Oceanic slab melting and mantle metasomatism - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles Science Progress Year : 2001

Oceanic slab melting and mantle metasomatism

Abstract

Modern plate tectonic brings down oceanic crust along subduction zones where it either dehydrates or melts. Those hydrous fluids or melts migrate into the overlying mantle wedge trigerring its melting which produces arc magmas and thus additional continental crust. Nowadays, melting seems to be restricted to cases of young (<50 Ma) subducted plates. Slab melts are silicic and strongly sodic (trondhjemitic). They are produced at low temperatures (<1000°C) and under water excess conditions. Their interaction with mantle peridotite produces hydrous metasomatic phases such as amphibole and phlogopite that can be more or less sodium rich. Upon interaction the slab melt becomes less silicic (dacitic to andesitic), and Mg, Ni and Cr richer. Virtually all exposed slab melts display geochemical evidence of ingestion of mantle material. Modern slab melts are thus unlike Archean Trondhjemite–Tonalite–Granodiorite rocks (TTG), which suggests that both types of magmas were generated via different petrogenetic pathways which may imply an Archean tectonic model of crust production different from that of the present-day, subduction-related, one.

Domains

Volcanology
Fichier principal
Vignette du fichier
Scaillet-ScienceProgress-2001.pdf (133.96 Ko) Télécharger le fichier
Loading...

Dates and versions

hal-00089820 , version 1 (24-08-2006)

Identifiers

  • HAL Id : hal-00089820 , version 1

Cite

Bruno Scaillet, Gaëlle Prouteau. Oceanic slab melting and mantle metasomatism. Science Progress, 2001, 84, pp.335-354. ⟨hal-00089820⟩
124 View
12614 Download

Share

Gmail Facebook Twitter LinkedIn More