A5024888016- Planetary Science and Exploration
- Astro and Planetary Science
- Space Science and Extraterrestrial Life
- Space Exploration and Technology
- Geology and Paleoclimatology Research
- Isotope Analysis in Ecology
- Geochemistry and Geologic Mapping
- Geological and Geochemical Analysis
- Spaceflight effects on biology
- Radioactivity and Radon Measurements
- X-ray Spectroscopy and Fluorescence Analysis
- Laser-induced spectroscopy and plasma
- Geophysics and Gravity Measurements
- Hepatitis C virus research
- Hepatitis B Virus Studies
- Emotion and Mood Recognition
- Liver Disease Diagnosis and Treatment
- Chromatography in Natural Products
- Gaze Tracking and Assistive Technology
- Nuclear Physics and Applications
- Chemical Analysis and Environmental Impact
- Cholangiocarcinoma and Gallbladder Cancer Studies
- Advanced Image and Video Retrieval Techniques
- Spacecraft and Cryogenic Technologies
- Natural product bioactivities and synthesis
Shandong University
2017-2025
Chinese Academy of Sciences
2013-2025
Second Military Medical University
2019-2025
Eastern Hepatobiliary Surgery Hospital
2019-2025
Center for Excellence in Molecular Cell Science
2020-2024
Institute of Space Sciences
2024
East China University of Technology
2023
China United Network Communications Group (China)
2023
Anhui Polytechnic University
2023
Beijing University of Technology
2020-2022
Lithium-ion batteries are the primary power source in electric vehicles, and prognosis of their remaining useful life is vital for ensuring safety, stability, long lifetime vehicles. Accurately establishing a mechanism model vehicle lithium-ion battery involves complex electrochemical process. Remaining (RUL) prognostics based on data-driven methods has become focus research. Current research methodologies summarized this paper. By analyzing problems practical applications, that need to be...
ABSTRACT As the cornerstone mission of fourth phase Chinese Lunar Exploration Program, Chang'E-7 (CE-7) was officially approved, and implementation started in 2022, including a main probe communication relay satellite. The probe, consisting an orbiter, lander, rover mini-flying is scheduled to be launched 2026. lander will land on Shackleton crater's illuminated rim near lunar south pole, along with probe. satellite (named Queqiao-2) February 2024 as independent support during scientific...
Abstract Submicroscopic metallic iron particles (SMFe) are unique components of lunar soil produced during long‐term exposure on the Moon's surface. They can significantly alter optical properties and this alteration is crucial for interpretation remote sensing data. The origin formation SMFe remain a subject controversy, with multiple competing mechanisms coexisting. newly returned Chang'e‐5 (CE‐5) samples provide new opportunity to elucidate SMFe. Here, we conducted systematical study...
Abstract Chang’E-4 landed in the South Pole-Aitken (SPA) basin, providing a unique chance to probe composition of lunar interior. Its landing site is located on ejecta strips Von Kármán crater that possibly originate from neighboring Finsen crater. A surface rock and regolith at 10 sites along rover Yutu-2 track were measured by onboard Visible Near-Infrared Imaging Spectrometer first three days mission operations. In situ spectra have peak band positions 1 2 μm, similar spectral data Moon...
Abstract Mars exploration motivates the search for extraterrestrial life, development of space technologies, and design human missions habitations. Here, we seek new insights pose unresolved questions relating to natural history Mars, habitability, robotic exploration, planetary protection, impacts on society. Key observations findings include: – high escape rates early Mars' atmosphere, including loss water, impact present-day habitability; putative fossils will likely be ambiguous...
Abstract The Chang'e‐5 (CE‐5) materials represent the youngest returned lunar samples. We performed a detailed Raman spectroscopic survey (1259‐point modal analysis) to evaluate mineralogical characteristics of CE‐5 soils, constraining source and shock effects these unique mineral chemistry (e.g., Mg# 3‐60 for mafic minerals) abundance (first distinguishing basaltic feldspathic glasses) mare soils are different from those Apollo high‐ low‐Ti basalts, possibly representing an intermediate‐Ti...
Abstract The Vastitas Borealis Formation is a Hesperian-aged sedimentary unit that mainly covers the Martian northern plains. Its environment of formation uncertain but may be related to an ancient ocean, outflow channel deposits, compaction and drainage activities, or subsurface ice-related processes. Here we investigate geological evolution using geochemical mineralogical data acquired by Mars Surface Composition Detector on board Zhurong rover at Tianwen-1 landing site. We find...
Abstract Amorphous silicates are common in extraterrestrial materials, especially carbonaceous chondrites of petrologic types 1 and 2. In addition, high percentage amorphous components poorly crystalline phyllosilicates were found the mudstones at Gale Crater by CheMin instruments on board Mar Curiosity rover, which illustrates importance characterizing future planetary surface explorations. The structure an silicate can vary two aspects: degree polymerization crystallinity. Here we present...
Abstract Understanding the sources of lunar water is crucial for studying history evolution, as well interaction solar wind with Moon and other airless bodies. Recent orbital spectral observations revealed that a significant exogenous driver surficial hydration. However, shielded over period 3–5 days per month passes through Earth’s magnetosphere, during which loss hydration expected. Here we report temporal spatial distribution polar OH/H 2 O abundance, using Chandrayaan-1 Mineralogy Mapper...
Abstract Phoxite, (NH4)2Mg2(C2O4)(HPO4)2·4H2O, was initially discovered in 1977 and then officially confirmed 2018. It is the first mineral known to contain both phosphate oxalate group. Phoxite only found so far, Petrogale Cave, Western Australia Rowley mine, Arizona. In this work, we synthesized phoxite using oxammite newberyite as precursors under different relative humidity. Then, a systematic spectral characterization of performed, including Raman spectroscopy, mid infrared (MIR)...
Abstract The surfaces of airless bodies are constantly exposed to high‐energy particles and ionizing radiation, which interact with surficial materials, inducing crystal defects modifying spectral characteristics. In this study, a series irradiation experiments were performed simulate different types space including H + ion irradiation, electron (HE) X‐ray ultraviolet (UV) irradiation. Their visible near‐infrared (VNIR) reflectance spectra exhibit characteristic absorption features centered...
Abstract Chang’E-4 (CE-4) successfully landed on the floor of Von Kármán crater within South Pole-Aitken basin (SPA). One its scientific objectives is to determine subsurface structure and thickness lunar regolith at landing site along traverse route Yutu-2 rover. Using orbital data, we employed small craters (diameters <1 km) as probes investigate stratigraphy CE-4 site. In this study, 40 dark-haloed that penetrate through surface Finsen ejecta excavate underlying mare deposits were...
Laboratory simulation is the only feasible way to achieve Martian environmental conditions on Earth, establishing a key link between laboratory and Mars exploration. The mineral phases of some surface materials (especially hydrated minerals), as well their spectral features, are closely related conditions. Therefore, environment necessary for detection analysis. A chamber (MEC) coupled with multiple in situ sensors (VIS (visible)-NIR (near-infrared) reflectance spectroscopy, Raman...
The Chang’E-6 (CE-6) mission successfully returned 1935.3 g of lunar soil samples from the Apollo basin within South Pole–Aitken basin. One its scientific objectives is to investigate subsurface structure and regolith thickness at landing site. Using remote sensing datasets, we estimated basalt thicknesses site by employing crater morphology method excavation technique. A total 53 concentric craters 108 fresh with varying depths were identified. Our results indicate that CE-6 ranges 1.1 7.0...
Abstract Mare basalts from lunar farside are pivotal for unraveling nearside-farside dichotomies and global thermal history. The Chang’e-6 (CE-6) mission conducted the first sampling a young basaltic unit within Apollo basin on farside. Here, we performed comprehensive petrological geochemical analyses CE-6 basalt clasts. is low-titanium (about 5 wt% TiO 2 ) depleted in KREEP components. absence of olivine, particularly magnesium-rich suggests that magma underwent extensive fractional...
Abstract Lunar soil samples from young maria (formed <3.0 billion years ago (Ga)) preserve key records of recent space weathering history in the Earth–Moon system. China’s Chang’e-6 mission returned first farside a mare (∼2.8 Ga) at northeastern South Pole–Aitken basin. We present preliminary results on properties soils. The glassy agglutinate content soils is approximately 30%, significantly lower than 50%–70% observed mature Apollo older (>3.0 and higher ∼21% found Chang’e-5 younger...