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Solar Flare Tracks: Unveiling Features and Their Impact on Distinct Lunar Soil Transformations

  • Yujie Chen
  • , Yan Fang
  • , Xiaoqian Fu
  • , Chenglin Pua
  • , Wentao Yuan
  • , Jiangang Guo
  • , Tianping Ying
  • , Yong Wang
  • , Jun Ding
  • , Suya Liu
  • , Guang Yang
  • , Zhen Chen
  • , Ze Zhang
  • , Fanqi Meng
  • , Lin Gu
  • , Xiaolong Chen
  • , Jinhua Li
  • , Qian Yu
  • Zhejiang University
  • Tsinghua University
  • The University of Hong Kong
  • Hainan University
  • CAS - Institute of Physics
  • Thermo Fisher Scientific, Inc.
  • Peking University
  • CAS - Institute of Geology and Geophysics

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

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.

Original languageEnglish
Article number2509781
JournalAdvanced Functional Materials
Volume35
Issue number47
DOIs
StatePublished - 19 Nov 2025

Keywords

  • 3D atomic structure
  • Chang'e-5 lunar soil
  • in situ TEM heating
  • solar flare tracks

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