Published January 11, 2017 | Version v1
Journal article Open

Early formation of the Moon 4.51 billion years ago

  • 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.

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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

UChicago Information

Division(s)
Physical Sciences Division
Department(s)
Geophysical Sciences