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Mantle plumes are oxidised

Author(s)
Moussallam, Yves  
Longpre, Marc-Antoine  
McCammon, Catherine  
Gomez-Ulla, Alejandra  
Rose-Koga, Estelle  
Scaillet, Bruno  
Peters, Nial  
Gennaro, Emanuela  
Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Palermo, Palermo, Italia  
Paris, Raphael  
Oppenheimer, Clive  
Language
English
Obiettivo Specifico
3V. Proprietà chimico-fisiche dei magmi e dei prodotti vulcanici
Status
Published
JCR Journal
JCR Journal
Journal
Earth and Planetary Science Letters  
Issue/vol(year)
/527 (2019)
Pages (printed)
115978
Date Issued
2019
DOI
10.1016/j.epsl.2019.115798
URI
https://www.earth-prints.org/handle/2122/13545
Abstract
From oxic atmosphere to metallic core, the Earth’s components are broadly stratified with respect to oxygen fugacity. A simple picture of reducing oxygen fugacity with depth may be disrupted by the accumulation of oxidised crustal material in the deep lower mantle, entrained there as a result of subduction. While hotspot volcanoes are fed by regions of the mantle likely to have incorporated such recycled material, the oxygen fugacity of erupted hotspot basalts had long been considered comparable to or slightly more oxidised than that of mid-ocean ridge basalt (MORB) and more reduced than subduction zone basalts. Here we report measurements of the redox state of glassy crystal-hosted melt inclusions from tephra and quenched lava samples from the Canary and Cape Verde Islands, that we can independently show were entrapped prior to extensive sulphurdegassing. We find high ferric iron to total iron ratios (Fe3+/ Fe) of up to 0.27–0.30, indicating that mantle plume primary melts are significantly more oxidised than those associated with mid-ocean ridges and even subduction zone. These results, together with previous investigations from the Erebus, Hawaiian and Icelandic hotspots, confirm that mantle upwelling provides a return flow from the deep Earth for components of oxidised subducted lithosphere and suggest that highly oxidised material accumulates or is generated in the lower mantle. The oxidation state of the Earth’s interior must therefore be highly heterogeneous and potentially locally inversely stratified.
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