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Distribution and Processing of Highly Siderophile Elements in Cratonic Mantle Lithosphere
Author(s) -
Sonja Aulbach,
James E. Mungall,
D. Graham Pearson
Publication year - 2015
Publication title -
reviews in mineralogy and geochemistry
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 5.63
H-Index - 119
eISSN - 1943-2666
pISSN - 1529-6466
DOI - 10.2138/rmg.2016.81.5
Subject(s) - mantle (geology) , geology , geochemistry , lithosphere , mineral redox buffer , mantle wedge , platinum group , chromite , chemistry , platinum , paleontology , tectonics , biochemistry , catalysis
Cratonic lithospheric mantle is composed of predominantly refractory materials that formed at higher mantle potential temperatures ( T P) than recorded in non-cratonic peridotites. It also shows stronger depletion and fractionation of Pd and Pt from Ru, Os and Ir than oceanic, supra-subduction zone or off-cratonic lithospheric mantle, as well as some of the lowest Se and Te contents. The varied response of the highly siderophile elements (HSE: Os, Ir, Ru, Rh, Pt, Pd, Re, Au), and their embedded radioactive decay systems, to changes in oxygen fugacity ( f O2), sulfur fugacity ( f S2) and pressure ( P )—in particular through the impact of these parameters on the stability of the main HSE-bearing sulfide and alloy phases makes them potentially powerful tracers of their melting environment. Therefore, investigation of the HSE systematics of cratonic mantle peridotites, in combination with information from Re–Os isotopes on time-integrated enrichment or depletion, can help us to understand processes leading to mantle differentiation and continental lithosphere formation in the Archean, which are controversial subjects despite decades of research.The longevity of the cratonic lithosphere implies that there was ample opportunity for secondary overprint, obscuring our view of earlier processes. For example, destabilization of platinum-group element (PGE: Os, Ir, Ru, Rh, Pt, Pd) alloy leading to depletions in the compatible PGE, and perhaps Pt, in some cratonic mantle samples may occur in an oxidizing mantle wedge or through interaction with oxidizing small-volume, volatile-rich melts that typically invade cratonic roots. Such melts may eventually deposit S, Pd, Pt and Re and also capture remaining PGE alloys, consistent with the anomalous S-rich character of many kimberlite-borne xenoliths. Their basalt-borne counterparts show additional late effects of subaerial degassing that can deplete volatile elements (S, Re, Os). Basaltic melts can also scavenge PGE alloys at depth, while still sulfide-undersaturated. Such melts, may, …

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