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DOI | 10.1016/j.epsl.2021.117107 |
Thermal evolution of water and hydrogen from Apollo lunar regolith grains | |
Jones B.M.; Aleksandrov A.; Hibbitts C.A.; Orlando T.M. | |
发表日期 | 2021 |
ISSN | 0012821X |
卷号 | 571 |
英文摘要 | The evolution of water and molecular hydrogen from Apollo lunar sample 15221, a mature mare soil, was examined by temperature program desorption (TPD) experiments conducted under ultra-high vacuum conditions. Desorption at the grain/vacuum interface with re-adsorption as water transports though the void space of the grains and activated sub-surface diffusion were found to reproduce the experimental TPD signal. Signal from the grain/vacuum interface yielded the second order desorption activation energies and site probability distributions. Water from sample 15221 exhibited a broad distribution of activation energies peaking at 130 kJ mol−1 extending up to 350 kJ mol−1 at zero coverage limit with an onset of 110 kJ mol−1 at full coverage. Our results suggest that water and hydrogen originating from lunar regolith contributes a minor amount to the observed mass in the LCROSS impact event. The abnormal amount of molecular hydrogen observed in the ejecta plume of the LCROSS impact may indicate that the radiolytic production of H2 from electron and galatic cosmic rays of physisorbed water is a contributor to the vast quantity of molecular hydrogen detected. © 2021 Elsevier B.V. |
关键词 | activation energieshydrogenlunar regolithrecombinative desorptionvolatileswater |
英文关键词 | Cosmology; Desorption; Hydrogen production; Lunar surface analysis; Probability distributions; Water; Energy; Lunar regolith; Lunar samples; Molecular hydrogen; Recombinative desorption; Temperature programme; Thermal evolution; Ultra-high; Vacuum interfaces; Volatile; Activation energy; Parnassius apollo |
语种 | 英语 |
来源期刊 | Earth and Planetary Science Letters |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/203155 |
作者单位 | School of Chemistry and Biochemistry, Georgia Institute of Technology, Atlanta, GA, United States; Center for Space Technology and Research, Georgia Institute of Technology, Atlanta, GA, United States; John Hopkins, Applied Physics Laboratory, Laurel, MD, United States; School of Physics, Georgia Institute of Technology, Atlanta, GA, United States |
推荐引用方式 GB/T 7714 | Jones B.M.,Aleksandrov A.,Hibbitts C.A.,et al. Thermal evolution of water and hydrogen from Apollo lunar regolith grains[J],2021,571. |
APA | Jones B.M.,Aleksandrov A.,Hibbitts C.A.,&Orlando T.M..(2021).Thermal evolution of water and hydrogen from Apollo lunar regolith grains.Earth and Planetary Science Letters,571. |
MLA | Jones B.M.,et al."Thermal evolution of water and hydrogen from Apollo lunar regolith grains".Earth and Planetary Science Letters 571(2021). |
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