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The lunar soil samples returned by China's Chang'e-5 (CE-5) contain valuable information on geological evolutions on the Moon. Herein, by employing high-resolution time-of-flight secondary ion mass spectrometry (TOF-SIMS), five rock chip samples from the CE-5 lunar soil are characterized in-depth, which reveal micro-morphological and compositional features. From the elemental/molecular ion distribution images, minerals such as pyroxene, ilmenite, feldspar, K-rich glass, silica, and silicate minerals are identified, along with their occurrence states and distribution results. More importantly, uncommon vesicle-like patterns are probed via TOF-SIMS, which may not be captured by conventional electron microscopy. The possible origins of vesicles are also proposed. Hopefully, these discoveries will provide essential guidance for future investigations on the Moon and accelerate the application of TOF-SIMS in space exploration.
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http://www.ncbi.nlm.nih.gov/pmc/articles/PMC11923877 | PMC |
http://dx.doi.org/10.1002/advs.202416639 | DOI Listing |
Sci Bull (Beijing)
August 2025
State Key Laboratory of Geological Processes and Mineral Resources, Frontiers Science Center for Deep-time Digital Earth, China University of Geosciences, Beijing 100083, China.
Langmuir
September 2025
State Key Laboratory of Advanced Environmental Technology & Guangdong Provincial Key Laboratory of Mineral Physics and Materials, Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou 510640, China.
Soil minerals are important natural adsorbents that regulate heavy metal fate; yet, the influence of natural drying on their adsorption behavior remains poorly understood. This study compared how drying affects Cd(II) and Zn(II) retention and selectivity on two widespread soil minerals, ferrihydrite (Fhy) and kaolinite (Kln), using single/binary adsorption experiments. Results indicated that drying significantly enhanced Cd(II) and Zn(II) retention on Fhy by promoting inner-sphere complexation and enhancing the stability of metal-mineral bonds, as evidenced by extended X-ray absorption fine structure (EXAFS) spectroscopy analyses.
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August 2025
State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
The role of widespread ilmenite in lunar mare regions in the abundance and diurnal variations of surficial OH/HO remains controversial. Here, we report the water content and hydrogen isotopes in the rims of lunar ilmenites from Chang'e-5 soil samples using an ion microprobe. Ilmenite rims exhibit higher water contents (~730 - 3,700 ppm) and lower δD values (-884 to -482‰) than that of the lunar mantle, indicating a predominantly endogenic origin from solar-wind (SW) implantation.
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July 2025
State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
The oxygen fugacity (fO) of the lunar mantle is of pivotal significance in comprehending the formation and evolution of the Moon. However, the fO of the lunar farside mantle remains unknown due to the lack of samples returned from the farside. Here, we determine the oxygen fugacity of 23 basaltic fragments from the Chang'e-6 (CE6) soil, the first farside sample collected from the South Pole-Aitken (SPA) basin.
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July 2025
Department of Mechanical Engineering, Johns Hopkins University, Baltimore, MD, USA.
From the crewed Apollo missions to the recent Chinese Chang'e landings, the interaction between spacecraft exhaust plumes and lunar soil produces dusty clouds with high-speed particle ejection. Despite varying landing sites, remarkably stable streak patterns were observed, raising questions about their origin. We solved this puzzle by showing that these patterns were driven by Görtler instability from the curved compressed shear layer of the supersonic but surprisingly laminar jet.
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