Overview
- The research team identified seven microscopic, olivine-bearing clasts whose Fe/Mn ratios, NiO and CrO contents, and oxygen and silicon isotopes match CI carbonaceous chondrites.
- Textural evidence shows the clasts are porphyritic impact-melt fragments that cooled rapidly after an asteroid strike on the lunar surface.
- The discovery provides the first direct physical evidence that fragile CI chondrites struck the Moon and can persist in lunar regolith.
- The authors estimate CI-like material may be much more common in the lunar impact record—potentially approaching 30 percent—underscoring biases in Earth’s meteorite collections.
- The samples from the South Pole–Aitken Basin also underpin reports of two far-side basaltic episodes (~4.2 and ~2.8 billion years ago) and signs of a transient magnetic field near 2.8 billion years ago.