Abstract
Trapped xenon isotopes in two Apollo 17 mare basalt fragments are similar to those in primitive meteorites. Xenon would have been effectively excluded from the Moon in the aftermath of its formation in a giant impact. As such, lunar mantle xenon trapped in the mare basalts is best explained as being derived from late accretion occurring before or concurrent with the formation of the lunar crust. The isotopic composition indicates that a combination of comets and carbonaceous chondrites delivered this xenon to the lunar mantle. The inferred mass of accreted cometary ice would have delivered significantly less than a part per million of water to the lunar mantle. The inferred mass of accreted carbonaceous chondrites would have supplied at least a half of a part per million of water. The data further indicate that enstatite chondrites are unlikely to have supplied the majority of late accreted mass.
| Original language | English |
|---|---|
| Article number | 119654 |
| Journal | Earth and Planetary Science Letters |
| Volume | 671 |
| DOIs | |
| State | Published - Dec 1 2025 |
Keywords
- Chondrites
- Comets
- Lunar late accretion
- Noble gas
- Xenon