4) landed in the Von Kármán crater within the South Pole–Aitken (SPA) basin on the far-side of the Moon on 3 January 2019. Following this, the moon rover Yutu-2 separated from the CE-4 lander and started its travels and exploration on the far-side of the Moon. Before this landing, humans had remotely observed the far-side of the Moon with lunar satellites. However, it was the first time that a man-made spacecraft had landed there and actually left behind wheel prints belonging to humanity. Since China's Lunar Exploration Project (CLEP), or Chang'e

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21

Wu, Xing, Yang Liu, Yazhou Yang, et al. "Mineralogy and regolith maturity at the Chang'E-5 landing site inferred from the Lunar Mineralogical Spectrometer." Earth and Planetary Science Letters 594 (September 2022): 117747. http://dx.doi.org/10.1016/j.epsl.2022.117747.

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22

Qian, Y. Q., L. Xiao, S. Y. Zhao, et al. "Geology and Scientific Significance of the Rümker Region in Northern Oceanus Procellarum: China's Chang'E-5 Landing Region." Journal of Geophysical Research: Planets 123, no. 6 (2018): 1407–30. http://dx.doi.org/10.1029/2018je005595.

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23

Zhao, Jiannan, Long Xiao, Le Qiao, Timothy D. Glotch, and Qian Huang. "The Mons Rümker volcanic complex of the Moon: A candidate landing site for the Chang'E-5 mission." Journal of Geophysical Research: Planets 122, no. 7 (2017): 1419–42. http://dx.doi.org/10.1002/2016je005247.

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24

Qian, Yuqi, Long Xiao, Shen Yin, et al. "The regolith properties of the Chang'e-5 landing region and the ground drilling experiments using lunar regolith simulants." Icarus 337 (February 2020): 113508. http://dx.doi.org/10.1016/j.icarus.2019.113508.

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25

Zou, Chen, Jialong Lai, Yanshuang Liu, Feifei Cui, Yi Xu, and Le Qiao. "Small lunar crater identification and age estimation in Chang'e-5 landing area based on improved Faster R-CNN." Icarus 410 (March 2024): 115909. http://dx.doi.org/10.1016/j.icarus.2023.115909.

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26

Yang, Hongmei, Haiyang Xian, Jianxi Zhu, et al. "Impact-induced fayalite glass from Chang'e-5 regolith revealed by electron pair distribution function and ReaxFF molecular dynamics." Icarus 438 (September 2025): 116643. https://doi.org/10.1016/j.icarus.2025.116643.

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27

Zhang, Tian, Hong Tang, Xiongyao Li, et al. "Unusual Space Weathering on a CE-5 Metal Grain Indicates Deceptive Surface Signatures of M-type Asteroids." Astrophysical Journal Letters 979, no. 2 (2025): L26. https://doi.org/10.3847/2041-8213/ada559.

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Abstract M-type asteroids are historically thought to be exposed metallic cores of differentiated planets with a composition dominated by pure iron and nickel. However, recent spectral and radar observations reveal an insufficient number of M-type asteroids in the main belt. Here, we report unusual space weathering characteristics associated with a natural metal grain found in Chang'e 5 lunar soil. Microcraters, impact glass, iron whiskers, and unique vesicular rims on the surface of this grain help to explain the unusual properties of some potential M-type asteroids, including low thermal ine

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28

Qiao, Le, Jian Chen, Luyuan Xu, et al. "Geology of the Chang'e-5 landing site: Constraints on the sources of samples returned from a young nearside mare." Icarus 364 (August 2021): 114480. http://dx.doi.org/10.1016/j.icarus.2021.114480.

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29

Bo, Zheng, Kaichang Di, Zhaoqin Liu, Zongyu Yue, Jia Liu, and Ke Shi. "A catalogue of meter-scale impact craters in the Chang'e-5 landing area measured from centimeter-resolution descent imagery." Icarus 378 (May 2022): 114943. http://dx.doi.org/10.1016/j.icarus.2022.114943.

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30

Hou, Xuting, Xiaohui Fu, Le Qiao, et al. "Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications." Icarus 372 (January 2022): 114730. http://dx.doi.org/10.1016/j.icarus.2021.114730.

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31

Jia, Mengna, Zongyu Yue, Kaichang Di, Bin Liu, Jianzhong Liu, and Gregory Michael. "A catalogue of impact craters larger than 200 m and surface age analysis in the Chang'e-5 landing area." Earth and Planetary Science Letters 541 (July 2020): 116272. http://dx.doi.org/10.1016/j.epsl.2020.116272.

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32

Qiu, Mengfan, Sen Hu, Huicun He, et al. "Corrigendum to “Discovery of a highly shocked alkali suite clast in the Chang'e-5 lunar soils” [Icarus 429 (2025) 116448]." Icarus 430 (April 2025): 116486. https://doi.org/10.1016/j.icarus.2025.116486.

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33

Su, Fei, Xuhang Zhang, Youjuan Li, et al. "Constraining 2.0 Ga Volcanism on the Moon via ⁴⁰Ar/³⁹Ar Dating of Chang'e‐5 Basalts." Journal of Geophysical Research: Planets 130, no. 2 (2025). https://doi.org/10.1029/2024je008495.

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AbstractThe Chang'e‐5 landing site provides an important window into the Moon's late Eratosthenian period of volcanism at ∼2 Ga. Clarifying the Moon's history of volcanic activity using radioisotopic dating assists investigations of the evolution of the lunar surface as well as the Moon's internal dynamics. Recent chronological investigations of Chang'e‐5 basalts produced ages spanning ∼100 Ma, thereby inhibiting interpretation of the duration of volcanism recorded in the returned samples. We used microcomputed tomography and Back‐Scatter Electron imaging to characterize the structure and morp

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34

Li, Ziqing, Bo Zhang, Shui‐jiong Wang, Xiaochao Che, and Tao Long. "Widespread Involvement of Low‐Abundance KREEP in the Mantle of Chang'e‐5 and Its Surrounding Units." Terra Nova, February 5, 2025. https://doi.org/10.1111/ter.12766.

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ABSTRACTThe return of the young Chang'e‐5 (CE‐5) samples provide new insights into the lunar thermal evolution. In this study, we present a new type of exotic low‐Ti basalt in CE‐5 breccia, which has a magmatic equigranular texture with low Ti content and high Mg bulk composition and minerals. Low rare earth elements (REEs) imply that the clast was probably derived from a primitive source, which may originate from western ancient mare unit. Based on fractional crystallisation modelling, the exotic basalt source is considered as low‐Ti high‐Al, opposing the source of CE‐5 basalts. Our partial m

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35

Wu, Wenhui, Xin Ren, Zhaopeng Chen, et al. "Oblique Impact Adjacent to Chang'E−5 Sampling Site: Fine‐Scale Analysis and Implication on the Provenance of Returned Samples." Journal of Geophysical Research: Planets 130, no. 1 (2024). https://doi.org/10.1029/2024je008474.

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AbstractImpact ejecta is a major source of lunar regolith. Symmetric ejecta thickness models are widely used to estimate ejecta distribution. However, they cannot accurately describe the asymmetric distributions from oblique impacts. Here, the Xu Guangqi crater provides an example for the study of oblique impacts. High‐resolution data from this crater, acquired during the Chang'E−5 mission, has facilitated studies of a potential oblique impact, the development of a correction model for asymmetric ejecta distribution, and a detailed analysis of regolith provenance at the sampling site. The resu

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36

Li, Linxi, Hejiu Hui, Sen Hu, et al. "Petrogenesis of Chang'E‐5 young mare low‐Ti basalts." Meteoritics & Planetary Science, September 21, 2023. http://dx.doi.org/10.1111/maps.14071.

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AbstractThe regolith samples returned by the Chang'E‐5 mission (CE‐5) contain the youngest radiometrically dated mare basaltic clasts, which provide an opportunity to elucidate the magmatic activities on the Moon during the late Eratosthenian. In this study, detailed petrographic observations and comprehensive geochemical analyses were performed on the CE‐5 basaltic clasts. The major element concentrations in individual plagioclase grain of the CE‐5 basalts may vary slightly from core to rim, whereas pyroxene has clear chemical zonation. The crystallization sequence of the CE‐5 mare basalts wa

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37

Wenzhe, Fa, Jia Bojun, Zhang Mingwei, Di Kaichang, xi Minggang, and Li Yang. "On the provenance of the Chang'E-5 lunar samples." August 12, 2022. https://doi.org/10.5281/zenodo.6984174.

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This website contains the derived data in the manuscript <em>On the provenance of the Chang’E-5 lunar samples</em> by Bojun Jia, Wenzhe Fa, Mingwei Zhang, Kaichang Di, Minggang Xie, Yushan Tai, and Yang Li that is published in <em>Earth and Planetary Science Letters</em>.

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38

Yan, Pan, Zhiyong Xiao, Yanxue Wu, Yunhua Wu, Mingchao Xiong, and Qing Pan. "Adhesion of Silicate Impact Melts on Impact Glasses of Chang'e‐5 Regolith." Journal of Geophysical Research: Planets 129, no. 12 (2024). https://doi.org/10.1029/2024je008777.

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AbstractMicroscopic silicate melts are ubiquitous on surfaces of lunar regolith particles, and they record physicochemical processes of regolith reworking on the Moon. Similar microstructures are visible on surfaces of the Chang'e‐5 lunar impact glass particles, which are predominantly sourced from local mare deposits. Therefore, the microscopic silicate melts provide an invaluable opportunity to study the movements, provenances, and chemical alterations of substances involved in regolith reworking. However, the small lateral sizes and thicknesses of the surface silicate melts are a challenge

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39

Yang, Chen, Xinmei Zhang, Lorenzo Bruzzone, et al. "Comprehensive mapping of lunar surface chemistry by adding Chang'e-5 samples with deep learning." Nature Communications 14, no. 1 (2023). http://dx.doi.org/10.1038/s41467-023-43358-0.

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AbstractLunar surface chemistry is essential for revealing petrological characteristics to understand the evolution of the Moon. Existing chemistry mapping from Apollo and Luna returned samples could only calibrate chemical features before 3.0 Gyr, missing the critical late period of the Moon. Here we present major oxides chemistry maps by adding distinctive 2.0 Gyr Chang’e-5 lunar soil samples in combination with a deep learning-based inversion model. The inferred chemical contents are more precise than the Lunar Prospector Gamma-Ray Spectrometer (GRS) maps and are closest to returned samples

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40

Liu, Yuanzhou, and Shaopeng Huang. "In-situ measurements of thermal environment on the Moon's surface revealed by the Chang'E-4 and Chang'E-5 missions." IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, 2023, 1–13. http://dx.doi.org/10.1109/jstars.2023.3340853.

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41

Tian, Heng‐Ci, Jialong Hao, Yangting Lin, et al. "Distribution and Abundance of Solar Wind‐Derived Water in Chang'E‐5 Core Samples and Its Implications." Geophysical Research Letters 51, no. 9 (2024). http://dx.doi.org/10.1029/2023gl107005.

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AbstractKnowledge regarding the abundance and distribution of solar wind (SW)‐sourced water (OH/H2O) on the Moon in the shallow subsurface remains limited. Here, we report the NanoSIMS measurements of H abundances and D/H ratios on soil grains from three deepest sections of the Chang'E‐5 drill core sampled at depths of 0.45–0.8 m. High water contents of 0.13–1.3 wt.% are present on approximately half of the grain surfaces (topmost ∼100 nm), comparable to the values of Chang'E‐5 scooped soils. The extremely low δD values (as low as −995‰) and negative correlations between δD and water contents

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42

Su, Yanze, Luyuan Xu, and Meng‐Hua Zhu. "Impact Gardening Affects the Composition of Chang'e‐5 Lunar Soils." Journal of Geophysical Research: Planets 130, no. 2 (2025). https://doi.org/10.1029/2024je008501.

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AbstractThe composition of lunar samples sheds light on the Moon's evolutional history. Analyses of Chang'e‐5 (CE‐5) lunar soils showed <5% of foreign materials, significantly less than numerical predictions (∼10%). To address this inconsistency, we simulated the impact gardening process, accounting for distal ejecta, and tracked the compositional changes in the top 1 m layer at CE‐5 landing area over time. Our results show that impact gardening brings deeper local materials to the surface, leading to a mixture that reduces the distal ejecta proportion within the top 1 m layer from which th

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43

Tang, Xu, Hengci Tian, Shiduo Sun, et al. "Origin and implication of pentlandite in Chang'e-5 lunar soils." Lithos, September 2023, 107342. http://dx.doi.org/10.1016/j.lithos.2023.107342.

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44

Tian, Heng-Ci, Wei Yang, Yubing Gao, et al. "Reassessing the classification of Chang'e-5 basalts using pyroxene composition." Lithos, August 2023, 107309. http://dx.doi.org/10.1016/j.lithos.2023.107309.

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45

Wu, Fu-Yuan, Qiu-Li Li, Yi Chen, et al. "Lunar Evolution in Light of the Chang'e-5 Returned Samples." Annual Review of Earth and Planetary Sciences 52, no. 1 (2024). http://dx.doi.org/10.1146/annurev-earth-040722-100453.

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The Chinese spacecraft Chang'e-5 (CE-5) landed on the northern Ocean Procellarum and returned 1,731 grams of regolith. The CE-5 regolith is composed mostly of fragments of basalt, impact glass, agglutinates, and mineral fragments. The basalts could be classified as of a low-Ti and highly fractionated type based on their TiO2 content of ∼5.3 wt% and Mg# of ∼28. Independent of petrographic texture, the CE-5 basalts have a uniform eruption age of 2,030 ± 4 Ma, demonstrating that the Moon remained volcanically active until at least ∼2.0 Ga. Although the CE-5 landing site lies within the so-called

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46

Wu, Huanyu, Yuan Zou, Chi Zhang, et al. "Micro‐CT Characterization of the Chang'e‐5 Lunar Regolith Samples." Journal of Geophysical Research: Planets 130, no. 3 (2025). https://doi.org/10.1029/2024je008787.

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AbstractChang'e‐5 (CE‐5) lunar regolith samples were scanned using X‐ray micro‐computed tomography (micro‐CT), and over 0.7 million particles were extracted from the images through machine learning‐based segmentation. This is the largest three‐dimensional (3D) image data set on lunar regolith particles to date, offering a unique opportunity to study the key characteristics of the lunar regolith. The image intensity was correlated with mineral density, allowing for the assessment of the bulk density (1.58 g/cm3), true density (3.17 g/cm3), and mineralogy of the lunar regolith. Glass and plagioc

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47

Wu, Yunhua. "Impact-related chemical modifications of the Chang'E-5 lunar regolith." May 30, 2023. https://doi.org/10.5281/zenodo.8382512.

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This is the research data related to the manuscript titled: <strong>Impact-related chemical modifications of the Chang’E-5 lunar regolith, </strong>including the raw data of Raman spectra, the script for kernel density calculation, major and minor element compositions, the iSALE-2D configuration files and scripts, and the numerical modeling results.

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48

Zhang, Chaoqun, Xiaoguang Niu, Lixin Gu, et al. "Atomic‐Level Structural Responses of Chang'e‐5 Ilmenite to Space Weathering." Journal of Geophysical Research: Planets 129, no. 11 (2024). http://dx.doi.org/10.1029/2024je008447.

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AbstractSpace weathering records provide insights to better understand the formation and evolution of the lunar regolith. Ilmenite has contrasting responses to different space weathering processes. However, the atomic‐scale structural modification of ilmenite induced using different space weathering processes remains poorly understood. Here, we investigate the effects of spacing weathering on lunar ilmenite grains returned from Chang'e‐5 (CE‐5) mission using a combination of transmission electron microscopy and thermodynamic modeling approaches. Experimental results show that melt shock induce

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49

Xie, Minggang, Zhiyong Xiao, Xunyu Zhang, and Aoao Xu. "The Provenance of Regolith at the Chang'e‐5 Candidate Landing Region." Journal of Geophysical Research: Planets 125, no. 5 (2020). http://dx.doi.org/10.1029/2019je006112.

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50

Shi, Yuruo, Wenxiao Peng, Katherine H. Joy, et al. "Petrological, chemical, and chronological study of breccias in the Chang'e‐5 soil." Meteoritics & Planetary Science, May 24, 2024. http://dx.doi.org/10.1111/maps.14192.

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AbstractWe carried out a petrological, mineralogical, and geochemical study of fragmental and regolith breccia clasts separated from two Chang'e‐5 (CE‐5) soil samples, CE5C0000YJYX03501GP and CE5C0400, which provide an opportunity to investigate the compositional change of regolith at the landing site through time. Fragmental breccia CE‐5‐B3 contains a diverse range of basaltic clasts and basaltic mineral fragments, and some rare Mg‐suite‐like minerals. Regolith breccias CE‐5‐B006, CE‐5‐B007, CE‐5‐B010‐08, CE‐5‐B010‐09, CE‐5‐B011‐07, and CE‐5‐B016‐03 contain mare basaltic fragments, mare vitro

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