Published January 11, 2017
| Version v1
Journal article
Open
Early formation of the Moon 4.51 billion years ago
Creators
- 1. University of California, Los Angeles
- 2. University of Chicago
- 3. Princeton University
Description
Establishing the age of the Moon is critical to understanding solar system evolution and the formation of rocky planets, including Earth. However, despite its importance, the age of the Moon has never been accurately determined. We present uranium-lead dating of Apollo 14 zircon fragments that yield highly precise, concordant ages, demonstrating that they are robust against postcrystallization isotopic disturbances. Hafnium isotopic analyses of the same fragments show extremely low initial 176Hf/177Hf ratios corrected for cosmic ray exposure that are near the solar system initial value. Our data indicate differentiation of the lunar crust by 4.51 billion years, indicating the formation of the Moon within the first ~60 million years after the birth of the solar system.
Data availability
All data needed to evaluate the conclusions in the paper are present in the paper and/or the Supplementary Materials. Additional data related to this paper may be requested from the authors.Files
sciadv.1602365.pdf
Files
(822.1 kB)
| Name | Size | Download all |
|---|---|---|
|
Supplementary materials md5:f90a4a808c509bdad45a20b39086ce9a |
554.7 kB | Preview Download |
|
Article md5:9e8b9dd57730899fec7562c1874c08a9 |
267.3 kB | Preview Download |
Additional details
Identifiers
- DOI
- 10.1126/sciadv.1602365
- Other
- oai:uchicago.tind.io:10988
Funding
- Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
- P300P2_147740
- National Aeronautics and Space Administration
- NNX16AD35G
- National Aeronautics and Space Administration
- NNX15AH43G