TY - JOUR
T1 - The discovery of silicon oxide nanoparticles in space-weathered of Apollo 15 lunar soil grains
AU - Gu, Lixin
AU - Zhang, Bin
AU - Hu, Sen
AU - Noguchi, Takaaki
AU - Hidaka, Hiroshi
AU - Lin, Yangting
N1 - Funding Information:
We are grateful to M. S. Thompson and other anonymous reviewers for their constructive reviews. The authors thank Yuchen Xu for sample preparing, Jinan Shi for TEM observation and Hitesh Changela for improving English with the manuscript. The Apollo 15 lunar soil sample was supplied by NASA, JSC. This research was supported by National Natural Science Foundation of China ( 41490631, 41521062 ) and the Key Research Program of Frontier Sciences, CAS (QYZDJ-SSW-DQC001). Bin Zhang also acknowledge the Fundamental Research Funds for the Central Universities of China (Grant Nos. 0903005203553 ).
Publisher Copyright:
© 2017 Elsevier Inc.
PY - 2018/3/15
Y1 - 2018/3/15
N2 - Space weathering is an important process on the Moon and other airless celestial bodies. The most common space weathering effects are amorphization of the top surface of soil grains and formation of nanophase iron particles (npFe) within the partially amorphous rims. Hence, space weathering significantly affects optical properties of the surface of the Moon and other airless celestial bodies. Transmission electron microscope (TEM) analysis of Apollo 15 soil grains displays npFe (≤5 nm in size) embedded in the space-weathered rim (∼60 nm in thickness) of a pyroxene grain, consistent with previous studies. In contrast, submicron-sized fragments that adhere to the pyroxene grain show distinct space weathering features. Silicon oxide nanoparticles (npSiOx) were observed with npFe in a submicron-sized Mg–Fe silicate fragment. This is the first discovery of npSiOx as a product of space weathering. The npSiOx and the coexisting npFe are ∼10–25 nm in size, significantly larger than the typical npFe in the space weathered rim of the pyroxene grain. The coexisting npSiOx and npFe were probably formed directly in micrometeorite shock-induced melt, instead of in a solar-wind generated vapor deposit or irradiated rim. This new observation will shed light on space weathering processes on the Moon and airless celestial bodies.
AB - Space weathering is an important process on the Moon and other airless celestial bodies. The most common space weathering effects are amorphization of the top surface of soil grains and formation of nanophase iron particles (npFe) within the partially amorphous rims. Hence, space weathering significantly affects optical properties of the surface of the Moon and other airless celestial bodies. Transmission electron microscope (TEM) analysis of Apollo 15 soil grains displays npFe (≤5 nm in size) embedded in the space-weathered rim (∼60 nm in thickness) of a pyroxene grain, consistent with previous studies. In contrast, submicron-sized fragments that adhere to the pyroxene grain show distinct space weathering features. Silicon oxide nanoparticles (npSiOx) were observed with npFe in a submicron-sized Mg–Fe silicate fragment. This is the first discovery of npSiOx as a product of space weathering. The npSiOx and the coexisting npFe are ∼10–25 nm in size, significantly larger than the typical npFe in the space weathered rim of the pyroxene grain. The coexisting npSiOx and npFe were probably formed directly in micrometeorite shock-induced melt, instead of in a solar-wind generated vapor deposit or irradiated rim. This new observation will shed light on space weathering processes on the Moon and airless celestial bodies.
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U2 - 10.1016/j.icarus.2017.12.028
DO - 10.1016/j.icarus.2017.12.028
M3 - Article
AN - SCOPUS:85040636057
SN - 0019-1035
VL - 303
SP - 47
EP - 52
JO - Icarus
JF - Icarus
ER -