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Please use this identifier to cite or link to this item:
http://hdl.handle.net/10174/40889
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| Title: | ND-SR ISOTOPE AND TRACE ELEMENT EVIDENCE FOR CONTRASTING MANTLE SOURCES IN THE BIMODAL GABBROIC AND SYENITIC COMPLEXES OF NE ALENTEJO, PORTUGAL (OSSA-MORENA ZONE) |
| Authors: | Pin, Christian Carrilho Lopes, José |
| Editors: | Errandonea Martin, Jon García de Madinabeitia, Sonia Sánchez Lorda, Maria Eugenia Sarrionandia, Fernando |
| Keywords: | gabbro syenite mantle-derived inherited SupraSubductionZone signature |
| Issue Date: | 4-Jul-2015 |
| Citation: | Pin, C. & Carrilho Lopes, J. (2025). Nd-Sr isotope and trace element evidence for contrasting mantle sources in the bimodal gabbroic and syenitic complexes of NE Alentejo, Portugal (Ossa-Morena Zone). In: Errandonea-Martin, J., García de Madinabeitia, S., Sánchez-Lorda, M.E. & Sarrionandia, F. (Eds.), Advances in Geochronology and Geochemistry: A tribute to José Ignacio Gil Ibarguchi, 45. https://doi.org/10.5281/zenodo.15796027 |
| Abstract: | The NE Alentejo features several pre-Variscan plutonic complexes of diverse
geochemical affinity: Alter do Chão/Alter Pedroso (AC/AP) (per)alkaline bimodal
associations of Early Ordovician age, and Elvas-Campo Maior (ECM) gabbros and
gabbro-diorites, of calc-alkaline affinity, and still uncertain emplacement age. The data
obtained for 22 mafic and salic samples highlight a great geochemical diversity. Salic
rocks, ranging from under-saturated syenite to granite, originated from mantle-derived
parental magmas. Minor amounts of crustal contamination are reflected by decreasing
Ndi values from +4.0 to +2.5 with increasing degree of silica saturation in AC/AP, but a
highly alkaline sample from Arronches with Ndi +5.0, suggests that some salic melts
may have been directly produced by very low degree of partial melting of a mantle
source. No typical crustal signatures were found among the felsic rocks, suggesting
that pervasive lower crustal melting did not occur. Gabbroic cumulates from AC and
two gabbroic samples from CM fractionated from basaltic or basanitic magmas. Their
very low Th/Nb ratio and radiogenic isotope signatures (Ndi ca. +5; 87Sr/86Sri ca. 0.704)
exclude any significant contamination during ascent through the continental crust. Their
parent magmas were extracted from a mantle reservoir that was characterized by
secular depletion of LREE, and was enriched in Nb and LREE, but not Th, at some
time predating the ~500 Ma magmatism. This perhaps occurred in the Late
Proterozoic, as might be inferred from TDM Nd model ages in the 0.7-0.8 Ga range.
Gabbroic to dioritic rocks from ECM have variable degrees of enrichment in Th and
LREE, marked depletion in Nb, and Ndi = -1 to -5, pointing to a strong imprint of
materials from the upper continental crust. However, given the basic major element
composition of these rocks, and the lack of evidence for abundant crustal melting, it is
inferred that their parent magmas owe their signature to a mantle source that
underwent a style of enrichment style very different from that observed in the AC
gabbros. Indeed, while the AC source was enriched in Nb and LREE without major
change of its depleted mantle isotope signature, the ECM mantle source was
penetrated, at some earlier epoch, by silicic melts rich in Th and LREE, but relatively
poor in Nb, that had a drastic effect on the incompatible trace element budget of the
peridotite country-rock. This might have occurred in supra-subduction zone (SSZ)
settings of Late Proterozoic age, through hydrous partial melting of the uppermost
oceanic crust and clastic sediments from tha ca. 2 Ga West African craton. Such
inherited SSZ signatures are well known in other within-plate basaltic provinces
generated during continental break-up episodes such as, for example, the Jurassic
Karoo-Ferrar igneous province.
All plutons may have emplaced during a single, broad igneous event associated with
the Cambro-Ordovician rifting episode well documented in the Ossa-Morena Zone, but
precise U-Pb dating is needed to establish the igneous sequence on a firm basis, and
verify whether the ECM plutons do not reflect a much younger, entirely separate event. |
| URI: | https://doi.org/10.5281/zenodo.15796027 http://hdl.handle.net/10174/40889 |
| Type: | bookPart |
| Appears in Collections: | GEO - Publicações - Capítulos de Livros
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