HR: 0800h
AN: V31C-0625 [Abstracts]
TI: Stability of Titanian Clinohumite-olivine Intergrowths in HFSE-enriched Chlorite-harzburgite produced
by High-pressure Dehydration of Antigorite-serpentinite and its Potential Implications for the Origin
of Subduction Signatures
AU: SanchezVizcaino, V
EM: vlopez@ujaen.es
AF: Departamento de Geologia, Universidad de Jaen, E.U. Politecnica, Alfonso X El Sabio 28, Linares, 23700
Spain
AU: * Garrido, C J
EM: carlosg@ugr.es
AF: Dpto. Mineralogia y Petrologia, Universidad de Granada, Facultad de Ciencias, Fuentenueva sn, Granada,
18002
Spain
AU: Trommsdorff, V
V31C-0625
AF: Institut fur Mineralogie und Petrographie, ETH Zentrum, Sonneggstrasse 5, Zurich, CH-8092
Switzerland
AU: Gomez Pugnaire, M
V31C-0625
AF: Dpto. Mineralogia y Petrologia, Universidad de Granada, Facultad de Ciencias, Fuentenueva sn, Granada,
18002
Spain
AU: Connolly, J A
V31C-0625
AF: Institut fur Mineralogie und Petrographie, ETH Zentrum, Sonneggstrasse 5, Zurich, CH-8092
Switzerland
AB:
Depletion of high-field-strength trace elements (HFSE) relative to N-MORB is the most distinctive geochemical fingerprint of
subduction magmatism. Proposed hypotheses advocate that this subduction signature is acquired during melting and/or fluid
transfer either in the mantle wedge or in the crust of the subducting oceanic plate. Here we provide field-based and
geochemical evidence from the Cerro del Almirez ultramafic massif (Sierra Nevada, Betic Cordillera, S.Spain) showing that
high-pressure dehydration of antigorite-serpentinite produces chlorite-harzburgite relatively enriched in HFSE due to the
stabilization of F-OH-Ti-clinohumite intergrowths with prograde olivine. F-OH-Ti-clinohumite occurs as porphyroblastic grains
and within prograde olivine as irregular and lamellar, planar intergrowths at microscopic and submicroscopic scales.
Chlorite-harzburgite is characterized by a brown pleochroic olivine with abundant oriented microscopic to submicroscopic
oxide particles. The mean Ti content of bulk brown olivine is 144 ppm. Brown olivine preserves Ti-clinohumite lamellae that
sometimes grade into ghost lamellae outlined by oxide trails. This observation suggests that some of the oxide inclusions in
brown olivine are derived from the breakdown of Ti-clinohumite intergrowths.
Thermodynamic modelling for selected Almirez bulk rock compositions indicates 695 oC and 1.7 to 2.0 GPa, as the
PT stability conditions for the Almirez Ti-clinohumite -olivine intergrowths. The computed phase diagrams, in conjunction
with geothermal conditions envisaged for different subduction settings, indicate that Ti-clinohumite is stable in the
vicinity of the antigorite-serpentinite/chlorite-harzburgite phase boundary at subarc depths. In these settings,
deserpentinization may act as a source of fluids leaching LILE, Pb, and Sr from the overlying crust and sediments on their
way up to the mantle wedge. Stabilization of chlorite-harzburgites with clinohumite-olivine intergrowths in the mantle wedge
may acts as a sink of HFSE by selectively fractionating them from other incompatible trace elements in fluids emanating from
the slab. Resulting arc fluids in equilibrium with wedge chlorite-harzburgite are strongly depleted in HFSE and transfer this
depletion to the overlying hot mantle wedge, where subduction magmas are generated.
DE: 3630 Experimental mineralogy and petrology
DE: 3640 Igneous petrology
DE: 3660 Metamorphic petrology
SC: Volcanology, Geochemistry, Petrology [V]
MN: Fall Meeting 2005