The combined short-lived 146Sm–142Nd and 182Hf–182W radiogenic isotope systems provide critical insights into early Earth differentiation and long-term preservation of mantle heterogeneities. Although Archean rocks often display resolvable 142Nd and 182W anomalies, these signatures diminish with time due to convective homogenization of the mantle. Proposed origins for these anomalies include early silicate-silicate or metal-silicate differentiation, and heterogeneous incorporation of late-accreted material [e.g., 1-4]. To further investigate these processes, we obtained high-precision 182W isotope data for the 2.7 Ga old Theo’s Flow tholeiites. We show that, in addition to the previously reported 142Nd excess [5], the Theo's Flow tholeiites also have a positive 182W anomaly, indicating the survival of an early-formed mantle domain for nearly 1.8 Ga. The 142Nd anomaly is best attributed to silicate differentiation at ~4.4 Ga, whereas the 182W signature likely reflects incomplete mixing of late-accreted materials, consistent with a ‘grainy’ accretion scenario. Comparison with coeval komatiites from Boston Creek, which were derived from the same mantle plume [6], highlight spatial heterogeneity in the incorporation of late-accreted material at the single plume scale. These findings support inefficient mantle mixing during the Archean and are more consistent with a stagnant-lid tectonic regime than with modern-style plate tectonics.
References: [1] Boyet and Carlson (2006) EPSL 250, 254-268. [2] Puchtel et al. (2016) G3 17, 2168-2193 [3] Touboul et al. (2012) Science 335, 1065-1069 [4] Willbold et al. (2011) Nature 477, 195-199. [5] Debaille et al. (2013) EPSL 373, 83-92. [6] Puchtel et al. (2018) GCA 228, 1-26.