Zhang Xian, Liu Yiwei, Zhao Shaofan, Song Jian, Yao Wei, Wang Weihua, Zou Zhigang, Yang Mengfei
Qian Xuesen Laboratory of Space Technology, China Academy of Space Technology (CAST), Beijing 100094, China.
Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China.
Research (Wash D C). 2024 Sep 23;7:0486. doi: 10.34133/research.0486. eCollection 2024.
Melting and solidification of lunar regolith are pivotal for comprehending the evolutionary dynamics of lunar volcanism, geology, and impact history. Additionally, insights gained from these processes can contribute to the advancement of in situ resource utilization technologies, for instance additive manufacturing and resource extraction systems. Herein, we conduct the direct observation of the melting and rapid solidification of lunar particles returned by the Chang'E 5 mission. The melting temperature and melting sequence were obtained. Bubble generation, growth, and release were clearly observed, with a maximum bubble diameter of 5 µm, which is supposed to be according to the release of volatiles that embedded in the particles. During the solidification process, evident crystallization occurred with incremental crystal growth rate approximately of 27 nm/s. Scanning electron microscopy and energy-dispersive x-ray spectroscopy results verified that the Fe-rich mineral crystalizes first. These results would improve the understanding of the evolution of lunar volcanism, geology, and impact history.
月球风化层的熔化和凝固对于理解月球火山活动、地质和撞击历史的演化动力学至关重要。此外,从这些过程中获得的见解有助于推进原位资源利用技术的发展,例如增材制造和资源提取系统。在此,我们对嫦娥五号任务带回的月球颗粒的熔化和快速凝固进行了直接观测。获得了熔化温度和熔化顺序。清晰地观察到气泡的产生、生长和释放,最大气泡直径为5微米,这应该是由于颗粒中所含挥发物的释放所致。在凝固过程中,出现了明显的结晶现象,晶体生长速率逐渐增加,约为27纳米/秒。扫描电子显微镜和能量色散X射线光谱分析结果证实,富铁矿物最先结晶。这些结果将有助于增进对月球火山活动、地质和撞击历史演化的理解。