Ja. Miller et al., An O-isotope profile through the HP-LT Corsican ophiolite, France and its implications for fluid flow during subduction, CHEM GEOL, 178(1-4), 2001, pp. 43-69
Subduction zones are important sites for fluid generation as the downgoing
slab undergoes progressive high-pressure metamorphism. These fluids are tho
ught to play an important role in the generation of arc-magmas, but their a
ffect on the subducted slab itself is less clear. In this study, the stable
isotope geochemistry of the Corsican ophiolite, which is variably affected
by subduction-related metamorphism, was investigated to assess the impact
of subduction zone fluid flow on the downgoing slab. A total of 170 stable
isotope analyses (oxygen and carbon) showed the following features: (1) ove
rall, the ophiolite preserves the same oxygen isotope profile with depth as
unmetamorphosed ophiolites; (2) the variation in oxygen isotope values for
different areas does not correlate with metamorphic grade; (3) oxygen and
carbon isotope values for calcite in the ophiolite are not in equilibrium w
ith the ophiolite but are similar to those of the overlying calc-schists (S
chistes Lustres); and (4) hydrogen isotopes indicate that serpentinitisatio
n of ultramafics occurred during sub-seafloor hydrothermal alteration and p
robably also during tectonic emplacement of the ophiolite. These features i
ndicate that large-scale fluid flow did not affect the Corsican ophiolite d
uring subduction zone metamorphism. Calcite in the ophiolite was probably p
recipitated from CO2-bearing fluids derived from decompression dehydration
reactions affecting the overlying Schistes Lustres during exhumation of the
ophiolite-bearing Schistes Lustres nappes. Given that ocean crust must und
ergo at least some dehydration during prograde subduction zone metamorphism
, the evolved fluids must be either highly channelled or exit the slab rela
tively quickly so as to not interact with it. The results of this study ind
icate that the important fluid pathways on Corsica have yet to be identifie
d, but are probably the shear zones and fault systems that bound different
slices of the high-pressure nappe stack. (C) 2001 Elsevier Science B.V. All
rights reserved.