Submicroscopic magnetite may be ubiquitous in lunar regolith of high-Ti region

The research team led by Li Yang and Cao Zhi at the Institute of Geochemistry of the Chinese Academy of Sciences confirmed for the first time that submicroscopic magnetite particles are common throughout the lunar surface. This information updates our understanding of the lunar microscale oxidation environment.

Researchers conducted in-situ electron microanalysis of droplet-like, rounded iron-sulfide grains embedded within impact glasses in the finest Chang’e-5 lunar soil and confirmed that impact-induced submicroscopic magnetite is ubiquitous in the lunar regolith. The content of magnetite is closely related to the Ti content in the region.

Magnetite is an important oxidized mineral in planetary science and its presence is related to paleomagnetic fields and indicators of life. It is commonly believed to be rare on the reduced lunar surface.

Although Mössbauer spectroscopy and electron spin resonance (ESR) studies have hypothesized the prevalence of submicroscopic “magnetite-like” phases in Apollo lunar soils, there is no correlative mineralogical evidence for their genesis and potential distribution on the moon.

Li and Cao’ s study showed that a large number of submicroscopic magnetite particles existed in the droplet-like, rounded iron-sulfide grains embedded within impact glasses, and the content of magnetite is positively correlated with the Ti content in the glass. Microanalysis showed that this type of magnetite is induced by the impact event.

The researchers used the eutectoid reaction mechanism (4FeO = Fe₃O₄ + Fe) to explain its formation.

Statistical results showed that seven droplet-like iron-sulfide grains with magnetite on the surface of about 200 glassy grains. The sulfide-droplet-on-glass assemblage is common but has a certain probability, and the formation of magnetite conforms to the rule emphasized in relation to the Ti content in the impact glass.

“We believe that the submicroscopic magnetite in the droplet-like iron-sulfide grains provides in-situ mineralogical proof of the sub-microscopic ‘magnetite-like’ phases recognized during the Apollo era,” said Li Yang, “This provides a solid basis for the conclusion that impact-induced submicroscopic magnetite may be ubiquitous in the lunar regolith of the high-Ti region.”

The study was published in the journal Science Advances on September 20.

Potentially ubiquitous production of ferromagnetic minerals reported in this study also provides further support for an impact-induced mechanism for lunar surface magnetic anomalies in previous studies.

The sulfides in the liquid outer core and ilmenite carried by the early lunar mantle overturning events came into contact with each other in the high-pressure environment (~4.75 GPa) of the lunar core-mantle boundary. This may have resulted in the presence of dissolved oxygen in the sulfide and the formation of magnetite in the deep moon.