TY - JOUR
T1 - Solar Flare Tracks
T2 - Unveiling Features and Their Impact on Distinct Lunar Soil Transformations
AU - Chen, Yujie
AU - Fang, Yan
AU - Fu, Xiaoqian
AU - Pua, Chenglin
AU - Yuan, Wentao
AU - Guo, Jiangang
AU - Ying, Tianping
AU - Wang, Yong
AU - Ding, Jun
AU - Liu, Suya
AU - Yang, Guang
AU - Chen, Zhen
AU - Zhang, Ze
AU - Meng, Fanqi
AU - Gu, Lin
AU - Chen, Xiaolong
AU - Li, Jinhua
AU - Yu, Qian
N1 - Publisher Copyright:
© 2025 Wiley-VCH GmbH.
PY - 2025/11/19
Y1 - 2025/11/19
N2 - Studying crystal defects is essential for understanding a material's origin, evolution, and behavior. Lunar materials can exhibit defects from space weathering including high-energy ion implantations, which rarely happens on Earth. Investigating the variation in defects’ structure along the direction of implantation and its impact on lunar materials’ transformation is vital, but unfortunately, this remains unclear. Using multi-scale, 3D characterization of lunar olivine from Chang'e-5 mission, it is found that solar flare tracks, common lunar defects induced by implantation, have a “near-linear” structure. These tracks show varied shuffling of oxygen and silicon atoms and vacancies along the traces. Intriguingly, the in situ electron microscopy heating experiments, detected for the first time that the evolution of solar flare tracks leads to the generation of iron nanoparticles and the release of oxygen upon heating. This reaction is rarely observed on Earth and unreported on the Moon before, which produces resources that can be harnessed for future human exploration and the establishment of lunar habitats.
AB - Studying crystal defects is essential for understanding a material's origin, evolution, and behavior. Lunar materials can exhibit defects from space weathering including high-energy ion implantations, which rarely happens on Earth. Investigating the variation in defects’ structure along the direction of implantation and its impact on lunar materials’ transformation is vital, but unfortunately, this remains unclear. Using multi-scale, 3D characterization of lunar olivine from Chang'e-5 mission, it is found that solar flare tracks, common lunar defects induced by implantation, have a “near-linear” structure. These tracks show varied shuffling of oxygen and silicon atoms and vacancies along the traces. Intriguingly, the in situ electron microscopy heating experiments, detected for the first time that the evolution of solar flare tracks leads to the generation of iron nanoparticles and the release of oxygen upon heating. This reaction is rarely observed on Earth and unreported on the Moon before, which produces resources that can be harnessed for future human exploration and the establishment of lunar habitats.
KW - 3D atomic structure
KW - Chang'e-5 lunar soil
KW - in situ TEM heating
KW - solar flare tracks
UR - https://www.scopus.com/pages/publications/105007549322
U2 - 10.1002/adfm.202509781
DO - 10.1002/adfm.202509781
M3 - 文章
AN - SCOPUS:105007549322
SN - 1616-301X
VL - 35
JO - Advanced Functional Materials
JF - Advanced Functional Materials
IS - 47
M1 - 2509781
ER -