TY - JOUR
T1 - Geochemical record of subduction initiation in the sub-arc mantle
T2 - insights from the Loma Caribe peridotite (Dominican Republic)
AU - Marchesi, Claudio
AU - Garrido, Carlos J.
AU - Proenza, Joaquin A.
AU - Hidas, Karoly
AU - Isabel Varas-Reus, Maria
AU - Butjosa, Lidia
AU - Lewis, John F.
PY - 2016/5
Y1 - 2016/5
N2 - The Loma Caribe peridotite body is mainly composed of serpentinized spinet harzburgites and lherzolites and minor orthopyroxene-bearing dunites and dunites. Modal proportions, mineral and whole-rock major and trace element compositions generally coincide with those of abyssal mantle rocks from mid-ocean ridges for the Iherzolites, and refractory supra-subduction peridotites for the harzburgites and dunites. The clinopyroxene-bearing harzburgites have intermediate compositions that overlap with those of residual mantle from both these settings. Major elements in the peridotites were mostly undisturbed by serpentinization and/or seafloor weathering whereas light rare earth elements (LREE) and large ion lithophile elements (LILE) were enriched by syn- and/or post-melting interaction with fluids/melts. Major element variations indicate that protoliths of the Loma Caribe peridotites mostly melted at 1-2 GPa and 1250 degrees C-1500 degrees C, as normal mid-ocean ridge and supra-subduction zone mantle. The MREE/HREE fractionations in both whole rocks and clinopyroxene can be explained by initial low (5%-6%) fractional melting of a garnet lherzolite source followed by variable (5%-20%) melting in the spinet stability field. The lherzolites and clinopyroxene-bearing harzburgites are residues of increasing melting triggered by increasing addition of slab fluids to a spinet peridotite source, while melting of the harzburgite protoliths was likely the result of focused flux of slab hydrous melts. The dunites and orthopyroxene-bearing dunites are products of pyroxene dissolution in residual peridotites caused by reaction with two different subduction-related melts, probably the parental magmas of Early Cretaceous low Ti island arc tholeiites (IAT) and boninites from Central Hispaniola, respectively. We conclude that the geochemical heterogeneity of the Loma Caribe peridotites records shifting conditions of melting during the development of subduction beneath the incipient Greater Antilles paleo-island arc in the Early Cretaceous. (c) 2016 Elsevier B.V. All rights reserved.
AB - The Loma Caribe peridotite body is mainly composed of serpentinized spinet harzburgites and lherzolites and minor orthopyroxene-bearing dunites and dunites. Modal proportions, mineral and whole-rock major and trace element compositions generally coincide with those of abyssal mantle rocks from mid-ocean ridges for the Iherzolites, and refractory supra-subduction peridotites for the harzburgites and dunites. The clinopyroxene-bearing harzburgites have intermediate compositions that overlap with those of residual mantle from both these settings. Major elements in the peridotites were mostly undisturbed by serpentinization and/or seafloor weathering whereas light rare earth elements (LREE) and large ion lithophile elements (LILE) were enriched by syn- and/or post-melting interaction with fluids/melts. Major element variations indicate that protoliths of the Loma Caribe peridotites mostly melted at 1-2 GPa and 1250 degrees C-1500 degrees C, as normal mid-ocean ridge and supra-subduction zone mantle. The MREE/HREE fractionations in both whole rocks and clinopyroxene can be explained by initial low (5%-6%) fractional melting of a garnet lherzolite source followed by variable (5%-20%) melting in the spinet stability field. The lherzolites and clinopyroxene-bearing harzburgites are residues of increasing melting triggered by increasing addition of slab fluids to a spinet peridotite source, while melting of the harzburgite protoliths was likely the result of focused flux of slab hydrous melts. The dunites and orthopyroxene-bearing dunites are products of pyroxene dissolution in residual peridotites caused by reaction with two different subduction-related melts, probably the parental magmas of Early Cretaceous low Ti island arc tholeiites (IAT) and boninites from Central Hispaniola, respectively. We conclude that the geochemical heterogeneity of the Loma Caribe peridotites records shifting conditions of melting during the development of subduction beneath the incipient Greater Antilles paleo-island arc in the Early Cretaceous. (c) 2016 Elsevier B.V. All rights reserved.
KW - Caribbean
KW - Hydrous melting
KW - Ophiolite
KW - Peridotite
KW - Subduction initiation
UR - http://www.scopus.com/inward/record.url?scp=84959334056&partnerID=8YFLogxK
U2 - 10.1016/j.lithos.2016.02.009
DO - 10.1016/j.lithos.2016.02.009
M3 - Article
VL - 252-253
SP - 1
EP - 15
JO - Lithos
JF - Lithos
SN - 0024-4937
ER -