CRUSTAL AND TECTONIC EVOLUTION OF ACCRETIONARY OROGENS IN NE ASIA
The majority of granitoids in the NEAOB formed from Jurassic to late Cenozoic, with Cretaceous as the dominant period of felsic magmatism and silicic volcanism. Though remnants of Paleozoic granitoids have been preserved in Japan, most granitic rocks were emplaced in the Mesozoic and Cenozoic times. Cretaceous granitoids are widespread in Sikhote-Alin and Japan, whereas Cenozoic granitoids occur only in Sakhalin and Hokkaido. Cretaceous to Paleogene granitoids from Sikhote-Alin share the same geochemical and Sr-Nd isotopic signatures as those from SW Japan. Likewise, Cenozoic granitoids of Hokkaido and Sakhalin have remarkably similar chemical and isotopic characteristics. Geochemical and isotopic data suggest that the granitoids from the NEAOB were generated by melting of sources with mixed lithologies, including subducted accretionary complexes and probably some hidden older basement rocks. However, Nd isotopic data also suggest that a significant amount of juvenile crust was produced and added to the NEAOB.
Many workers have proposed geological correlations between Sikhote-Alin and Japan, and between Sakhalin and Hokkaido. Our age and geochemical work lends support to the general scenario. However, a significant difference between SW Japan and NE Japan in crustal composition and probably tectonic evolution has to be reckoned. The two geologic entities might have evolved in very different ways.