EGU23-4201
https://doi.org/10.5194/egusphere-egu23-4201
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Reassessment of the Phanerozoic net crustal growth: U–Pb and Hf zircon data for the Central Asian Orogenic Belt

Ariuntsetseg Ganbat1,2,3, Tatsuki Tsujimori2,4, Daniel Pastor-Galán5,6, and Alexander Webb1
Ariuntsetseg Ganbat et al.
  • 1Department of Earth Sciences, The University of Hong Kong, Pokfulam Road, Hong Kong
  • 2Graduate School of Science, Tohoku University, Aoba, Sendai 980-8578, Japan
  • 3Geoscience Center, Mongolian University of Science and Technology, Ulaanbaatar 120646, Mongolia
  • 4Center for Northeast Asian Studies, Tohoku University, Aoba, Sendai 980-8576, Japan
  • 5Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Aoba, Sendai 980-0845, Japan
  • 6Department of Geodynamics, University of Granada, Granada, Spain

The Central Asian Orogenic Belt (CAOB) consists of several continental blocks, was assembled during the Phanerozoic, and preserves large volumes of Phanerozoic granitoids with juvenile Nd and Hf isotope characteristics, and thus regarded as the largest site of Phanerozoic continental growth on Earth. Nonetheless, it remains disputed whether the significant crustal additions occurred during the Phanerozoic. We compiled available zircon U–Pb geochronological and Hf-in-zircon isotopic data for granitoids from the orogenic segments of CAOB. Using this data, we estimated the percentage of juvenile versus evolved crustal portions in different Phanerozoic time slices of the CAOB.     

The areal distribution of Hf isotopic information shows a younging trend in the Hf model age and radiogenic Hf values from northeast to southwest. For many orogenic segments of the CAOB, the range of hafnium isotope signatures for the granitoids shifted towards more radiogenic compositions over time. We interpret these findings to indicate that the lower crust and lithospheric mantle beneath the CAOB continental blocks were largely removed during continuous oceanic subduction and replaced by juvenile crust. Melts of this crust display the radiogenic hafnium signature. The juvenile versus evolved crustal portion estimations in different time slices show that the crustal growth has taken place in a steady-state mode, and the rate of the radiogenic crustal generation is close to overall global averaged rates of crust generation. It follows that Phanerozoic net crustal growth in accretionary orogens, as exemplified by the CAOB, may have been overestimated as it has been compensated by crustal destruction.

How to cite: Ganbat, A., Tsujimori, T., Pastor-Galán, D., and Webb, A.: Reassessment of the Phanerozoic net crustal growth: U–Pb and Hf zircon data for the Central Asian Orogenic Belt, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-4201, https://doi.org/10.5194/egusphere-egu23-4201, 2023.