EGU25-4835, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-4835
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 01 May, 08:30–10:15 (CEST), Display time Thursday, 01 May, 08:30–12:30
 
Hall X2, X2.49
Short-lived Arc Magmatism in the Arabia-Eurasia Collision Zone with Implications for Continental Crust Formation
Sun-Lin Chung1,2, Yu-Chin Lin1,2, A. Feyzi Bingöl3, Xian-Hua Li4, Jin-Hui Yang4, and Hao-Yang Lee1
Sun-Lin Chung et al.
  • 1Institute of Earth Sciences, Academia Sinica, Taipei, Taiwan (sunlin@ntu.edu.tw)
  • 2Department of Geosciences, National Taiwan University, Taipei, Taiwan
  • 3Department of Geological Engineering, Firat University, Elaziğ, Turkey
  • 4Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China

Arc-continent collision plays a key role in the formation of continental crust. However, details on the processes remain unclear particularly in old collision zones where geologic records are incomplete. Here we present a high-resolution age and geochemical dataset of Late Cretaceous magmatic rocks from Elazig area, SE Turkey along the Arabia-Eurasia collisional orogen. Zircon U-Pb ages obtained by SIMS and LA-ICPMS from 17 samples constrain a short magma duration from 83 to 73 Ma. All the rocks show relative depletions in HFSE (Ti, Nb and Ta), similar to arc lavas from subduction zones. They are heterogeneous (SiO2 = 45-78 wt.%), varying from low-K tholeiitic to calc-alkaline and shoshonitic composition with associated progressive enrichments in LREE and LILE, and change in radiogenic isotopic ratios, such as whole-rock εHf(t) values from +16 to -2. The Elazig magmatism can be explained specifically by a tectonic setting that switched rapidly from an intra-oceanic subduction to arc-continent collision within this part of Tethys where numbers of continental ribbons were present. The geochemical and isotopic variations can be attributed to melting of subducted sediments or mélange diapirs in the mantle wedge, with involvement of the continental materials increasing from 0.5 to 8 vol.%. It is evident that, while the intra-oceanic subduction gave rise to the tholeiitic arc crust from 83 Ma, the soon subsequent arc-continent collision in the region served as an efficient mechanism that transformed the juvenile arc crust toward a more mature continental crust. We argue that similar scenarios may have taken place worldwide in the early stage of collisional orogens, as also exemplified by the present-day Australia-Eurasia collision zone.

How to cite: Chung, S.-L., Lin, Y.-C., Bingöl, A. F., Li, X.-H., Yang, J.-H., and Lee, H.-Y.: Short-lived Arc Magmatism in the Arabia-Eurasia Collision Zone with Implications for Continental Crust Formation, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-4835, https://doi.org/10.5194/egusphere-egu25-4835, 2025.