1000 resultados para datação U-Pb
Resumo:
The SW region of Amazonian craton presents policyclic evolution between 1.80-1.00 Ga and is comprised of the Rio Negro-Juruena, Rondoniana and Sunsas Provinces. The evolution of this region has being characterized by four orogens: Alto Jauru (1.79-1.74 Ga), Cachoeirinha (1.58-1.52 Ga), Suíte Santa Helena (1.45-1.42 Ga) e Sunsas/Aguapeí (1.0-0.9 Ga). The Alto Jauru orogen consists of TTG gneissic associations, greenstone sequences and intrusive granitoids origined in volcanic arc setting. Eight 40Ar/39Ar step-heating analyses were carried out in minerals (biotiteand hornblende) to investigate the thermal history and crustal evolution of this region. From the Alto Jauru orogen was sampled the gneiss banded and two biotite grains provide large dispersion of apparent ages, suggesting heterogenity in reservoir of the argon. Apparent age diagram yielded integrated ages of 1472 ± 6 Ma, interpreted as minimum ages of regional cooling episode. Three analyses of hornblende present ages varing from 1310 to 1400 Ma, possibly because smaller grain size become more susceptible to argon loss. 40Ar/39Ar step-heating methodology applied on biotite of pyroclastic tuff (U-Pb age about 1758 ± 7 Ma) presented integrated age of 1507 ± 7 Ma. The results found for this terrane demonstrated a geochronological correlation with metamorphic process linked Cachoeirinha orogen. Biotite and hornblende grains separates from granite and a tonalite origined during Cachoeirinha orogen were analyzed and the apparent age diagrams indicated well-defined plateau ages of 1520-1540 Ma. Biotite grains from a granitic sample were analized, and integrated ages about 1526 ± 2 Ma were obtained due argon loss in the initial steps. Thermochronologic history of SW region Amazonian craton is coherent with regional policyclic events and 40Ar/39Ar ages here presented probably correspond to regional cooling period of Cachoeirinha orogen.
Resumo:
The Serra do Caramuru and Tapuio stocks, located in the extreme NE of Rio Piranhas-Seridó Domain (RN), are representative of the Ediacaran-Cambrian magmatism, an important magmatic feature of the Brasilian / Panafrican orogeny of the Borborema Province. These bodies are lithologically similar, intrusive in paleoproterozoic gneiss embasement, being separated by a thin belt of mylonitic orthogneiss. The field relations show a magmatic stratigraphy initiated by dioritic facies that coexists with the porphyritic granitic and equigranular granitic I facies, and less frequently with equigranular granitic II facies. These rocks are crosscut by late granitic dykes and sheets with NE-SW / NNE-SSW orientation. The dioritic facies (diorite, quartz diorite, quartz monzodiorites, tonalite and granodiorite) is leucocratic to melanocratic, rich in biotite and hornblende. The granitic facies are hololeucocratic to leucocratic, and have biotite ± hornblende. Petrographic and geochemical (whole rock) data, especially from Serra do Caramuru pluton, suggest fractionation of zircon, apatite, clinopyroxene (in diorites), opaque minerals, titanite, biotite, hornblende, allanite, plagioclase, microcline and garnet (in dykes). The behavior of trace elements such as Zr, La and Yb indicates that the dioritic magma does not constitute the parental magma for the granitic facies. On the other hand, the granitic facies seems to be cogenetic to each other, displaying differentiation trends and very similar rare earth elements (REE) spectra [12.3≤(La/Yb)N≤190.8; Eu/Eu*=0.30-0.68]. Field relationships and REE patterns [6.96≤(La/Yb)N≤277.8; Eu/Eu*=0.18-0.58] demonstrate that the granitic dykes and sheets are not cogenetically related to the Serra do Caramuru magmatism. The dioritic facies is metaluminous (A/CNK = 0.88-0.74) and shoshonitic, whereas the granitic ones are metaluminous to peraluminous (A/CNK = 1.08-0.93) and high potassium calc-alkaline. Dykes and sheets are strictly peraluminous (A/CNK = 1.01-1.04). Binary diagrams relating compatible and incompatible trace elements and microtextures indicate the fractional crystallization as the dominant mechanism of magmatic evolution of the various facies. The Serra do Caramuru and Tapuio stocks have well preserved magmatic fabric, do not show metamorphic minerals and are structurally isotropic, showing crosscutting contact with the ductile fabric of the basement. These observations lead to interpretate a stage of relative tectonic stability, consistent with the orogenic relaxation period of the Brasiliano / Pan-African orogeny. Chemical plots involving oxides and trace elements indicate late to post-collisional emplacement. In this context, the assumed better mechanism to describe the stocks emplacement within an extensional T Riedel joint, with ENE-WSW extensional vector. The U-Pb zircon age of 553 ± 10 Ma allows correlating the Serra do Caramuru magmatism to the group of post-collisional bodies, equigranular high potassium calc-alkaline granites of the NE of Rio Piranhas-Seridó Domain.
Resumo:
The Serra do Caramuru and Tapuio stocks, located in the extreme NE of Rio Piranhas-Seridó Domain (RN), are representative of the Ediacaran-Cambrian magmatism, an important magmatic feature of the Brasilian / Panafrican orogeny of the Borborema Province. These bodies are lithologically similar, intrusive in paleoproterozoic gneiss embasement, being separated by a thin belt of mylonitic orthogneiss. The field relations show a magmatic stratigraphy initiated by dioritic facies that coexists with the porphyritic granitic and equigranular granitic I facies, and less frequently with equigranular granitic II facies. These rocks are crosscut by late granitic dykes and sheets with NE-SW / NNE-SSW orientation. The dioritic facies (diorite, quartz diorite, quartz monzodiorites, tonalite and granodiorite) is leucocratic to melanocratic, rich in biotite and hornblende. The granitic facies are hololeucocratic to leucocratic, and have biotite ± hornblende. Petrographic and geochemical (whole rock) data, especially from Serra do Caramuru pluton, suggest fractionation of zircon, apatite, clinopyroxene (in diorites), opaque minerals, titanite, biotite, hornblende, allanite, plagioclase, microcline and garnet (in dykes). The behavior of trace elements such as Zr, La and Yb indicates that the dioritic magma does not constitute the parental magma for the granitic facies. On the other hand, the granitic facies seems to be cogenetic to each other, displaying differentiation trends and very similar rare earth elements (REE) spectra [12.3≤(La/Yb)N≤190.8; Eu/Eu*=0.30-0.68]. Field relationships and REE patterns [6.96≤(La/Yb)N≤277.8; Eu/Eu*=0.18-0.58] demonstrate that the granitic dykes and sheets are not cogenetically related to the Serra do Caramuru magmatism. The dioritic facies is metaluminous (A/CNK = 0.88-0.74) and shoshonitic, whereas the granitic ones are metaluminous to peraluminous (A/CNK = 1.08-0.93) and high potassium calc-alkaline. Dykes and sheets are strictly peraluminous (A/CNK = 1.01-1.04). Binary diagrams relating compatible and incompatible trace elements and microtextures indicate the fractional crystallization as the dominant mechanism of magmatic evolution of the various facies. The Serra do Caramuru and Tapuio stocks have well preserved magmatic fabric, do not show metamorphic minerals and are structurally isotropic, showing crosscutting contact with the ductile fabric of the basement. These observations lead to interpretate a stage of relative tectonic stability, consistent with the orogenic relaxation period of the Brasiliano / Pan-African orogeny. Chemical plots involving oxides and trace elements indicate late to post-collisional emplacement. In this context, the assumed better mechanism to describe the stocks emplacement within an extensional T Riedel joint, with ENE-WSW extensional vector. The U-Pb zircon age of 553 ± 10 Ma allows correlating the Serra do Caramuru magmatism to the group of post-collisional bodies, equigranular high potassium calc-alkaline granites of the NE of Rio Piranhas-Seridó Domain.
Resumo:
In this report, I present trace element data for basement samples at Ocean Drilling Program (ODP) Site 1256. The samples analyzed represent a subset of the group ("pool") samples from ODP Leg 206, and these trace element data are part of a more comprehensive data suite for the same samples, with analyses of stable and radiogenic isotopes (e.g., Sr, Li, and O) in progress or recently completed that will be presented elsewhere. The trace element analyses were performed in the GeoAnalytical Lab at Washington State University. The following elements were analyzed: La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb, Lu, Ba, Th, Nb, Y, Hf, Ta, U, Pb, Rb, Cs, Sr, Sc, and Zr. Trace element data indicate that the igneous basement at Site 1256 is geochemically normal mid-ocean-ridge basalt. A massive ponded flow sampled in both Holes 1256C and 1256D is distinguished by higher abundances of rare earth elements (REE) and most of the other trace elements analyzed. One interval of highly altered basalt has significantly higher concentrations of Cs, Rb, and Ba and lower concentrations of Sr, Pb, Zr, Hf, Sc, and most REE than the samples of background alteration or halos. No correlation is obvious between trace element abundance and macroscopic type of alteration within the background alteration or halos.
Resumo:
Oceanic flood basalts are poorly understood, short-term expressions of highly increased heat flux and mass flow within the convecting mantle. The uniqueness of the Caribbean Large Igneous Province (CLIP, 92-74 Ma) with respect to other Cretaceous oceanic plateaus is its extensive sub-aerial exposures, providing an excellent basis to investigate the temporal and compositional relationships within a starting plume head. We present major element, trace element and initial Sr-Nd-Pb isotope composition of 40 extrusive rocks from the Caribbean Plateau, including onland sections in Costa Rica, Colombia and Curaçao as well as DSDP Sites in the Central Caribbean. Even though the lavas were erupted over an area of ~3*10**6 km**2, the majority have strikingly uniform incompatible element patterns (La/Yb=0.96+/-0.16, n=64 out of 79 samples, 2sigma) and initial Nd-Pb isotopic compositions (e.g. 143Nd/144Ndin=0.51291+/-3, epsilon-Nd i=7.3+/-0.6, 206Pb/204Pbin=18.86+/-0.12, n=54 out of 66, 2sigma). Lavas with endmember compositions have only been sampled at the DSDP Sites, Gorgona Island (Colombia) and the 65-60 Ma accreted Quepos and Osa igneous complexes (Costa Rica) of the subsequent hotspot track. Despite the relatively uniform composition of most lavas, linear correlations exist between isotope ratios and between isotope and highly incompatible trace element ratios. The Sr-Nd-Pb isotope and trace element signatures of the chemically enriched lavas are compatible with derivation from recycled oceanic crust, while the depleted lavas are derived from a highly residual source. This source could represent either oceanic lithospheric mantle left after ocean crust formation or gabbros with interlayered ultramafic cumulates of the lower oceanic crust. High 3He/4He in olivines of enriched picrites at Quepos are ~12 times higher than the atmospheric ratio suggesting that the enriched component may have once resided in the lower mantle. Evaluation of the Sm-Nd and U-Pb isotope systematics on isochron diagrams suggests that the age of separation of enriched and depleted components from the depleted MORB source mantle could have been <=500 Ma before CLIP formation and interpreted to reflect the recycling time of the CLIP source. Mantle plume heads may provide a mechanism for transporting large volumes of possibly young recycled oceanic lithosphere residing in the lower mantle back into the shallow MORB source mantle.
Resumo:
Analyses of Pb from mid-ocean ridge basalts obtained from DSDP Leg 37 lie on a line of near-zero-age slope. The data seem consistent with an evolutionary model of three stages, the beginning of the second stage being at about 600 m.y. - the model age obtained for the least radiogenic Pb. The beginning of the third stage of evolution at the time of formation of the rocks apparently did not change the average Th/U ratio since measured values are consistent with the ratio deduced from Pb isotope ratios. Ratios of U/Pb are not consistent with Pb isotope ratios, however, thus ruling out a simple two-stage evolutionary model.
Resumo:
A Cadeia Varisca Europeia, formada no final do Paleozóico, estende-se desde a Europa de Leste até à Península Ibérica e inclui extensas áreas ocupadas por rochas graníticas, representando, por isso, uma das regiões do globo em que mais se têm investigado os processos de reciclagem e acreção crustal em contexto de colisão continental. O Maciço Ibérico constitui o segmento mais ocidental do orógeno varisco europeu e uma das áreas onde a actividade plutónica está mais bem expressa e mostra uma maior diversidade tipológica. No Maciço Ibérico, em particular na Zona Centro Ibérica (ZCI), a intrusão de rochas granitóides de idade varisca está preferencialmente associada com a terceira fase de deformação (D3). De acordo com as suas relações com este evento de deformação, os granitóides da ZCI foram subdivididos em dois grandes grupos: sin-D3 e tardi-pós-D3. Em termos petrográficos e geoquímicos, os maciços graníticos sin- e tardi-pós-D3 têm sido integrados em duas séries principais: (a) a série dos granitos de duas micas e dos leucogranitos fortemente peraluminosos e (b) a série dos monzogranitos e granodioritos, metaluminosos a fracamente peraluminosos, com biotite ± anfíbola. Os granitos da primeira série apresentam uma filiação de tipo S e resultam da anatexia de materiais supracrustais durante o clímax de metamorfismo regional, enquanto.os granitóides da segunda série exibem características transicionais I-S e têm sido interpretados, quer como produtos da hibridização de magmas félsicos crustais com magmas básicos de proveniência mantélica, quer como resultantes da anatexia de protólitos metaígneos da crosta inferior. O trabalho realizado no batólito das Beiras revela que o clímax de metamorfismo regional foi atingido neste sector durante um evento extensional (D2), que foi acompanhado por intensa migmatização. No ínício da D3, o volume de fundidos crustais já seria suficientemente grande (ca. 15-35%) para que pudesse ocorrer a sua separação do resíduo sólido. Assim, durante a tectónica transcorrente D3, dá-se a ascenção, diferenciação e consolidação de abundantes quantidades de magmas graníticos, fortemente peraluminosos e isotopicamente evoluídos (tipo-S), que vêm a originar enormes batólitos de leucogranitos de duas micas, com idades entre 317-312 Ma. No final da D3, com a progressiva substituição do manto litosférico pela astenosfera, mais quente, diminui a densidade da coluna litosférica e ocorre o levantamento isostático e exumação da crusta. A fusão por descompressão da astenosfera gera líquidos básicos que hibridizam com os fundidos félsicos crustais, em proporções variáveis, e produzem magmas metaluminosos a ligeiramente peraluminosos, de afinidade calco-alcalina. A ascenção destes magmas terá tido lugar nos últimos estádios da deformação transcorrente e a sua instalação no nível crustal final ocorre após a D3, dando origem aos inúmeros maciços compósitos de granitóides biotíticos híbridos tardi-pós-cinemáticos, presentes no batólito das Beiras. Os dados de campo mostram que estes granitóides são intrusivos nos plutões sin-D3, cortam as estruturas regionais e provocam metamorfismo de contacto nas sequências do Carbónico Superior. Com base nas idades U-Pb obtidas em zircões e monazites, é possível datar este importante período de plutonismo granítico com 306-294 Ma. A assinatura geoquímica e isotópica dos granitóides híbridos tardi-pós-D3 revela que, para além da mistura de componentes com proveniência distinta (manto empobrecido e crusta continental), a sua evolução foi, em grande parte, controlada por processos de cristalização fraccionada (modelo AFC).
Resumo:
O complexo batolítico das Beiras está localizado na Zona Centro Ibérica (ZCI), no centro norte de Portugal. É predominantemente composto por rochas granitóides instaladas em metassedimentos de idade Neoproterozóica - Câmbrica Inferior, Ordovícica e Carbonífera Superior, durante ou após a última fase de deformação dúctil varisca (D3). No seu conjunto, as rochas granitóides do Batólito das Beiras cobrem um amplo espectro de idades (sin-, tardi- e tardi-pós-D3) e tipologias (tipo S e transicionais I-S). Neste trabalho apresentam-se dados petrográficos, mineralógicos, geoquímicos e isotópicos para estas intrusões e discutem-se os principais processos envolvidos na sua génese.
Resumo:
VESPA was a successful 25 day research cruise on R/V l'Atalante that took place in May and June 2015. The main aim was to acquire new rock samples from extinct volcanoes on the Norfolk, Loyalty and Three Kings ridges, which connect New Caledonia and New Zealand. This was in order to test various hypotheses of Late Cretaceous-Miocene SW Pacific tectonic development relating to (i) nature and duration of magmatism on the ridges; (ii) timing of subduction initiation east of northern Zealandia; (iii) postulated subduction polarity changes. A total of 3400 km of 'sismique rapide' shallow reflection seismic data were acquired and processed onboard. The seismic lines provided a very useful structural-stratigraphic framework for the rock dredging. Combined with multibeam bathymetry data they allowed intelligent targeting of acoustic basement (lavas) and specific seismic reflectors (sedimentary strata) on rocky slopes and fault scarps. Different stratigraphic levels of the Loyalty and Three Kings Ridge volcanic piles were sampled by dredging at different water depths on the Cook Fracture Zone and Cagou Trough fault scarps. By the end of the cruise, 43 dredges had been attempted and 36 of them yielded igneous or sedimentary rocks potentially useful to the VESPA project. Onboard use of a portable X-ray fluorescence unit confirmed the presence of intraplate (but no arc) volcanoes on the Norfolk Ridge and presence of arc, intraplate and shoshonitic volcanoes on the Loyalty and Three Kings Ridges. A total of 770 kg of rock was retained for post-cruise analysis in New Caledonia, France and New Zealand. Future work will include micropaleontological dating of sedimentary rocks, U-Pb and Ar-Ar isotopic dating of igneous rocks, and whole rock geochemical and tracer isotope analyses. We are optimistic that many of the initial research hypotheses will be able to be tested.
Resumo:
Tese (doutorado)—Universidade de Brasília, Instituto de Geociências, Programa de Pós-Graduação em Geologia, 2016.
Resumo:
Dataciones geocronológicas U-Pb en circones detríticos, edades 40Ar/ 39Ar en mica blanca, análisis estructurales, texturales, la composición química de elementos mayores, traza y tierras raras (REE) así como la composición química mineral de las rocas metamáficas, metultramáficas y metasedimentarias, fueron determinadas con el fin de determinar las condiciones metamórficas, el ambiente tectónico y la procedencia del Esquisto Granjeno en el noreste de México (Nuevo León y Tamaulipas). En el país existen rocas metamórficas paleozoicas que están relacionados con los procesos que dieron lugar a la colisión entre Laurentia y Gondwana durante la formación Pangea. Vestigios de la configuración continental paleozoica de México se encuentran en el Esquisto Granjeno, que forma parte del basamento metamórfico de la Sierra Madre Oriental. Relaciones de campo y análisis petrográficos indican que el Esquisto Granjeno consiste de rocas metamórficas con protolitos sedimentarios (psamita, pelita, turbidita, conglomerado, lutita negra) e ígneos (toba, flujos de lava, lava meta-almohadillada y cuerpos ultramáficos). El geotermómetro de clorita, el geobarómetro de fengita y la edad 40Ar/ 39Ar calculada indican que el Esquisto Granjeno fue afectado por metamorfismo en facies de sub-esquistos verdes a facies de esquistos verdes-anfibolita, (165-410°C y 2.5-4 kbar ) durante el Carbonífero (330±30 Ma). Las rocas metamáficas del Esquisto Granjeno tienen una afinidad sub-alcalina a alcalina y se caracterizan por un bajo contenido de SiO2 (40-50 wt%), alto contenido de Al2O3 (19 wt%) y #MgO de 48-67. La abundancia de tierras raras (∑REE) varía de 51-167 ppm. Estas rocas presentan patrones de REE normalizados a condrita moderadamente fraccionados, con valores de LaN/YbN 0.74-8.88. La anomalía de europio es variable (Eu/Eu* 0.80- 1.09) y presenta una tendencia ligeramente negativa (Eu/Eu* 0.96). Las rocas metamáficas tienen composiciones correspondientes a basaltos de cresta (MORB) e isla oceánica (OIB), de acuerdo a los valores en las relaciones Zr/Y=6-8 y Zr/Nb=4-9 para OIB y 0.9-3; 14-53 para MORB. Los protolitos de la serpentinita y el metacumulato corresponden a dunita y harzburgita. La serpentina y el metacumulato tienen un contenido de MgO (16-39 wt%), SiO2 (36-45 wt%), FeO (2-11 wt%), Al2O3 (0.76-13 wt%), CaO (< 22wt%) y #MgO (85-98, 69). Las rocas de talco presentan contenido de MgO (26-33wt%), SiO2 (31- 61wt%), FeO (3.7-9.8wt%), Al2O3 (1.2-19wt%), CaO (0.25-2.0wt%), y #Mg (83-93). Los patrones de tierras raras casi horizontals (LaN/YbN=0.51-19.95 y la relación LaN/SmN=0.72-9.08 sugieren un origen vinculado a un ambiente de dorsal oceánica y de suprasubducción para las rocas ultramáficas. Las serpentinitas contienen cromita rica en Al, ferrit-cromita y magnetita. La cromita rica en Al tiene #Cr 0.48-0.55 que indica que este mineral fue formado a partir de una fuente tipo MORB y que fue afectada hasta un 18% fusión parcial durante su formación. La ferritchromita tiene #Cr 0.93-1.00 que indica un origen metamórfico. La composición química de roca total indica que los protolitos de las rocas metasedimentarias consisten de lutita, grauvaca y arenita. La metapelita y metapsamita tienen un contenido de SiO2 (69-78% y 80-96% ) y de Al2O3 (9-13% y 1-8%). La abundancia de ∑REE son variables en los metasedimentos (9-178 ppm). Presentan patrones de REE normalizados a condrita con una tendencia más fraccionada que los de las rocas metamáficas, con valores en las relaciones LaN/YbN de 3-16. Las rocas metasedimentarias tienen anomalías de europio negativa (Eu/Eu* 0.67). Los datos obtenidos sugieren que los protolitos de las rocas metasedimentarias derivan de fuentes mixtas con una composición ígnea félsica-básica. (Ti/Nb 200-400). Según los valores de las relaciones de los elementos traza Th/Sc y Zr/Sc de 0.2-3.6 y 0.2-220, respectivamente se sugiere un ambiente de depósito para los protolitos de margen continental activo.
Resumo:
Dissertação (mestrado)—Universidade de Brasília, Instituto de Geociências, Pós-Graduação em Geologia, 2016.
Resumo:
Detrital zircons from Holocene beach sand and igneous zircons from the Cretaceous syenite forming Cape Sines (Western Iberian margin) were dated
using laser ablation – inductively coupled plasma – mass spectrometry. The
U–Pb ages obtained were used for comparison with previous radiometric
data from Carboniferous greywacke, Pliocene–Pleistocene sand and Cretaceous syenite forming the sea cliff at Cape Sines and the contiguous coast.
New U–Pb dating of igneous morphologically simple and complex zircons
from the syenite of the Sines pluton suggests that the history of zircon crystallization was more extensive (ca 87 to 74 Ma), in contrast to the findings of
previous geochronology studies (ca 76 to 74 Ma). The U–Pb ages obtained in
Holocene sand revealed a wide interval, ranging from the Cretaceous to the
Archean, with predominance of Cretaceous (37%), Palaeozoic (35%) and
Neoproterozoic (19%) detrital-zircon ages. The paucity of round to subrounded grains seems to indicate a short transportation history for most of
the Cretaceous zircons (ca 95 to 73 Ma) which are more abundant in the
beach sand that was sampled south of Cape Sines. Comparative analysis
using the Kolmogorov–Smirnov statistical method, analysing sub-populations separately, suggests that the zircon populations of the Carboniferous
and Cretaceous rocks forming the sea cliff were reproduced faithfully in
Quaternary sand, indicating sediment recycling. The similarity of the pre-
Cretaceous ages (>ca 280 Ma) of detrital zircons found in Holocene sand, as
compared with Carboniferous greywacke and Pliocene–Pleistocene sand, provides support for the hypothesis that detritus was reworked into the beach
from older sedimentary rocks exposed along the sea cliff. The largest percentage of Cretaceous zircons (
Resumo:
The late Paleozoic collision between Gondwana and Laurussia resulted in the polyphase deformation and magmatism that characterizes the Iberian Massif of the Variscan orogen. In the Central Iberian Zone, initial con- tinental thickening (D1; folding and thrusting) was followed by extensional orogenic collapse (D2) responsible for the exhumation of high-grade rocks coeval to the emplacement of granitoids. This study presents a tectonometamorphic analysis of the Trancoso-Pinhel region (Central Iberian Zone) to ex- plain the processes in place during the transition froman extension-dominated state (D2) to a compression-dom- inated one (D3).Wereveal the existence of low-dipping D2 extensional structures later affected by several pulses of subhorizontal shortening, each of them typified by upright folds and strike-slip shearing (D3, D4 and D5, as identified by superimposition of structures). The D2 Pinhel extensional shear zone separates a low-grade domain from an underlying high-grade domain, and it contributed to the thermal reequilibration of the orogen by facil- itating heat advection from lower parts of the crust, crustal thinning, decompression melting, and magma intru- sion. Progressive lessening of the gravitational disequilibrium carried out by this D2 shear zone led to a switch from subhorizontal extension to compression and the eventual cessation and capture of the Pinhel shear zone by strike-slip tectonics during renewed crustal shortening. High-grade domains of the Pinhel shear zone were folded together with low-grade domains to define the current upright folded structure of the Trancoso-Pinhel re- gion, the D3 Tamames-Marofa-Sátão synform. Newdating of syn-orogenic granitoids (SHRIMP U\\Pb zircon dat- ing) intruding the Pinhel shear zone, together with the already published ages of early extensional fabrics constrain the functioning of this shear zone to ca. 331–311 Ma, with maximum tectonomagmatic activity at ca. 321–317 Ma. The capture and apparent cessation of movement of the Pinhel shear zone occurred at ca. 317– 311 Ma.