EGU23-1701, updated on 22 Feb 2023
https://doi.org/10.5194/egusphere-egu23-1701
EGU General Assembly 2023
© Author(s) 2023. This work is distributed under
the Creative Commons Attribution 4.0 License.

Paleomagnetism of Late Triassic Volcanic Rocks From the Southern Qiangtang Block, Tibet: Constrains on the Closure of the Paleo-Tethys Ocean

Bitian Wei1, Xin Cheng1, Mathew Domeier2, and Hanning Wu1
Bitian Wei et al.
  • 1State Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Xi’an 710069, China.
  • 2Centre for Earth Evolution and Dynamics (CEED), University of Oslo, PO Box 1028 Blindern 0316 Oslo, Norway

To better constrain the drift history of the South Qiangtang block and the closure of the Paleo-Tethys Ocean, we report a paleomagnetic result isolated from 25 sites (199 samples) of Late Triassic volcanic rocks from the Xiaoqiebao Formation. The directions of the characteristic remanent magnetization isolated from these rocks pass both fold- and reversal tests, and are likely primary magnetizations. On base of these data, we estimate that the South Qiangtang block occupied a paleolatitude of 30.1°N±4.6 at 222Ma. When combined with existing paleomagnetic constraints, these new results indicate that the South Qiangtang block moved rapidly northward between the middle Permian and Late Triassic, at an average south‐north speed of ~13.4 cm/yr during middle Permian to Late Triassic. Our new data further suggest that the Paleo-Tethys likely closed by ~222Ma, and the north-south width of the Neo- Tethys Ocean was reached ca. 7000 km at this time.

How to cite: Wei, B., Cheng, X., Domeier, M., and Wu, H.: Paleomagnetism of Late Triassic Volcanic Rocks From the Southern Qiangtang Block, Tibet: Constrains on the Closure of the Paleo-Tethys Ocean, EGU General Assembly 2023, Vienna, Austria, 24–28 Apr 2023, EGU23-1701, https://doi.org/10.5194/egusphere-egu23-1701, 2023.