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Rui Zhao et al.
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Jiayan Nie et al.
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Zongyu Zhang et al.
Summary: The Lunar Regolith Penetrating Radar (LRPR) on the Chang'E 5 lander is the first antenna-array radar deployed for the exploration of extraterrestrial objects. It can measure the subsurface structure of the moon with a resolution of about 10 cm. This study presents a cable delay calibration method and an imaging method based on radio astronomy to visualize the subsurface structure of the Chang'E-5 landing site. The radar images derived from LRPR observations show consistency and match the drilling process record.
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Heng-Ci Tian et al.
Summary: This study investigates the mineralogy and geochemistry of lunar basalts from the Chang'e-5 mission, revealing limited magma recharge or shallow-level assimilation in most crystals. Thermal modeling shows an enhanced magmatic flux around 2 billion years ago, suggesting episodic eruptions at the final stage could have above average eruptive fluxes, revising models of lunar thermal evolution.
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Song Mi et al.
Summary: Determining the mineral components of the lunar regolith is essential for understanding the Moon's origin and evolution, and it is a significant scientific objective of the Chang'E-5 Mission. The proposed sparse unmixing method based on the spectral library of various particle-size minerals provides valuable data for interpreting the mineral composition of the landing site. The analysis of the LMS reflectance spectra shows that the lunar soil in the sampling area is composed of agglutinates and glass, pyroxene, plagioclase, ilmenite, and olivine.
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Hui Zhang et al.
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Chunlai Li et al.
Summary: The CE-5 lunar sample collected by China's Chang'E-5 mission is consistent with weathered mare basalts in terms of mineralogy and petrochemistry. It is classified as a low-Ti/low-Al/low-K type with lower rare-earth-element (REE) contents compared to KREEP. This new sample, characterized by high FeO and low Mg index, could potentially represent a new class of lunar basalt.
NATIONAL SCIENCE REVIEW
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Honglei Lin et al.
Summary: Analysis of reflectance spectra from the Chang'E-5 lander reveals that lunar regolith samples from the Northern Oceanus Procellarum contain up to 120 ppm of water, mostly attributed to solar wind implantation. A light-colored rock named CE5-Rock near the lander exhibits stronger absorption and potentially contains around 180 ppm of water, suggesting an additional water source from the lunar interior. The low water content of the regolith may indicate degassing of the mantle reservoir beneath the Chang'E-5 landing site.
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Changyi Zhou et al.
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Jieneng Liang et al.
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Jianqing Feng et al.
Summary: This study examines the dielectric properties and stratigraphy of lunar regolith on the far side of the moon using data obtained from the Chang'E-4 mission. The results indicate that the regolith in the landing site is composed of fine-grained, low-loss material that is more homogeneous than previous research areas. The study also identifies a series of impact events, with the top layer primarily consisting of ejecta from a large crater located 140 km away.
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Keqing Zong et al.
Summary: The chemical composition study of CE-5 lunar soil shows that its major and trace elements are uniform and representative of the underlying basalt; CE-5 soil differs from basalt and soils returned by Apollo and Luna missions, but the depletion of volatile or siderophile elements in their mantle sources is comparable; The mantle source of CE-5 basalt may contain KREEP components, likely as trapped interstitial melts.
GEOCHIMICA ET COSMOCHIMICA ACTA
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Haoqiu Zhou et al.
Summary: This paper provides analyses on the maturity of lunar regolith at different depths and identifies the factors contributing to the variations in maturity levels. The results reveal that the near-surface regolith has a higher maturity compared to deeper layers, with localized regions exhibiting anomalously low maturity. Additionally, a newly discovered sandwich structure with low maturity between 12 and 18 m depth is attributed to heterogeneous weathering in a paleo-crater.
GEOPHYSICAL RESEARCH LETTERS
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Jianjun Liu et al.
Summary: The distribution, characteristics, and sources of lunar water are still controversial. In this study, the Chang'E-5 mission conducted in-situ spectral observations and laboratory analysis of returned samples to investigate the hydroxyl contents in lunar soils. The results show that the hydroxyl contents in the Chang'E-5 landing site are relatively weak, consistent with predictions from remote sensing and ground-based telescopic data. The study also suggests that apatite may be an important source of excess hydroxyl observed in young mare regions.
NATURE COMMUNICATIONS
(2022)
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Jianqing Feng et al.
Summary: This study uses Lunar Regolith Penetrating Radar (LRPR) observations to reconstruct the subsurface structure of the regolith under the Chang'E-5 lander. It identifies irregular, high-density zones in the regolith, speculates that rock fragments from these zones obstructed the drilling process, leading to an early termination. The study models the LRPR echoes using a finite-difference time-domain method to verify their inference of the regolith structure.
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Geochemistry & Geophysics
Bojun Jia et al.
Summary: China's Chang'E-5 mission has collected 1.731 kg samples from a young mare basalt unit in the northeastern Oceanus Procellarum region of the Moon. The provenance, chemical composition, formation, and evolution processes of the regolith at the CE-5 landing site are analyzed. The results provide key information on sample provenance and regolith stratigraphy of the landing site, which is crucial to deciphering the returned CE-5 samples.
EARTH AND PLANETARY SCIENCE LETTERS
(2022)
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Environmental Sciences
Yuxi Li et al.
Summary: This study presents the results of the Lunar Regolith Penetrating Radar (LRPR) equipped on China's Chang'E-5 probe, revealing the lunar regolith structure and electromagnetic properties of the landing site.
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Environmental Sciences
Yiping Yang et al.
Summary: This paper proposes an imaging method based on single-channel ultra-wideband (UWB) radar and dual-view observation for detecting non-line-of-sight (NLOS) targets. The method successfully eliminates ghosts and retains targets through dual-view observation at the levels of radar echo and image.
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Environmental Sciences
Chunyu Ding et al.
Summary: In this study, the loss tangent of lunar regolith at the Chang'E-5 landing site was estimated using the frequency shift method. The results showed that the loss tangent at the landing site is substantially higher than the typical lunar regolith, indicating a young basalt age and high TiO2+FeO content.
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Svein-Erik Hamran et al.
Summary: The Radar Imager for Mars Subsurface Experiment has conducted the first rover-mounted ground-penetrating radar survey of the Martian subsurface, revealing strongly reflecting layered sequences and providing insights into the geological history of Mars.
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Zhiyong Xiao et al.
Summary: Radar scans and orbital observations by the Yutu-2 rover have revealed post-mare deposits at the Chang'E-4 landing site, with ejecta potentially originating from the Finsen crater. There is debate over whether the Alder crater also contributes to these deposits, but the predicted thicknesses of ejecta from all potential source craters do not align adequately with observations.
GEOPHYSICAL RESEARCH LETTERS
(2021)
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Yuqi Qian et al.
Summary: Chang'e-5 successfully returned approximately 1,731 g of lunar samples, with findings indicating that the regolith at the landing site is around 4-6 meters thick and ejecta primarily coming from craters such as Xu Guangqi. Additionally, distal materials are mainly sourced from craters like Harpalus, Copernicus, Aristarchus, and Mairan G.
GEOPHYSICAL RESEARCH LETTERS
(2021)
Review
Astronomy & Astrophysics
Jianjun Liu et al.
Summary: The selection of landing sites is crucial for lunar landing missions and is closely linked to scientific goals. China has conducted landing site selection for a series of Chang' E missions, analyzing the support for lunar research and potential contributions. This study also highlights the implications of selected landing sites for key lunar questions and suggests the South Pole Region as a high-priority landing site for future missions.
SPACE SCIENCE REVIEWS
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Yuqi Qian et al.
Summary: Chang'e-5 is China's first lunar sample return mission, targeting to land in the northern Oceanus Procellarum region for various geological reasons. The Em4 mare basalts, which cover an area of 37,000 km(2) and are high-Ti basalts from the Eratosthenian age, will provide significant insights into lunar geology.
EARTH AND PLANETARY SCIENCE LETTERS
(2021)
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Engineering, Aerospace
ShaoXiang Shen et al.
Summary: The sampling return in Chang'E-5 mission is the third phase of China's lunar program, utilizing the Lunar Regolith Penetrating Radar (LRPR) to support drilling and sampling devices. The system design includes an antenna array and pre-amplifier circuit to enhance detection, with pre-stack Kirchhoff depth migration imaging used to identify target burial depth and thickness. Verification results meet task requirements.
IEEE AEROSPACE AND ELECTRONIC SYSTEMS MAGAZINE
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Multidisciplinary Sciences
Sen Hu et al.
Summary: This study analyzed samples returned from the surface of the Moon to reveal the water content and hydrogen isotope compositions of the Moon's youngest volcanic activities. The results suggest that the Moon's youngest volcanism was not driven by abundant water in its mantle source, but rather by previous volcanic activities causing dehydration of the mantle.
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Qiu-Li Li et al.
Summary: The study reports the youngest crystallization age of lunar basalts obtained through radiometric dating, extending the duration of lunar volcanic activity and providing a crucial calibration point for crater-counting chronology in the inner Solar System, shedding light on the volcanic and thermal history of the Moon.
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Multidisciplinary Sciences
Xiaochao Che et al.
Summary: By analyzing the youngest basalt lavas on the Moon, scientists have determined their age to be 1963 million years. This finding provides important constraints on the formation history and thermal evolution of the Moon. Additionally, there is no evidence for high concentrations of heat-producing elements in the deep mantle of the Moon, suggesting the need for alternative mechanisms to explain the continuous formation of lunar magmatism.
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Chunlai Li et al.
Summary: The Chang'e-4 (CE-4) mission is China's first human lander/rover mission on the far side of the Moon, aimed at conducting scientific exploration and studying the geology, environment, and astronomical phenomena of the lunar far side. The mission carries a variety of scientific instruments, has achieved numerous scientific objectives, and made significant progress in understanding the Moon's far side.
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Environmental Sciences
Jia Wang et al.
Summary: The Chang'e-5 mission landed successfully in Northern Oceanus Procellarum, with precise localization being crucial for engineering operations and scientific research. Localization was achieved through radio-tracking and image-based methods, aiding in mission planning and scientific analysis.
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Le Qiao et al.
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Ruigang Wang et al.
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