Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
5784738 | Precambrian Research | 2017 | 13 Pages |
â¢Lu-Hf isotopes of detrital zircons from two Precambrian successions were in situ analyzed to constrain the Precambrian crustal evolution of Hainan Island.â¢The generation of juvenile curst in Hainan Island predominantly occurred at ca. 2.7 Ga and ca. 1.5-1.0 Ga, respectively.â¢Precambrian crustal evolution of Hainan Island characterized episodic crustal growth mode at 2.7 Ga, 2.3 Ga and 2.1-1.8 Ga, respectively.â¢Hainan Island might be not a part of the Cathaysia Block of South China before or during the Rodinia assembly.
Combined with the previous detrital zircons U-Pb ages of the two Precambrian successions, i.e. the Shilu Group and the Shihuiding Formation in Hainan Island of South China, the in situ Lu-Hf isotopes of detrital zircons were performed to evaluate the growth and reworking of Hainan Island continental crust during Precambrian. The results of 171 Hf-isotopic analyses on zircon grains from the Shihuiding Formation yield 176Hf/177Hf ratios between 0.280786 and 0.281188, 176Lu/177Hf ratios between 0.000228 and 0.003388, Hf model ages (TDMC) between 3.8 Ga and 1.2 Ga, and εHf(t) values ranging from â12.5 to +10.6. The analyzed results of 272 Hf-isotopic data on zircon grains from the Shilu Group exhibit a wide range of 176Hf/177Hf ratios (0.280810-0.282512), 176Lu/177Hf ratios (0.000062-0.004060), TDMC ages (3.7 Ga-1.1 Ga), and εHf(t) values (â20.5 to +12.3).The continental crust of Hainan Island maybe appeared firstly at ca. 4.0-3.8 Ga and then was reworked. The 91.8% of detrital zircon grains from the Shihuiding Formation and 93.8% of the ones from the Shilu Group have crustal incubation time larger than 300 Ma, indicating an involvement of reworked materials into the sedimentation of both the successions. Unambiguously, the crustal basement rocks in Hainan Island were formed mainly through reworking the previous continental components with minor input of juvenile materials. The generation of juvenile curst in Hainan Island predominantly occurred at ca. 2.7 Ga and ca. 1.5-1.0 Ga, which are consistent with that for the assembly of the Kenorland, and the Columbia breakup and subsequent amalgamation of the Rodinia, respectively. The present study further reveals that the crustal growths in Hainan Island are present at 2.7 Ga, 2.3 Ga and 2.1-1.8 Ga, which is more favorable to the episodic growth mode. Moreover, a rough trend of decreasing maximum crustal incubation time of Hainan Island demonstrates that the incubation time of the juvenile crust is shorter when compared with that of the Cathaysia Block in the late Mesoproterozoic. Link to the previously reported geological works, we consider that Hainan Island did not share the same evolution history with the Cathaysia Block of South China during Precambrian.