月面土壌中の余剰アルゴン40の地球風起源を提案（Chinese Scientists Propose Excess 40Ar in Lunar Soil Possibly from Earth Wind）

2025-09-28 中国科学院(CAS)

＜関連情報＞

• https://english.cas.cn/newsroom/cas_media/202509/t20250929_1058939.shtml
• https://www.sciencedirect.com/science/article/abs/pii/S0019103525003513

嫦娥5号の月の土壌中の40Arの過剰は地球の風が起源である可能性を示唆している Excess 40Ar in Chang’e-5 lunar soils suggests a possible origin from Earth wind

Li Zhao, Liwu Li, Chunhui Cao, Qingyan Tang, Xianbin Wang
Icarus  Available online: 8 September 2025
DOI:https://doi.org/10.1016/j.icarus.2025.116803

Graphical abstract

Highlights

• Excess ⁴⁰Ar in Chang’e-5 soils exceeds solar wind and ⁴⁰K decay predictions.
• Stepwise heating (200 °C–1300 °C) reveals distinct Ar isotope correlations.
• ⁴⁰Ar linked to ³⁶Ar: Earth wind; isolated ⁴⁰Ar: lunar ⁴⁰K decay.
• Earth wind likely major contributor to ⁴⁰Ar via solar wind mixing.
• Far-side Moon samples (Chang’e-6) may test terrestrial origin hypothesis.

Abstract

The abundance of ⁴⁰Ar in lunar soils is significantly higher than the expected values from solar wind implantation and ⁴⁰K decay, a phenomenon known as ⁴⁰Ar excess. Traditionally, this excess is attributed to ⁴⁰Ar generated by the decay of ⁴⁰K within the Moon. This radiogenic ⁴⁰Ar degasses to the lunar surface, where it is ionized by solar radiation and subsequently captured by lunar soils. However, stepwise heating (200 °C–1300 °C) and degassing analyses of noble gas isotopes in Chang’e-5 lunar soils samples reveal the presence of two types of ⁴⁰Ar: one unrelated to ³⁶Ar, likely originating from in situ ⁴⁰K decay in the soils, and another correlated with ³⁶Ar, which may primarily derive from Earth wind. Earth wind, an ion flux formed by the escape of Earth’s atmosphere, is thought to be injected onto the lunar surface under the regulation of Earth’s magnetosphere. The study proposes that the excess ⁴⁰Ar in lunar soils may primarily stem from the continuous escape of Earth’s atmosphere and be injected onto the lunar surface through both the inner and outer regions of Earth’s magnetosphere, offering a new perspective for understanding volatile exchange between the Earth-Moon system.