Search Results - "Li, Xiongyao"
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Chang’E-5 samples reveal high water content in lunar minerals
Published in Nature communications (10-09-2022)“…The formation and distribution of lunar surficial water remains ambiguous. Here, we show the prominence of water (OH/H 2 O) attributed to solar wind…”
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Nanophase Iron Particles Derived From Fayalitic Olivine Decomposition in Chang'E‐5 Lunar Soil: Implications for Thermal Effects During Impacts
Published in Geophysical research letters (16-03-2022)“…Surface‐correlated nanophase iron particles (npFe0) alter the reflectance spectrum characteristics of airless bodies, thus making it an essential aspect of…”
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3
Vacuum sintering behavior and magnetic transformation for high-Ti type basalt simulated lunar regolith
Published in Icarus (New York, N.Y. 1962) (01-09-2020)“…Lunar regolith in-situ utilization receives increasing attentions due to development of lunar exploration research. The complex composition of lunar regolith…”
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Discovery of nanophase iron particles and high pressure clinoenstatite in a heavily shocked ordinary chondrite: Implications for the decomposition of pyroxene
Published in Geochimica et cosmochimica acta (01-03-2020)“…Although pure metallic iron (i.e. that with an Fe content of greater than 99%) commonly occurs in achondrites, and within the returned soil from asteroids or…”
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Study of the Self-Polymerization of Epoxy/Phthalonitrile Copolymers and Their High-Performance Fiber-Reinforced Laminates
Published in Polymers (23-08-2023)“…Self-polymerization epoxy/phthalonitrile (APPEN) pre-polymers were studied systematically, and then, gelation time and differential scanning calorimetry (DSC)…”
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Sub-microscopic magnetite and metallic iron particles formed by eutectic reaction in Chang’E-5 lunar soil
Published in Nature communications (23-11-2022)“…Ferric iron as well as magnetite are rarely found in lunar samples, and their distribution and formation mechanisms on the Moon have not been well studied…”
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New Evidence for 4.32 Ga Ancient Silicic Volcanism on the Moon
Published in Geophysical research letters (16-07-2021)“…The currently available Apollo‐returned granitic lithology is restricted to only the nearside of the Moon (e.g., Procellarum KREEP Terrane [PKT]). In contrast,…”
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Revealing High‐Manganese Material on Mars at Microscale
Published in Geophysical research letters (16-09-2021)“…High‐manganese materials would provide valuable information about the history of a water‐rich and oxidizing environment on early Mars. However, the detailed…”
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Effect of crustal porosity on lunar magma ocean solidification
Published in Acta geochimica (01-04-2021)“…The lunar ferroan anorthosites, formed by plagioclase flotation from the crystallization of the lunar magma ocean, have an age span of over ~ 200 Ma. However,…”
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Inversions of subsurface temperature and thermal diffusivity on the Moon based on high frequency of Chang’E-1 microwave radiometer data
Published in Icarus (New York, N.Y. 1962) (01-09-2016)“…•We inverted mean subsurface temperature and regolith thermal diffusivity.•Thermal anomalous areas and hot/cold spots were identified by diffusivity.•Geologic…”
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The layered structure model for winonaite parent asteroid implicated by textural and mineralogical diversity
Published in Earth, planets, and space (02-04-2019)“…The winonaites are primitive achondrites that are associated with IAB iron meteorites. They provide valuable insights into differentiation processes on…”
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Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
Published in Frontiers in astronomy and space sciences (25-05-2023)“…The internal heat flow related to the Moon’s composition, interior structure, and evolution history is not well-constrained and understood on a global scale…”
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Experimental constraints on the formation of oxychlorine species by UV irradiation and mechanical pulverization on the lunar surface
Published in Acta geochimica (01-08-2024)“…Perchlorate and chlorate are present in various extraterrestrial celestial bodies throughout the solar system, such as Mars, the moon, and asteroids. To date,…”
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The Itokawa regolith simulant IRS-1 as an S-type asteroid surface analogue
Published in Icarus (New York, N.Y. 1962) (15-11-2019)“…Asteroid regolith simulants (i.e., substitute materials for asteroid surface regoliths) are useful for the preparation of asteroid landing and/or sample-return…”
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Oldest Immiscible Silica‐rich Melt on the Moon Recorded in a ~4.38 Ga Zircon
Published in Geophysical research letters (28-02-2020)“…The temporal duration of lunar‐evolved magmatism is still poorly constrained. In lunar meteorite Northwest Africa (NWA) 10049, a melt inclusion‐bearing zircon…”
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Occurrence and implications of secondary olivine veinlets in lunar highland breccia Northwest Africa 11273
Published in Meteoritics & planetary science (01-01-2020)“…Lunar breccias preserve the records of geologic processes on the Moon. In this study, we report the occurrence, petrography, mineralogy, and geologic…”
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In Situ Investigations of Dust Above the Lunar Terminator at the Chang'E‐3 Landing Site in the Mare Imbrium
Published in Geophysical research letters (16-09-2020)“…It was suspected that the horizon glow observed over the lunar terminator was caused by electrostatically levitated dust particles, but do high concentrations…”
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Petrology, mineralogy, porosity, and cosmic‐ray exposure history of Huaxi ordinary chondrite
Published in Meteoritics & planetary science (01-05-2017)“…A meteorite fall was heard and collected on July 13, 2010 at about 18:00 (local time) in the Shibanjing village of the Huaxi district of Guiyang, Guizhou…”
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New Martian Dust Simulant JMDS‐1 and Applications to Laboratory Thermal Conductivity Measurements
Published in Earth and space science (Hoboken, N.J.) (01-01-2022)“…Martian dust simulant (i.e., a terrestrial substitute for Martian dust) is the basis for experimentally investigating the properties of Martian dust and its…”
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In-situ lunar dust deposition amount induced by lander landing in Chang’E-3 mission
Published in Science China. Technological sciences (01-03-2020)“…China first in-situ lunar dust experiment is performed by a lunar dust detector in Chang’E-3 mission. The existed dust (less than 20 µm in diameter)…”
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