Unraveling the India-Eurasia Collision Pattern: Insights from Subduction to Collision-Related Magmatism in the Chagai Hills

Guangping Zeng , Yunying Zhang , Zhen Sun , Mubashir Mehmood , Syed Ahsan Hussain Gardezi , Xiuquan Miao , Liheng Sun , Xuqing Li

Journal of Earth Science ›› : 1 -15.

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Journal of Earth Science ›› :1 -15. DOI: 10.1007/s12583-025-0244-z
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Unraveling the India-Eurasia Collision Pattern: Insights from Subduction to Collision-Related Magmatism in the Chagai Hills
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Abstract

The pattern of India-Eurasia collision is critical for understanding plateau uplift and Cenozoic global climate change. However, the initial collisional timing and location remain debated. This study investigates magmatic rocks from the Chagai Hills in the western India-Eurasia collision zone, integrating petrological, geochronological and geochemical analyses of andesites (56.2 Ma), granodiorites (50.0 Ma) and granites (51.6–47.5 Ma). The arc-like andesites with depleted Nb-Ta-Ti, low 87Sr/86Sr of 0.704 2–0.705 1 and high εNd(t) of 4.3–4.5, reflect a subduction-modified mantle origin. Granodiorites display adakitic features, including elevated Sr/Y (>131) ratios and high Sr (>761 ppm) but low Y (<6.26 ppm) concentrations as well as high Mg# (53–61) values, Cr (up to 122 ppm) and Ni (up to 44.5 ppm) contents, pointing to a derivation from interaction of delaminated lower crustal melts with mantle peridotite under a collision-related setting. The I-type granites with low initial 87Sr/86Sr of 0.704 1–0.704 4 and high εNd(t) (4.0–4.2) values were likely originated from juvenile lower crustal melts. Coupled with regional geological and paleogeographic data, it is suggested that the 56.2 Ma arc andesites were formed during the subduction of the Neo-Tethys Ocean, while the delamination-related adakitic granodiorites (50.0 Ma) and lower crust-derived granites (51.6–47.5 Ma) were produced during the collisional stage. Therefore, the tectonic transition from subduction to collision in the Chagai area occurred between 56.2 and 51.6 Ma. Obviously, the collision in the Chagai area took place later than the initial collision in the central India-Eurasia collision zone (Gangdese, ∼59 ± 1 Ma), supporting a diachronous collision model that collision initiated in the center zone and subsequently propagated laterally.

Keywords

India-Eurasia collision pattern / Chagai Hills / magmatism / transition from subduction to collision / geochemistry

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Guangping Zeng, Yunying Zhang, Zhen Sun, Mubashir Mehmood, Syed Ahsan Hussain Gardezi, Xiuquan Miao, Liheng Sun, Xuqing Li. Unraveling the India-Eurasia Collision Pattern: Insights from Subduction to Collision-Related Magmatism in the Chagai Hills. Journal of Earth Science 1-15 DOI:10.1007/s12583-025-0244-z

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