TY - JOUR

T1 - Tectonothermal Model and Magmatism Evolution of the Postcollisional (pre-Plume) Stage of the Kara Orogen (Northern Taimyr, Central Arctic)

AU - Vernikovsky, V. A.

AU - Semenov, A. N.

AU - Polyansky, O. P.

AU - Babichev, A. V.

AU - Vernikovskaya, A. E.

AU - Matushkin, N. Yu

N1 - This work was financially supported by the Russian Science Foundation (grants no. 19-17-00091-П and 22-27-00178). Публикация для корректировки.

PY - 2024/1

Y1 - 2024/1

N2 - 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 U–Th–Pb isotope data, the granites have been divided into syncollisional and postcollisional intrusions formed at 315–282 and 264–248 Ma respectively. Our previously published tectonothermal model [1] concerned the syncollisional formation stage of the Kara orogen at 315–282 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 Permian–Triassic boundary. The existence of multiple bodies of allochthonous granitoids aged 265–248 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 orogen’s crust is used alongside geochemical and isotope data that reflects the magmatic sources of the granitoids.

AB - 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 U–Th–Pb isotope data, the granites have been divided into syncollisional and postcollisional intrusions formed at 315–282 and 264–248 Ma respectively. Our previously published tectonothermal model [1] concerned the syncollisional formation stage of the Kara orogen at 315–282 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 Permian–Triassic boundary. The existence of multiple bodies of allochthonous granitoids aged 265–248 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 orogen’s crust is used alongside geochemical and isotope data that reflects the magmatic sources of the granitoids.

KW - Arctic

KW - Kara orogen

KW - Siberian craton

KW - collision

KW - granite

KW - mantle plume

KW - northern Taimyr

KW - thermal model

UR - https://www.scopus.com/record/display.uri?eid=2-s2.0-85179368672&origin=inward&txGid=9f9e32b26f98ad6ea7807a94f17be733

UR - https://www.mendeley.com/catalogue/1b298a29-3a24-3e57-b58d-dbb973f8ff88/

U2 - 10.1134/S1028334X23602699

DO - 10.1134/S1028334X23602699

M3 - Article

VL - 514

SP - 43

EP - 49

JO - Doklady Earth Sciences

JF - Doklady Earth Sciences

SN - 1028-334X

IS - 1

ER -