Paleoproterozoic accretion in the Northeast Siberian craton: Isotopic dating of the Anabar collision system |
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| Authors: | O M Rosen L K Levskii D Z Zhuravlev A Ya Rotman Z V Spetsius A F Makeev N N Zinchuk A V Manakov V P Serenko |
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| Institution: | (1) Geological Institute, Russian Academy of Sciences, Pyzhevskii per. 7, Moscow, 119017, Russia;(2) Institute of Precambrian Geology and Geochronology, Russian Academy of Sciences, nab. Makarova 2, St. Petersburg, 199034, Russia;(3) Institute of Mineralogy and Geochemistry of Rare Elements, Ministry of Natural Resources, Moscow, Russia;(4) Yakutniipromalmaz, AK ALROSA, Mirnyi, Russia;(5) Yakut Research and Geological Prospecting Enterprise, AK ALROSA, Mirnyi, Russia |
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| Abstract: | Geochronological database considered in the work and characterizing the Anabar collision system in the Northeast Siberian craton includes coordinated results of Sm-Nd and Rb-Sr dating of samples from crustal xenoliths in kimberlites, deep drill holes, and bedrock outcrops. As is inferred, collision developed in three stages dated at 2200–2100, 1940–1760, and 1710–1630 Ma. The age of 2000–1960 Ma is established for substratum of mafic rocks, which probably originated during the lower crust interaction with asthenosphere due to the local collapse of the collision prism. Comparison of Sm-Nd and Rb-Sr isochron dates shows that the system cooling from ≈700 to ≈300°C lasted approximately 300 m.y. with a substantial lag relative to collision metamorphism and granite formation. It is assumed that accretion of the Siberian craton resulted in formation of a giant collision mountainous structure of the Himalayan type that was eroded by 1.65 Ga ago, when accumulation of gently dipping Meso-to Neoproterozoic (Riphean) platform cover commenced. |
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| Keywords: | Sm-Nd and Rb-Sr isotopic dating Early Precambrian Earth crust accretion collision kimberlite diamond Siberian craton |
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