- Institute of Geology and Geophysics, Chinese Academy of Sciences, China
Lunar soils, formed in the absence of a long-lived atmosphere and a global magnetic field, record volatile inputs from both solar-wind implantation and planetary impacts. For most species, including water and noble gases, solar-wind implantation dominates. Nitrogen, however, behaves fundamentally differently. We present stepwise-heating nitrogen measurements of Chang’e-5 and Chang’e-6 lunar soils, providing the first paired mid-latitude samples from the lunar near side and far side. The Chang’e soils show that most trapped nitrogen is supplied by micro-impactor delivery rather than solar-wind implantation. However, when integrated with low-latitude Apollo and Luna datasets, the combined results reveal that spatial variations in nitrogen isotopic compositions across the Moon are primarily controlled by variations in solar-wind flux.
How to cite: Li, Y., Su, F., Zhang, X., Liu, Z., and He, H.: Volatile nitrogen study of Chang’e-5 and Chang’e-6 soils, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9046, https://doi.org/10.5194/egusphere-egu26-9046, 2026.