EGU23-2901, updated on 11 Apr 2024
https://doi.org/10.5194/egusphere-egu23-2901
EGU General Assembly 2023
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Implications of zircon Th/U for global continental crustal evolution and geodynamics

Yujing Wu1, Xianjun Fang2, and Jianqing Ji3
Yujing Wu et al.
  • 1School of Earth and Space Sciences, Peking University, Beijing, China (1901110590@pku.edu.cn)
  • 2School of Earth and Space Sciences, Peking University, Beijing, China (xianjun.fang@erdw.ethz.ch)
  • 3School of Earth and Space Sciences, Peking University, Beijing, China (grsange@pku.edu.cn)

The continental crust is formed by the mantle’s successive crystallization differentiation and then aggregation, which is the result of the continuous energy acquisition and evolution of the mantle. This process has been objectively recorded in the growth of zircons which are widely present in the continental crust, owing to the close relationship between the zircon Th/U ratio and the crystallization temperature of zircons. As shown by theoretical calculations, phenomenon statistics, and/or crystallization simulations, higher zircon Th/U generally indicates higher zircon (re)crystallization temperature in metamorphic and magmatic systems. Here, we compiled ~600,000 zircon Th/U data from the global continental crust and obtained the time series of zircon Th/U ratios. The average level of the Th/U ratio in global zircons has a slow growth trend from old to new and fluctuates quasi-periodically around 0.5. There are two significant cycles of zircon Th/U ratios, ca. 600 and 120 Myr, which are associated with the supercontinent cycle and whole-mantle convection, respectively. It is inferred that the zircon Th/U periodicity is related to the periodic thermal state changes in the mantle, which might be regulated by tidal energy dissipation.

How to cite: Wu, Y., Fang, X., and Ji, J.: Implications of zircon Th/U for global continental crustal evolution and geodynamics, EGU General Assembly 2023, Vienna, Austria, 23–28 Apr 2023, EGU23-2901, https://doi.org/10.5194/egusphere-egu23-2901, 2023.