SOLVING THE MYSTERY OF BERMUDA: USING ZN ISOTOPES TO TRACE THE SOURCE OF DEEP CARBON
Stable Zn isotopes (δ66Zn as the ‰ deviation of 66Zn/64Zn from the JMC-Lyon standard) have been used to differentiate various recycled carbon-bearing lithologies in mantle-derived melts [e.g., 2, 3]. Partially melting mantle peridotites (δ66Zn = 0.18 ± 0.06 ‰) can generate slight fractionation in δ66Zn (δ66Zn = 0.28 ± 0.04 ‰), whereas marine carbonates are isotopically heavy (δ66Zn = 0.91 ± 0.24 ‰), making Zn isotope systematics well-suited to trace recycling of carbonates in the mantle.
We present new δ66Zn data to help improve our understanding of the source of the Bermuda SU lavas. Bermuda SU lavas are on the high-end of Zn concentration averages reported for other OIBs ([Zn] = 122.3 ± 18.3 ppm, Zn/Fe⋅104 = 13.4 ± 2.4, n = 23), and while such elevated [Zn] could suggest incorporation of carbonated eclogite in the mantle source, olivine trace element data indicate a carbonated peridotite source instead [1]. Preliminary δ66Zn from Bermuda yields an average of 0.23 ± 0.07‰ (n=6), which implies that Bermuda is the result of partially melting peridotite without significant input from recycled marine carbonates.
[1] Mazza et al. (2019) Nature [2] Beunon et al. (2020) Earth-Science Reviews [3] Zhu et al. (2021) Chemical Geology