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Tungsten isotope composition of the Acasta Gneiss Complex

Abstract : High-precision tungsten (W-182/(184)w) isotope measurements on well-characterised mafic and felsic samples of the ca. 3960 Ma Acasta Gneiss Complex (AGC; Northwest Territories, Canada) show radiogenic epsilon W-182 values between +0.06 to +0.15. Two ca. 3600 Ma felsic samples from this terrane have epsilon W-182 similar to 0 and are the oldest samples so far documented to have a W isotopic composition indistinguishable from that of the modern mantle. The epsilon W-182 data are correlated with epsilon Nd-142 (Roth et al., 2014) and we attribute this variability to incomplete metamorphic homogenisation of the 3960 Ma protolith with more recent material in a 3370 Ma tectono-thermal event. Notably, the value of the positive epsilon W-182 anomalies seen in the 3960 Ma AGC samples that are least affected by metamorphic homogenisation is comparable to that observed in other early Archean rocks (Isua Supracrustal Belt, Greenland; Nuvvuagittuq Supracrustal Belt, Canada) and the late Archean Kostomuksha komatiites (Karelia). This demonstrates a globally constant signature. We infer that the presence of a pre-late veneer mantle represents the most straightforward interpretation of a uniform distribution of epsilon W-182 similar to +0.15 value in Archean rocks of different ages. We show that such a notion is compatible with independent constraints from highly siderophile element abundances in mafic and ultra-mafic Archean mantle-derived rocks. The absence of anomalous epsilon W-182 and epsilon Nd-142 so far measured in samples younger than ca. 2800 Ma suggests progressive convective homogenisation of silicate reservoirs. The downward mixing of an upper mantle rich in late-delivered meteoritic material might account for these combined observations. (C) 2015 The Authors. Published by Elsevier B.V.
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https://hal-univ-lyon1.archives-ouvertes.fr/hal-02340929
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M. Willbold, S. J. Mojzsis, H. -W. Chen, T. Elliott. Tungsten isotope composition of the Acasta Gneiss Complex. Earth and Planetary Science Letters, Elsevier, 2015, 419, pp.168-177. ⟨10.1016/j.epsl.2015.02.040⟩. ⟨hal-02340929⟩

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