Carbon concentrations and isotopic ratios of eclogites from the Dabie and Sulu terranes in China

Both concentration and isotope composition of bulk carbon in apatite and host eclogites from the Dabie–Sulu ultrahigh pressure (UHP) terranes in China have been determined along with their oxygen isotope composition. The results show significant 13C-depletion in the apatite (δ13C=−27.7‰ to −20.8‰) with the carbon concentrations of 0.59 to 1.65 wt.% CO2 despite a large variation in δ18O (−6.5‰ to +9.5‰). The bulk carbon in 21 of the 24 eclogites has low δ13C values of −26.1‰ to −17.9‰ with low carbon content of 500 to 1000 ppm, whereas the other three samples show high δ13C values of −7.1‰ to −2.8‰ with high carbon contents of 2400 to 4300 ppm. Noncarbonate carbon was measured by treating the all eclogites with 5 N HCl solution, yielding uniformly low δ13C values of −27.9‰ to −24.2‰ and carbon contents of 200 to 300 ppm. Carbonate carbon is thus calculated by mass balance to have also low δ13C values of −25.6‰ to −15.1‰ for the 21 samples but high δ13C values of −4.3‰ to −1.2‰ for the remaining three samples. Secondary carbonate was identified in the three eclogites that are also depleted in 13C primarily, but subjected to overprint of 13C-rich CO2-bearing fluid subsequent to the UHP metamorphism. otopically light carbon in both eclogite and apatite is interpreted to represent the isotope composition of carbon in eclogite precursors before plate subduction, and thus has an origin of organic carbon from the Earthʹs surface. The uniformly low δ13C values of apatite suggest that the CO2 of metamorphic fluid in equilibrium with the host-eclogites would be derived from the oxidation of organic carbon rather than the decarbonation of underthrust carbonates during progressive metamorphism. Protoliths of the eclogites are inferred to be of igneous origin, which underwent more extensive interaction with organic matter than with meteoric-hydrothermal fluid on the subsurface of the continental crust. The break off of the subducted plate containing the isotopically light carbon and subsequent interactions with the surrounding mantle could produce the mafic and/or silicic magmas that are significantly depleted in 13C relative to the primary mantle carbon. This may provide evidence for a linkage of the 13C-depleted mantle carbon to a surficial source via plate subduction.