Space Weathering of the Chang'e-5 Lunar Sample From a Mid-High Latitude Region on the Moon

被引:67
作者
Gu, Lixin [1 ]
Chen, Yongjin [2 ]
Xu, Yuchen [3 ]
Tang, Xu [1 ]
Lin, Yangting [1 ,4 ]
Noguchi, Takaaki [5 ]
Li, Jinhua [1 ,4 ]
机构
[1] Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
[2] Ctr High Pressure Sci & Technol Adv Res, Beijing, Peoples R China
[3] Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China
[4] Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China
[5] Kyushu Univ, Fac Arts & Sci, Fukuoka, Japan
基金
中国国家自然科学基金;
关键词
Chang'e-5; space weathering; solar wind; micrometeorite impacts; Moon; lunar soil; SURFACE; DISCOVERY; ORIGIN; RIMS;
D O I
10.1029/2022GL097875
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Micrometeorite impacts and solar wind irradiation, the dominant space weathering (SW) processes, largely modified compositions and microtexture of soil materials on the Moon. Here, we report the SW characteristics of the Chang'e-5 lunar soils from mid-high latitude (43.06 degrees N). All mineral phases exposed on the surface of a single basalt clast have a vapor deposit layer, whereas the textures of the solar wind irradiation-damaged zone are dependent on the host mineral species. Nanophase Fe (npFe(0)) particles are spherical in the amorphized zone of pyroxenes, elongated in ilmenite, and irregular on the jagged surface of iron sulfide, but not found in Fe-poor merrillite. Vesicles were found in the damaged zone of ilmenite and merrillite, but with different shapes. The observations were compared to Apollo samples and demonstrate no significant altitude-dependent effects on the SW, which is important for decoding the reflectance spectra of the Moon.
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页数:9
相关论文
共 31 条
[1]  
Assonov S., 1998, LUNAR PLANETARY SCI, DOI [10.1080/01619563409535205, DOI 10.1080/01619563409535205]
[2]   Comparison of space weathering features in three particles from Itokawa [J].
Burgess, K. D. ;
Stroud, R. M. .
METEORITICS & PLANETARY SCIENCE, 2021, 56 (06) :1109-1124
[3]   Phase-dependent space weathering effects and spectroscopic identification of retained helium in a lunar soil grain [J].
Burgess, K. D. ;
Stroud, R. M. .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2018, 224 :64-79
[4]   EFFECTS OF DARKENING PROCESSES ON SURFACES OF AIRLESS BODIES [J].
CASSIDY, W ;
HAPKE, B .
ICARUS, 1975, 25 (03) :371-383
[5]   Microstructure, chemistry, and origin of grain rims on ilmenite from the lunar soil finest fraction [J].
Christoffersen, R ;
Keller, LP ;
McKay, DS .
METEORITICS & PLANETARY SCIENCE, 1996, 31 (06) :835-848
[6]   The discovery of silicon oxide nanoparticles in space-weathered of Apollo 15 lunar soil grains [J].
Gu, Lixin ;
Zhang, Bin ;
Hu, Sen ;
Noguchi, Takaaki ;
Hidaka, Hiroshi ;
Lin, Yangting .
ICARUS, 2018, 303 :47-52
[7]   Space weathering from Mercury to the asteroid belt [J].
Hapke, B .
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS, 2001, 106 (E5) :10039-10073
[8]   The mineralogy and space weathering of a regolith grain from 25143 Itokawa and the possibility of annealed solar wind damage [J].
Harries, Dennis ;
Langenhorst, Falko .
EARTH PLANETS AND SPACE, 2014, 66
[9]  
Keller L., 2001, LUN PLAN SCI C
[10]   Solar energetic particle tracks in lunar samples: A transmission electron microscope calibration and implications for lunar space weathering [J].
Keller, Lindsay P. ;
Berger, Eve L. ;
Zhang, Shouliang ;
Christoffersen, Roy ;
Sandford, Scott .
METEORITICS & PLANETARY SCIENCE, 2021, 56 (09) :1685-1707