Xiaohui Fu
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View article: Discovery of crystalline Fe <sub>2</sub> O <sub>3</sub> in returned lunar soils
Discovery of crystalline Fe <sub>2</sub> O <sub>3</sub> in returned lunar soils Open
Lunar materials were believed to have formed and been preserved in a reducing environment, with only Fe 2+ and Fe 0 present. Native oxidized minerals, such as hematite, have not been validated in previously returned lunar samples. In this …
View article: Impact-induced mixing generated the stratified soils of the Lunar South Pole Aitken Basin
Impact-induced mixing generated the stratified soils of the Lunar South Pole Aitken Basin Open
The Mg-pyroxene annulus in the South Pole–Aitken (SPA) basin holds crucial information about the lunar crustal evolution, yet its mineralogy and origin remain debate. Here we analyzed the mineralogy, exogenic ejecta, and soil evolution of …
View article: Space Weathering Properties of Chang’e-6 Soils and Implication for Regolith Evolution of Young Lunar Maria
Space Weathering Properties of Chang’e-6 Soils and Implication for Regolith Evolution of Young Lunar Maria Open
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 the first farside soil samples from a young mare …
View article: Petrogenesis of Chang’e-6 Basalts and Implication for the Young Volcanism on the Lunar Farside
Petrogenesis of Chang’e-6 Basalts and Implication for the Young Volcanism on the Lunar Farside Open
Mare basalts from lunar farside are pivotal for unraveling lunar nearside-farside dichotomies and global thermal history. The Chang’e-6 (CE-6) mission conducted the first sampling from a young basaltic unit within the Apollo basin on the l…
View article: Mare Volcanism in Apollo Basin Evaluating the Mare Basalt Genesis Models on the Moon
Mare Volcanism in Apollo Basin Evaluating the Mare Basalt Genesis Models on the Moon Open
The Apollo basin is a well-preserved double-ringed impact basin located on the northeastern edge of the South Pole–Aitken (SPA) basin. The Apollo basin has been flooded and filled with large volumes of mare lavas, indicating an active volc…
View article: <scp>HBcrAg</scp> is associated with prognosis of hepatitis B virus‐related hepatocellular carcinoma in patients after hepatectomy undergoing antiviral therapy
<span>HBcrAg</span> is associated with prognosis of hepatitis B virus‐related hepatocellular carcinoma in patients after hepatectomy undergoing antiviral therapy Open
Serum hepatitis B core‐related antigen (HBcrAg) is considered a surrogate marker of the amount and activity of intrahepatic covalently closed circular DNA. This study aimed to explore the prognostic value of HBcrAg on patients with hepatit…
View article: The Lunar Regolith Thickness and Stratigraphy of the Chang’E-6 Landing Site
The Lunar Regolith Thickness and Stratigraphy of the Chang’E-6 Landing Site Open
The Chang’E-6 (CE-6) mission successfully returned 1935.3 g of lunar soil samples from the Apollo basin within the South Pole–Aitken basin. One of its scientific objectives is to investigate the subsurface structure and regolith thickness …
View article: Microphase iron particle growth promoted by solar wind implantation in lunar soils
Microphase iron particle growth promoted by solar wind implantation in lunar soils Open
Lunar soils record the history and spectral changes resulting from the space-weathering process. The solar wind and micrometeoroids are the main space-weathering agents leading to darkening (decreasing albedo) and reddening (increasing ref…
View article: Benefits of entecavir therapy in HBV-related hepatocellular carcinoma patients with compensated cirrhosis after hepatectomy: a ten-year cohort study
Benefits of entecavir therapy in HBV-related hepatocellular carcinoma patients with compensated cirrhosis after hepatectomy: a ten-year cohort study Open
Background Data on the impact of antiviral therapy(AVT) on the long-term outcomes of hepatitis B virus(HBV)-related hepatocellular carcinoma(HCC) patients with cirrhosis after hepatectomy are limited. We aimed to determine the effect of AV…
View article: Scientific objectives and payload configuration of the Chang'E-7 mission
Scientific objectives and payload configuration of the Chang'E-7 mission Open
As the cornerstone mission of the fourth phase of the Chinese Lunar Exploration Program, Chang'E-7 (CE-7) was officially approved, and implementation started in 2022, including a main probe and a communication relay satellite. The main pro…
View article: Dust events control nitrogen cycling and nitrate/(per)chlorate relationships on Mars
Dust events control nitrogen cycling and nitrate/(per)chlorate relationships on Mars Open
Nitrogen is an important part of any biosphere/organic cycling, but aspects of the nitrogen cycle for Mars are quite unclear. Nitrate and (per)chlorate have been detected in sedimentary rocks and aeolian sediments in Gale crater on Mars as…
View article: Solid−gas carbonate formation during dust events on Mars
Solid−gas carbonate formation during dust events on Mars Open
Electrostatic discharge experiments under simulated martian atmospheric conditions indicate that atmospheric CO2 has been sequestered into carbonate by the Mars dust activities during the Amazonia era.
View article: Aqueous alteration of the Vastitas Borealis Formation at the Tianwen-1 landing site
Aqueous alteration of the Vastitas Borealis Formation at the Tianwen-1 landing site Open
The Vastitas Borealis Formation is a Hesperian-aged sedimentary unit that mainly covers the Martian northern plains. Its environment of formation is uncertain but may be related to an ancient Martian ocean, outflow channel deposits, compac…
View article: A Raman Spectroscopic and Microimage Analysis Perspective of the Chang'e‐5 Lunar Samples
A Raman Spectroscopic and Microimage Analysis Perspective of the Chang'e‐5 Lunar Samples Open
The Chang'e‐5 (CE‐5) materials represent the youngest returned lunar samples. We performed a detailed Raman spectroscopic survey (1259‐point Raman modal analysis) to evaluate the mineralogical characteristics of CE‐5 soils, constraining th…
View article: A Martian Analogues Library (MAL) Applicable for Tianwen-1 MarSCoDe-LIBS Data Interpretation
A Martian Analogues Library (MAL) Applicable for Tianwen-1 MarSCoDe-LIBS Data Interpretation Open
China’s first Mars exploration mission, named Tianwen-1, landed on Mars on 15 May 2021. The Mars Surface Composition Detector (MarSCoDe) payload onboard the Zhurong rover applied the laser-induced breakdown spectroscopy (LIBS) technique to…
View article: Liver transplantation for late-onset ornithine transcarbamylase deficiency: A case report
Liver transplantation for late-onset ornithine transcarbamylase deficiency: A case report Open
LT can significantly improve partial neurological impairment caused by late-onset OTCD hyperammonemic encephalopathy, and LT can be actively considered when early drug therapy is ineffective.
View article: Radiative Transfer Modeling of Chang’e-4 Spectroscopic Observations and Interpretation of the South Pole-Aitken Compositional Anomaly
Radiative Transfer Modeling of Chang’e-4 Spectroscopic Observations and Interpretation of the South Pole-Aitken Compositional Anomaly Open
Chang’e-4 landed in the Von Kármán basaltic zone affected by Finsen ejecta from the South Pole-Aitken (SPA) “compositional anomaly” (SPACA), providing an opportunity to untangle the origin of the SPACA. We developed a mineral abundance unm…
View article: Regolith at Chang'E-5 landing site: mature lunar soils from Fe-rich and young mare basalts
Regolith at Chang'E-5 landing site: mature lunar soils from Fe-rich and young mare basalts Open
Space weathering process on airless bodies produces metallic iron (Fe 0 ) particles widely existing in the rim and interior of mineral grains, which complicate visible and near-infrared spectra of surface materials. Although these space we…
View article: Mars: new insights and unresolved questions – Corrigendum
Mars: new insights and unresolved questions – Corrigendum Open
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View article: Understanding the mineralogy and geochemistry of Chang'E-5 soil and implications for its geological significances
Understanding the mineralogy and geochemistry of Chang'E-5 soil and implications for its geological significances Open
Here we present the mineralogical and chemical data sources of Apollo, Luna, and Chang'E-5 (CE-5) missions. All the data are complied from previous studies. More reference details can be found in each excel files. Table S1 Modal mineralogy…
View article: Mars: new insights and unresolved questions
Mars: new insights and unresolved questions Open
Mars exploration motivates the search for extraterrestrial life, the development of space technologies, and the design of human missions and habitations. Here, we seek new insights and pose unresolved questions relating to the natural hist…
View article: Geomorphology, Mineralogy, and Geochronology of Mare Basalts and Non-Mare Materials around the Lunar Crisium Basin
Geomorphology, Mineralogy, and Geochronology of Mare Basalts and Non-Mare Materials around the Lunar Crisium Basin Open
The Nectarian-aged Crisium basin exhibits an extremely thin crust and complicated lunar geological history. This large multi-ring impact basin is characterized by prolonged lunar volcanism ranging from the Imbrian age to the Eratosthenian …
View article: Spatio-Temporal Analysis of Dust Storm Activity in Chryse Planitia Using MGS-MOC Observations from Mars Years 24–28
Spatio-Temporal Analysis of Dust Storm Activity in Chryse Planitia Using MGS-MOC Observations from Mars Years 24–28 Open
Dust storms, observed in all seasons, are among the most momentous of Mars’ atmospheric activities. The Entry–Descent–Landing (EDL) activity of a Martian landing mission is influenced by local atmospheric conditions, especially the probabi…
View article: Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications
Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications Open
We used the Crater Size Frequency distribution (CSFD) method to yield the formation ages of Pythagora, Sharp B, and Harpalus crater, and the crater density values (N(1)). Here we provide the crater counting data.
View article: Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications
Absolute model ages of three craters in the vicinity of the Chang'E-5 landing site and their geologic implications Open
We used the Crater Size Frequency distribution (CSFD) method to yield the formation ages of Pythagora, Sharp B, and Harpalus crater, and the crater density values (N(1)). Here we provide the crater counting data.
View article: A Mars Environment Chamber Coupled with Multiple In Situ Spectral Sensors for Mars Exploration
A Mars Environment Chamber Coupled with Multiple In Situ Spectral Sensors for Mars Exploration Open
Laboratory simulation is the only feasible way to achieve Martian environmental conditions on Earth, establishing a key link between the laboratory and Mars exploration. The mineral phases of some Martian surface materials (especially hydr…
View article: Earth Wind as a Possible Exogenous Source of Lunar Surface Hydration
Earth Wind as a Possible Exogenous Source of Lunar Surface Hydration Open
Understanding the sources of lunar water is crucial for studying the history of lunar evolution, as well as the interaction of solar wind with the Moon and other airless bodies. Recent orbital spectral observations revealed that the solar …