We present a tectonothermal model showing the evolution of magmatism during the late Paleozoic postcollisional (pre-plume) development stage of the Kara orogen in northern Taimyr, Central Arctic. The model is based on new and published structural, petrologic, geochemical and geochronological data, as well as thermophysical parameters obtained for the Kara orogen that includes large amounts of syncollisional and postcollisional granites that formed due to the collision of the Kara microcontinent and the Siberian craton. Based on geological, geochemical and UThPb isotope data, the granites have been divided into syncollisional and postcollisional intrusions formed at 315282 and 264248 Ma respectively. Our previously published tectonothermal model [1] concerned the syncollisional formation stage of the Kara orogen at 315282 Ma, during which the emplacement of anatectic granites took place. In this new study, we focus on the evolution of postcollisional magmatism in the orogen at the PermianTriassic boundary. The existence of multiple bodies of allochthonous granitoids aged 265248 Ma in the Kara orogen that predate the extensive eruption of the Siberian traps (˜250 Ma) motivates us to reconstruct the thermal state and melting mechanisms of the crust on the pre-plume stage. To solve this problem, numerical modeling of the thermal, tectonic, and magmatic evolution of the Kara orogens crust is used alongside geochemical and isotope data that reflects the magmatic sources of the granitoids.
