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Chang'e-6 Samples Confirm First Crystalline Hematite and Maghemite on the Moon

Peer-reviewed analyses point to impact-vapor oxidation as the likely formation mechanism.

Overview

  • A team from IGCAS and Shandong University identified micron-scale hematite (α‑Fe2O3) and maghemite (γ‑Fe2O3) in soil returned from the South Pole–Aitken Basin by China's Chang'e‑6 mission.
  • Science Advances published the findings on November 14, providing direct mineralogical evidence of highly oxidized iron phases in lunar material.
  • Electron microscopy, electron energy loss spectroscopy and Raman spectroscopy confirmed the crystal structures and lunar origin of the grains, ruling out terrestrial contamination.
  • Researchers propose that large impacts created brief high‑oxygen‑fugacity vapor conditions that oxidized iron released from minerals such as troilite and deposited it as micron-sized Fe2O3.
  • The minerals occur alongside magnetite, reinforcing prior hints from Chang'e‑5 and remote sensing and offering new clues to persistent lunar magnetic anomalies and the Moon’s redox evolution.