Scientists clarify origins of lunar metallic iron

In a study published in Nature Astronomy, Profs. Shen Laiquan, Bai Haiyang, et al. from Prof. Wang Weihua’s group at the Institute of Physics of the Chinese Academy of Sciences have clarified the respective effects of irradiation and impacts on the formation of metallic iron nanoparticles (npFe⁰).

Based on precise observations of glass beads returned by the Chang’e-5 mission, they showed that the formation of small and large npFe⁰ with distinct optical effects is independently controlled by solar wind irradiation and micrometeorite impacts.

npFe⁰ are widely distributed on the moon, and their accumulation changes the optical spectrum of the lunar surface over time. How the surface color changes depends largely on the size of the npFe⁰: Smaller npFe⁰ redden the reflectance spectra, while larger npFe⁰ cause darkening.

The resultant color variations greatly complicate remote sensing studies, posing long-term puzzles to astronomers. Furthermore, the origin of npFe⁰ of different sizes was not well understood before this study.

npFe⁰ are known as products of space weathering, which includes the two main agents: micrometeorite impacts and solar wind irradiation. Yet the specific roles of these two agents in the formation of different-sized npFe⁰ have been unclear, hindering our understanding of color variations of the lunar surface or asteroids in complex space environments.

“We discovered that the glass beads in the Chang’e-5 lunar soil can preserve iron particles of different sizes, from about 1 nanometer to 1 micrometer,” said Prof. Bai.

“It is generally difficult to distinguish npFe⁰ of different origins observed together in single samples. Here we used the rotation feature of the impact glass beads to clearly distinguish npFe⁰ formed before and after the solidification of the host glass beads.”

In this study, the scientists found numerous discrete large npFe⁰, tens of nanometers in size, which tended to concentrate towards the extremities of the glass beads. This concentration effect can cause ultralarge npFe⁰ to protrude from the extremities.

Such a feature is exactly consistent with the migration phenomenon occurring in rotational glass-forming droplets triggered by hypervelocity impacts. In such scenarios, Fe0 with higher density than the matrix migrates to the extremities driven by centrifugal forces, indicating that these large npFe⁰ were formed in impact-derived melts before the glass beads solidified.

In contrast, they also identified abundant small npFe⁰, several nanometers in size, densely populating the surfaces of the glass beads. These small npFe⁰ exhibit distribution characteristics similar to irradiation-induced vesicle damage.

Along the depth direction of the glass beads, both small npFe⁰ and vesicles gradually decrease in size and abundance, corresponding to the decreasing amount of implanted solar wind ions with increasing depth.

Furthermore, when the size of the lunar grains is smaller than twice the penetration depth of the solar wind ions, small npFe⁰ can completely fill up the tiny grains. These results emphasize that solar wind irradiation is the primary driver of the observed small npFe⁰.

The study demonstrates that solar wind irradiation and micrometeorite impacts both play important but distinct roles in npFe⁰ formation. The independent growth of small and large npFe⁰ revealed in this research matches well with many remote sensing measurements, providing valuable insights for understanding and predicting the optical properties of airless bodies exposed to different space environments.