Search Results - "Li, Xiongyao"

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  1. 1

    Chang’E-5 samples reveal high water content in lunar minerals by Zhou, Chuanjiao, Tang, Hong, Li, Xiongyao, Zeng, Xiaojia, Mo, Bing, Yu, Wen, Wu, Yanxue, Zeng, Xiandi, Liu, Jianzhong, Wen, Yuanyun

    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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  2. 2

    Nanophase Iron Particles Derived From Fayalitic Olivine Decomposition in Chang'E‐5 Lunar Soil: Implications for Thermal Effects During Impacts by Guo, Zhuang, Li, Chen, Li, Yang, Wen, Yuanyun, Tai, Kairui, Li, Xiongyao, Liu, Jianzhong, Ouyang, Ziyuan

    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. 3

    Vacuum sintering behavior and magnetic transformation for high-Ti type basalt simulated lunar regolith by Song, Lei, Xu, Jiao, Tang, Hong, Liu, Jiquan, Liu, Jianzhong, Li, Xiongyao, Fan, Shuqian

    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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  4. 4

    Discovery of nanophase iron particles and high pressure clinoenstatite in a heavily shocked ordinary chondrite: Implications for the decomposition of pyroxene by Guo, Zhuang, Li, Yang, Liu, Shen, Xu, Huifang, Xie, Zhidong, Li, Shijie, Li, Xiongyao, Lin, Yangting, Coulson, Ian M., Zhang, Mingming

    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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  5. 5

    Study of the Self-Polymerization of Epoxy/Phthalonitrile Copolymers and Their High-Performance Fiber-Reinforced Laminates by Xu, Mingzhen, Li, Bo, Li, Xiongyao, Fan, Zexu, Ren, Dengxun

    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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  6. 6

    Sub-microscopic magnetite and metallic iron particles formed by eutectic reaction in Chang’E-5 lunar soil by Guo, Zhuang, Li, Chen, Li, Yang, Wen, Yuanyun, Wu, Yanxue, Jia, Bojun, Tai, Kairui, Zeng, Xiaojia, Li, Xiongyao, Liu, Jianzhong, Ouyang, Ziyuan

    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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  7. 7

    New Evidence for 4.32 Ga Ancient Silicic Volcanism on the Moon by Zeng, Xiaojia, Li, Xiongyao, Xia, Xiao‐Ping, Liu, Jianzhong, Cui, Zexian, Yu, Wen, Ouyang, Ziyuan

    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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  8. 8

    Revealing High‐Manganese Material on Mars at Microscale by Zeng, Xiaojia, Wu, Yanxue, Zhao, Yuyan S., Pang, Runlian, Mo, Bing, Wen, Yuanyun, Li, Xiongyao, Liu, Jianzhong

    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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  9. 9

    Effect of crustal porosity on lunar magma ocean solidification by Zhang, Mingming, Xu, Yingkui, Li, Xiongyao

    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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  10. 10

    Inversions of subsurface temperature and thermal diffusivity on the Moon based on high frequency of Chang’E-1 microwave radiometer data by Wei, Guangfei, Li, Xiongyao, Wang, Shijie

    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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  11. 11

    The layered structure model for winonaite parent asteroid implicated by textural and mineralogical diversity by Zeng, Xiaojia, Shang, Yingli, Li, Shijie, Li, Xiongyao, Wang, Shijie, Li, Yang

    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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  12. 12

    Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations by Wei, Guangfei, Li, Xiongyao, Gan, Hong, Shi, Yaolin

    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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  13. 13

    Experimental constraints on the formation of oxychlorine species by UV irradiation and mechanical pulverization on the lunar surface by Li, Jiamei, Zhao, Yu-Yan Sara, Cui, He, Qu, Shuai-Yi, Peng, Yanhua, Yang, Yuhong, Li, Xiongyao

    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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  14. 14

    The Itokawa regolith simulant IRS-1 as an S-type asteroid surface analogue by Zeng, Xiaojia, Li, Xiongyao, Martin, Dayl J.P., Tang, Hong, Yu, Wen, Yang, Kang, Wang, Zegui, Wang, Shijie

    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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  15. 15

    Oldest Immiscible Silica‐rich Melt on the Moon Recorded in a ~4.38 Ga Zircon by Zeng, Xiaojia, Joy, Katherine H., Li, Shijie, Lin, Yangting, Wang, Nian, Li, Xiongyao, Li, Yang, Hao, Jialong, Liu, Jianzhong, Wang, Shijie

    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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  16. 16

    Occurrence and implications of secondary olivine veinlets in lunar highland breccia Northwest Africa 11273 by Zeng, Xiaojia, Li, Shijie, Joy, Katherine H., Li, Xiongyao, Liu, Jianzhong, Li, Yang, Li, Rui, Wang, Shijie

    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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  17. 17
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    Petrology, mineralogy, porosity, and cosmic‐ray exposure history of Huaxi ordinary chondrite by Li, Shijie, Wang, Shijie, Leya, Ingo, Li, Yang, Li, Xiongyao, Smith, Thomas

    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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  19. 19

    New Martian Dust Simulant JMDS‐1 and Applications to Laboratory Thermal Conductivity Measurements by Yu, Wen, Zeng, Xiaojia, Li, Xiongyao, Wei, Guangfei, Fang, Jichao

    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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  20. 20

    In-situ lunar dust deposition amount induced by lander landing in Chang’E-3 mission by Zhang, HaiYan, Wang, Yi, Chen, LiPing, Zhang, He, Li, CunHui, Zhuang, JianHong, Li, DeTian, Wang, YongJun, Yang, ShengSheng, Li, XiongYao, Wang, WeiDong

    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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