The origin of enriched mantle beneath São Miguel, Azores

Details The origin of enriched mantle beneath São Miguel, Azores The origin of enriched mantle beneath São Miguel, Azores

Jan 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007gecoa..71..219e&link_type=abstract

Geochimica et Cosmochimica Acta, Volume 71, Issue 1, p. 219-240.

Computer Science

17

Scientific paper

Lavas from the island of São Miguel, Azores Archipelago have long been known to display large radiogenic isotopic variability, that ranges from “depleted” isotopic signatures (e.g. high ɛNd ˜ +5) in the west, typical of many ocean island basalts, to more “enriched” compositions (e.g. low ɛNd ˜ +1) in the east. Here, we further characterise the geochemistry of lavas from this remarkable locality, focussing on the nature and origin of the enriched source. Our new isotope data define a striking, linear array in Nd and Hf isotope space that points towards an unusual, enriched composition below the mantle array. This distinctive Hf Nd isotope signature is associated with elevated values of all three radiogenic Pb isotope ratios. Although the enriched component has certain geochemical similarities to both terrigenous sediments and some samples of the continental mantle lithosphere, such comparisons do not stand closer examination. In the absence of a clear, modern analogue we explore the isotope evolution of some simple, model melt compositions to investigate plausible means of producing an appropriate enriched component. Nd Hf isotope characteristics provide the tightest constraints and can be reproduced by an ancient (˜3 Ga), modest-degree melt (˜2%) from a garnet peridotite source. Currently, modest-degree melts from garnet-bearing sources are found forming some major oceanic islands. Subduction, isolation and later mixing of small amounts (<5%) of such basaltic material with more ubiquitous ambient mantle can account for the isotopic characteristics of the enriched São Miguel source. Yet the incompatible element ratios of the enriched São Miguel lavas do not show “recycled” signatures of near-surface alteration nor subduction zone dehydration. Thus, we infer that the enriched component was originally under-plated basalt, intruded into oceanic mantle lithosphere rather than forming the island edifice itself. Since the extreme isotope compositions of São Miguel reflect unextraordinary, albeit ancient, magmatic fractionation, the general rarity of such signatures indicates the efficiency of mantle processes in homogenising or hiding similar sources.

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