Exploring the oxygen and carbon isotopic composition of the Mediterranean red coral (Corallium rubrum) for seawater temperature reconstruction

Abstract Here we provide first evidence that the stable oxygen and carbon isotopic composition (δ 18 O, δ 13 C) of the high-magnesium calcite skeleton red coral Corallium rubrum can be used as a reliable seawater temperature proxy. This is based upon the analyses of living colonies of C. rubrum from different depths and localities in the Western Mediterranean Sea. The assessment of the growth rates has been established through the analysis of growth band patterns. The δ 18 O and δ 13 C compositions show large variability with a significant difference between the branches and the bases of the colonies. In both coral portions, the δ 18 O and δ 13 C values are highly correlated and show well-defined linear trends. Following the “lines technique” approach developed by Smith et al. (2000) for scleractinian aragonitic deep-water corals, our data have been combined with published values for the deep-sea gorgonian corals Isididae and Coralliidae from Kimball et al. (2014) and Hill et al. (2011) resulting in the following δ 18 O temperature equation: T ° C = − 5.05 ± 0.24 × δ 18 O intercept + 14.26 ± 0.43 R 2 = 0.962 p value 0.0001 The error associated with this equation is ± 0.5 °C at the mean temperature of the data set, ± 0.7 °C for corals living in 2 °C water and ± 1 °C for coral living in warmer water (17 °C). The highly significant δ 18 O intercept vs. temperature relationship combined with the “lines technique” method can be reliably applied to the calcitic skeleton to obtain calcification temperature estimates in the past, although this approach requires the knowledge of the past δ 18 O and δ 13 C composition of seawater and it is labor and time intensive.