Mantle transition zone input to kimberlite magmatism near a subduction zone: Origin of anomalous Nd–Hf isotope systematics at Lac de Gras, Canada

• Published in: Earth and planetary science letters 2013-06, Vol.371-372, p.235-251
• Main Authors: Tappe, Sebastian, Graham Pearson, D., Kjarsgaard, Bruce A., Nowell, Geoff, Dowall, David
• Format: Article
• Language: English
• Subjects: convecting upper mantle domains; kimberlite magma origin; mantle transition zone; Nd–Hf isotope decoupling; recycled OIB-type oceanic crust
• ISSN: 0012-821X; 1385-013X
• DOI: 10.1016/j.epsl.2013.03.039

Late Cretaceous–Eocene kimberlites from the Lac de Gras area, central Slave craton, show the most extreme Nd–Hf isotope decoupling observed for kimberlites worldwide. They are characterized by a narrow range of moderately enriched Nd isotope compositions (εNd(i)=−0.4 to −3.5) that contrasts strongly with their moderately depleted to highly enriched εHf(i) values (+3.9 to −9.9). Although digestion of cratonic mantle material in proto-kimberlite melt can theoretically produce steep arrays in Nd–Hf isotope space, the amount of contaminant required to explain the Lac de Gras data is unrealistic. Instead, it is more plausible that mixing of compositionally discrete melt components within an isotopically variable source region is responsible for the steep Nd–Hf isotope array. As development of strongly negative ΔεHf requires isotopic aging of a precursor material with Sm/Nd⪢Lu/Hf for billion-year timescales, a number of models have been proposed where ancient MORB crust trapped in the mantle transition zone is the ultimate source of the extreme Hf isotope signature. However, we provide a conceptual modification and demonstrate that OIB-type domains within ancient subducted oceanic lithosphere can produce much stronger negative ΔεHf during long-term isolation. Provided that these OIB-type domains have lower melting points compared with associated MORB crust, they are among the first material to melt within the transition zone during thermal perturbations. The resulting hydrous alkali silicate melts react strongly with depleted peridotite at the top of the transition zone and transfer negative ΔεHf signatures to less dense materials, which can be more easily entrained within upward flowing mantle. Once these entrained refertilized domains rise above 300km depth, they may become involved in CO2- and H2O-fluxed redox melting of upper mantle peridotite beneath a thick cratonic lid. We argue that incorporation of ancient transition zone material, which includes ultradeep diamonds, into the convecting upper mantle source region of Lac de Gras kimberlites was due to vigorous mantle return flow. This occurred in direct response to fast and complex subduction along the western margin of North America during the Late Cretaceous. [Display omitted] •Lac de Gras (LDG) kimberlites show extreme Nd–Hf isotope decoupling.•Recycled OIB materials from Transition Zone (TZ) impart low ΔεHf to kimberlites.•LDG kimberlites originate from convecting upper mantle with minor TZ entrainmen