Mixing model parameters

MA Michael A. Antonelli
JK Jillian Kendrick
CY Chris Yakymchuk
MG Martin Guitreau
TM Tushar Mittal
FM Frédéric Moynier
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In order to account for the three most important parameters indicative of sediment assimilation in NSB TTGs (high δ18O, high A/CNK, and low δ44Ca) we chose to perform three end-member mixing calculations in A/CNK vs. δ18O and δ44Ca vs. δ18O parameter space, with the results shown in Fig. 3 of the main text. We use (i) average shale22,5518O = +15‰, A/CNK = 1.87, and [Ca] = 1 wt%] with δ44Ca = −0.3‰ [the average value from shale standards SGR-1 and SBC-139,44,56,57], (ii) average TTG (δ18O = +6.5‰, A/CNK = 1.02, and [Ca] = 2 wt%) with δ44Ca = −0.25‰ (this study), and (iii) average carbonate [δ18O = +26‰, A/CNK = 0.18, and [Ca] = 40 wt%22] with δ44Ca = −1.25‰ (corresponding to precipitation from BSE-like seawater). The A/CNK of average carbonate comes from a compilation of data for Phanerozoic limestones with available Al2O3, CaO, Na2O, and K2O concentrations (n = 908) from the Earthchem database (http://www.earthchem.org/portal downloaded June 26, 2020, Supplementary Data 5). We note that assimilation of average continental crust cannot lead to high enough A/CNK or δ18O values [shown in Fig. 3 of the main text22,58] to explain the composition of our NSB samples.

We assume that (i) all three end-members have equivalent [O] concentrations, (ii) A/CNK mixes linearly, and that (iii) δ44Ca is dependent on [Ca] and thus produces curved mixing lines in δ44Ca vs. [Ca] parameter space (cf. straight mixing lines in ref. 59). For NSB sample INO5003, we find that an assimilated sediment fraction (80% shale with 20% carbonates) of ~0.3 explains the A/CNK, δ18O, and δ44Ca values, while sample INO5012 requires a sediment fraction of ~0.5 (95% shale with 5% carbonates). The mixing calculations yield final [Ca] concentrations for INO5003 and INO5012 of 4.0 and 2.5 wt%, respectively, which is moderately (but not grossly) higher than measured by Q-ICP-MS (Supplementary Data 1), potentially suggesting that the average [Ca] used in our mixing models (for the TTG and/or shale end-members) may be slightly high. Lower [Ca] estimates for TTG and shale end-members would mainly serve to lower [Ca] in the resulting mixtures but would not lead to significant differences in the estimated sediment fractions (due to the overwhelming influence of carbonate [Ca] on δ44Ca). The similar estimates for sediment fractions in both A/CNK vs. δ18O and δ44Ca vs. δ18O space, however, suggest that our mixing models are relatively robust and that the estimated parameters (e.g., δ44Ca of Eoarchean carbonates) are reasonable.

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