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The Huai’an gneiss terrane mainly consists of TTG gneisses and dioritic gneisses. Laser in situ U-Pb dating of magmatic zircon cores indicates that protolith of these gneisses was formed at ~2.5 Ga. The TTG gneisses have positive εNd(t) values of 2.7 to 4.3, and most of the magmatic zircons have positive εHf(t) values of 2.0 to 8.3. These positive εNd(t) and εHf(t) values are both similar to those of the contemporaneous depleted mantle at 2.5 Ga. Moreover, the young Hf model ages of 2.44 to 2.73 Ga for the magmatic zircons are close to the timing of the zircons growth. The whole-rock εNd(t) values are lower in the dioritic gneisses (0.8 to 1.7) than in the TTG gneisses due to the involvement of ancient crust in its source. However, many magmatic zircons from the dioritic gneisses have similar εHf(t) values (2.0 to 7.9) to that of the coeval depleted mantle; their Hf model ages of 2.49 to 2.75 Ga are close to the U-Pb ages of zircons. The highest εHf(t) values are close to the value of the depleted mantle, and the relatively high εHf(t) values corresponds to the relatively young Hf model age. These Nd and Hf isotope features suggest that these two types of gneisses of the Huai’an gneiss terrane originated from the juvenile crust at ca. 2.5 Ga.
The Huai’an gneiss terrane mainly consists of TTG gneisses and dioritic gneisses. Laser in situ U-Pb dating of magmatic zirconic cores indicates that the protolith of these gneisses was formed at ~ 2.5 Ga. The TTG gneisses have positive εNd (t) values of 2.7 to 4.3, and most of the magmatic zircons have positive εHf (t) values of 2.0 to 8.3. These positive εNd (t) and εHf (t) values are both similar to those of the contemporaneous depleted mantle at 2.5 Ga. Furthermore, the young Hf model ages of 2.44 to 2.73 Ga for the magmatic zircons are close to the timing of the zircons growth. The whole-rock εNd (t) values are lower in the dioritic gneisses (0.8 to 1.7) than in the TTG gneisses due to the involvement of ancient crust in its source. However, many magmatic zircons from the dioritic gneisses have similar εHf (t) values (2.0 to 7.9) to that of the coeval depleted mantle; their Hf model ages of 2.49 to 2.75 Ga are close to the U-Pb ages of zircons. The highest εHf (t) values are close to the value of the depleted mantle, and the relatively high εHf (t) values correspond to the relatively young Hf model age. These Nd and Hf isotope features suggest that these two types of gneisses of the Huai’an gneiss terrane originated from the juvenile crust at 2.5 Ga.