Preprints
https://doi.org/10.5194/egusphere-2024-2100
https://doi.org/10.5194/egusphere-2024-2100
21 Oct 2024
 | 21 Oct 2024
Status: this preprint is open for discussion.

Silurian syn- and post-collision granitic magmatism in the western section of the North Qinling Orogen: Implications for collisional orogenic processes

Hao Lin, Zuochen Li, Xianzhi Pei, Shaowei Zhao, Meng Wang, Hai Zhou, Feng Gao, Mao Wang, and Li Qin

Abstract. The Liqiao and Xianping plutons can provide crucial evidence for the collision-orogeny process of the Proto-Tethys Ocean in the western section of the North Qinling Orogen. In this study, we present petrological, zircon U-Pb geochronological, geochemical, and zircon Lu-Hf isotopic data for these plutons. Both the Liqiao and Xianping plutons are characterized as high-K, calc-alkaline, metaluminous to weakly peraluminous granites, with ages of 429 Ma and 421 Ma, respectively. The Liqiao pluton was classified as I-type granite, displaying positive εHf(t) values ranging from -0.1 to +3.4, and high Mg# values from 37.86 to 48.25. We interpret this to indicate that it was generated by the partial melting of juvenile felsic lower crust, with a contribution from mantle-derived material. In contrast, the Xianping pluton exhibited lower Mg# values (20.40 to 35.11) and negative εHf(t) values (-18.0 to -13.9), consistent with the geochemical characteristics of highly fractionated I-type granite. This suggests that the Xianping pluton formed through the partial melting and extensive fractional crystallization of ancient felsic crust. We propose that the Liqiao pluton originated in a syn-collisional setting, while the Xianping pluton formed in a post-collisional environment. Both plutons are products of the collisional orogeny between the Yangtze Block and the North Qinling Orogen, which were associated with the closure of the Wushan-Shangdan Ocean, the northern of the Proto-Tethys Ocean.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this preprint. The responsibility to include appropriate place names lies with the authors.
Hao Lin, Zuochen Li, Xianzhi Pei, Shaowei Zhao, Meng Wang, Hai Zhou, Feng Gao, Mao Wang, and Li Qin

Status: open (until 25 Dec 2024)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2024-2100', Mark Allen, 23 Oct 2024 reply
    • AC1: 'Reply on RC1', Hao Lin, 04 Nov 2024 reply
Hao Lin, Zuochen Li, Xianzhi Pei, Shaowei Zhao, Meng Wang, Hai Zhou, Feng Gao, Mao Wang, and Li Qin
Hao Lin, Zuochen Li, Xianzhi Pei, Shaowei Zhao, Meng Wang, Hai Zhou, Feng Gao, Mao Wang, and Li Qin

Viewed

Total article views: 137 (including HTML, PDF, and XML)
HTML PDF XML Total Supplement BibTeX EndNote
82 39 16 137 22 3 3
  • HTML: 82
  • PDF: 39
  • XML: 16
  • Total: 137
  • Supplement: 22
  • BibTeX: 3
  • EndNote: 3
Views and downloads (calculated since 21 Oct 2024)
Cumulative views and downloads (calculated since 21 Oct 2024)

Viewed (geographical distribution)

Total article views: 135 (including HTML, PDF, and XML) Thereof 135 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 20 Nov 2024
Download
Short summary
There is still considerable controversy over the duration of the subduction-collision orogeny process of the Wushan-Shangdan Ocean. Here, we present new geochronological and geochemical data for Silurian granites from the North Qinling Orogen. The main conclusions are as follows: (1) the ocean had closed prior to 438 Ma; (2) The transition phase from syn-collision to post-collision took place between 429 and 421 Ma; (3) A three-stage tectonic model of the Wushan-Shangdan Ocean is proposed.