Journal
EARTH AND PLANETARY SCIENCE LETTERS
Volume 419, Issue -, Pages 168-177Publisher
ELSEVIER
DOI: 10.1016/j.epsl.2015.02.040
Keywords
Archean; mantle; crust; late veneer; tungsten isotopes; Acasta Gneiss Complex
Categories
Funding
- NERC [NE/J018031/2, NE/L004011/1]
- ERC [321209]
- NASA Lunar Science Institute's Center for Lunar Origin and Evolution (CLOE)
- NASA Exobiology Program
- Natural Environment Research Council [NE/J018031/1, NE/J018031/2, NE/L004011/1, NE/J009024/1] Funding Source: researchfish
- NERC [NE/L004011/1, NE/J018031/1, NE/J009024/1, NE/J018031/2] Funding Source: UKRI
- European Research Council (ERC) [321209] Funding Source: European Research Council (ERC)
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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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