This thesis is a study of some of the processes which operate at mid crustal levels (10- 20km) during the emplacement of granitoid magmas, with particular reference to the process of in-situ expansion and the association between magma emplacement and orogen evolution. A number of plutons were studied to assess this the Ardara pluton from Donegal, NW Ireland, together with the Atibaia, Morro Azul, Imbiricu and Itapeti plutons from the Rio Paraiba do Sul shear belt (RPSSB), Sao Paulo state, SE Brazil. The emplacement of the Ardara pluton has been the subject of studies by many authors since the 1950's. It has been interpreted as a diapir ascending along a thrust, a granite balloon which forcefully created more than 60% of its space and, most recently, as a set of nested diapirs which forcefully created only 30% of their own space. Field mapping together with the determination of finite strain within the pluton, shortening estimates, shear sense determinations, petrographic deformation fabrics and computer modelling indicates that: i) the pluton displays a concentrically increasing finite strain and it expanded in-situ from a central 'injection point', having possibly ascended along a shear zone-related conduit; ii) the country rocks partitioned intense strains into the 500m closest to the pluton, a deformation feature which is shown to be consistent with a power-law wallrock theology; Hi) earlier granite pulses and the country rock were 'shouldered aside' to the east and west, expansion of the pluton, which was preferentially in a northwards direction; iv) that the intrusion related shortening preserved within the wallrocks was approximately equivalent to the strain preserved within pluton and the space requirements for the pluton are essentially met by preserved forceful emplacement-related strains; and v) if the pluton magma is considered as having ascended through dyke-like conduits emplacement could occur in a minimum of ~4000yrs, whereas magma ascent as a Hot Stokes diapir would require hundreds of thousands to millions of years for complete emplacement. Finally, the Ardara pluton does not conform to any of the established criteria for diapir-like ascent of a magma body and the data demonstrate it to be a testable example of a pluton which expanded entirely in-situ. The Rio Paraiba do Sul shear belt (RPSSB) is a dextral transpressional segment of the Late Precambrian Brasiliano-Pan African orogenic belt. The studied plutons were emplaced in the latter stages of this orogen in close spatial association with one of the many northeast-southwest trending, sub-vertical, continental-scale shear zones. All the granites show a similar emplacement and deformation history despite their different petrographic features and isotopic ages. This history consists of an early shallowly dipping, low angle fabric, in the country rocks, associated with crustal thickening, the later development of dominantly dextral sub-vertical shear zones, followed by the emplacement of the studied plutons and finally overprinting by a pervasive dextral plane strain and late-stage discrete mylonitic shears. Field examination demonstrates that: i) each of the plutons preserves an internally homogeneous emplacement-related finite strain, weak magmatic fabric, magma sheets and weakly deformed wallrocks; ii) magmatic shear sense determinations and wallrock deformation fabrics indicate that, during emplacement, the RPSSB was extending (at least at the emplacement level) in an east-west direction creating sinistral dilatational pull-aparts along the major shear zones, into which granitic magma was preferentially emplaced; and Hi) within this generally extensional context there was a component of long axis perpendicular in-situ forceful expansion, this created no more than 20% of the width of any one granite. Applying a simple pull-apart extension model suggests that pluton emplacement was associated with approximately 40% regional extension sub-parallel to the former orogenic convergence direction. This emplacement, as a result of sheeting through dyke-like conduits, requires thousands of years, rather than the millions of years required for ascent and emplacement of a Hot Stokes diapir. Interpreting these results suggests that the intruded granitoids are associated with a mid-crustal component of orogen perpendicular extension I collapse during the latter stages of the Brasiliano orogeny. Such extension I collapse could have been initiated by: a cessation in continental convergence or; by the delamination of a thickened thermal boundary layer, a process which has been suggested to be the driving force behind orogenic collapse in younger orogenic belts. These examples demonstrate that: i) 'forceful' balloon-like emplacement of granitic magma can occur; ii) there are very close inter-relationships between granite emplacement and orogenic dynamics; and Hi) that 'space' for granitoid magma can be created by a combination of forceful and dilatational and fault-related mechanisms.

<p> The thesis pluton is part of the Saanich granodiorite batholithic complex on south-east Vancouver Island. The pluton is 11 Km by 2 Km, elliptical and trends NW-SE. </p> <p> Petrographically its mineral composition is that of a granodiorite. Alteration is fairly intense as shown by plagioclase and potassium feldspar altering to sericite, as well as biotite and hornblende altering to chlorite. Deformation textures were observed in the form of strained quartz and bent cleavage in biotite. </p> <p> From chemical analyses it was found that the granodiorite represents part of a fractionation process along a calc-alkaline trend. The magma was derived from partial melting of the lower crust. </p> / Thesis / Bachelor of Science (BSc)

No description available.

Estudios en cuanto a petrología, microestructuras y de campo, fueron realizados en el plutón Sorata de edad Triásico Superior-Jurásico Inferior del segmento norte de la Cordillera Real, para caracterizar la evolución magmática y algunas implicancias tectónicas durante el adelgazamiento litosférico ocurrido en el intervalo Pérmico Superior- Jurásico Medio. La intrusión expone una zonación composicional definida por tres asociaciones de facies: granodioritas y tonalitas con biotita ± hornblenda ± piroxeno (Facie I); adamelitas con biotita (Facie II); y granitoides con muscovita ± biotita (Facie III). Los estudios geoquímicos detallados de este plutón revelan que los granitoides están agrupados en tres asociaciones geoquímicas, con clasificaciones genéticas diferentes: granitoides de las facies I y II, de tipo I; granitoides de la facie III, de tipo S; y xenolitos (cuarzodioritas, cuarzomonzonitas y monzonitas) de tipo A. Por lo que los granitoides del plutón Sorata no pueden ser clasificados como exclusivamente de tipo I, S o A; sin embargo, la agrupación en asociaciones de facies, permite clasificarlas en tipo I y tipo S, compartiendo algunas características tipo A. Basado en estos datos, los fundidos parentales de composición intermedia y tipo A (xenolitos) derivan de la fusión del manto litosférico durante el adelgazamiento litosférico del Triásico - Jurásico Medio. Estos magmas, posteriormente ascienden y contribuyen con la fusión parcial de las rocas metaígneas de la corteza inferior, sin evidencias de mezcla de magmas, generando magmas tipo I, que fueron luego emplazados y contaminados en la corteza superior (granitoides de las facies I y II). Este emplazamiento contribuyó a la fusión parcial de la corteza superior, produciendo magmas tipo S (granitoides de la facie III). Por lo tanto, el plutón Sorata es el resultado de tres episodios o pulsos magmáticos desarrollados de manera sucesiva durante el evento distensivo del Triásico – Jurásico Medio (McBride et al., 1983; Sempere et al., 1995 y 2005). Los estudios petrográficos a nivel microestructural, llevados a cabo en granitoides foliados de la facie I del flanco oriental del intrusivo, demuestran el origen primario de la foliación, la cuál es resultado de un evento de deformación dúctil (?) asociado a zonas de cizalla que probablemente afectaron el flanco oriental del intrusivo en una etapa previa a la cristalización completa del magma. Por último, la esquistosidad regional S1 existente en rocas ordovícicas del área de estudio, es resultado de un evento deformacional desarrollado con anterioridad a la intrusión del granitoide Sorata, a la que se superpuso posteriormente, una deformación S2 tardía, la cual es claramente evidente en el sector sur del área de estudio

The Egrigoz, Koyunoba, and Alacam plutons are located in the Northern Menderes Massif of western Turkey between the Simav normal fault to the south and the Izmir-Ankara-Erzincan suture to the north. Although much attention has focused on their geochemical and geochronological history, their relationship to each other and other major structures in the region is still debated. Some geologic maps show the Egrigoz and Koyunoba pluton bounded to the west by the low-angle Simav detachment fault. In contrast, other regional maps show no offsets between the plutons and surrounding metamorphic rocks. Yet other studies indicate thrust faults may be present near the Egrigoz pluton, between Menderes metamorphic rocks and a meta-rhyolite unit. To gain a better understanding of the history of the Egrigoz, Koyunoba, and Alacam plutons, ArcGIS digital elevation data from the region, geochronological data, geochemical analyses, and cathodoluminescence (CL) images were acquired to search for effects of micro- to macro-scales of deformation. Numerous ~E-W trending extension lineations that parallel the Simav graben and cut the plutons were observed in relief images. These lineations, likely due to large-scale ~N-S extension, continue across plutons inferring that extension continued after the exhumation of these rocks. The Simav graben and its associated high-angle fault are evident in the elevation data, but no other significant detachment-related basins or structures are shown, including the low-angle Simav detachment. U-Pb zircon ages, ranging from 29.9±3.9 Ma to 14.6±2.6 Ma, suggest the plutons crystallized over a ~15 m.y. time frame. Samples from the plutons are peraluminous S-type granite to granodiorites. The plutons were emplaced in a post-collisional volcanic-arc setting and range from magnesian to ferroan with increasing silica contents. Geochemical analyses show little difference between the three plutons, consistent with the rocks arising from a similar source. To document microstructures that might help explain these heterogeneities, CL images were obtained. CL images document a complicated tectonic history including magma mixing, multiple episodes of brittle deformation, and fluid alteration. The CL images constitute evidence of a complex multi-stage tectonic history for the region that includes water-mediated brittle deformation. / text

The Seiland Igneous Province, of which 5400 km2 is exposed, is hosted within a discrete terrane within the northernmost part of the Caledonian orogenic belt. The Province consists of numerous mafic and ultramafic plutons emplaced into a sedimentary succession indicative of a continental setting. Accompanying this mafic magmatism is a significant volume of intermediate monzonitic and dioritic rock (10% of the total exposed igneous rock), as well as numerous nepheline syenite and carbonatitic intrusions. This study reports ID-TIMS U-Pb analyses on magmatic zircons from a range of intrusions, which indicate that the bulk of the Seiland magmatism took place between 560 Ma and 570 Ma, whereas previous studies had produced a range of ages between 420 Ma and 830 Ma. The data indicate that only one magmatic episode is represented in the rocks of the Seiland Igneous Province, invalidating previous models involving multiple rifting events over a period of 300 m.y. Detailed geochemical investigation of several plutons from an evolved high alkali suite of gabbroic intrusions in the Seiland Igneous Province has shown that these plutons are generally enriched in trace elements compared to layered intrusions from other areas across the globe, but that geochemically the gabbros are relatively homogenous. The rocks yield εHf and εNd values for the gabbroic rocks ranging from +8 to -6 and from +4 to -4, respectively, indicative of the contamination of mantlederived material with crustal material. The most primitive isotopic values are similar to those obtained from the carbonatites and nepheline syenites, indicating the same mantle source gave rise to the magmas that were subsequently emplaced as the Seiland Igneous Province. The homogeneous trace element content of the different mafic rocks most likely indicates a relatively homogeneous mantle source for the original magmas of the province, which has subsequently been affected by processes of assimilation and crustal contamination. The monzonitic and dioritic bodies in the Seiland Igneous Province are not derived from melted silicic crustal material and may have been formed by the melting of pre-existing mafic material. The new geochronology invalidates the metamorphic framework previously proposed for the Seiland Igneous Province, which postulated several orogenic events between the emplacement of the magmas and the Caledonian Orogeny. There is no evidence for metamorphic activity in the period between 570 Ma and 420 Ma, and there are monazites in gneissic rocks hosted within mafic rocks of Seiland age that preserve an age of 640 Ma. This leads to the conclusion that only one metamorphic event, the 420 Ma Caledonian Orogeny caused by the collision of Baltica and Laurentia, affected the Seiland terrane after the emplacement of the Seiland magmas. The new data obtained lead to a model for the evolution of the Seiland Province in which a number of heavily modified and contaminated mantle-derived mafic magmas derived from the mantle were emplaced into the continental crust of the Seiland nappe between 560 and 570 Ma. This magmatism was accompanied by the injection of alkaline magmas into the same area of the crust, and the melting of mafic rock emplaced earlier. This magmatic event is considered to have occurred in an extensional stress regime, possibly during intracontinental rifting or back-arc spreading. This event took place well before the 420 Ma Caledonian Orogeny, and thus the Seiland Igneous Province can be considered a remnant of an older geological terrane that was emplaced onto the margin of Baltica during the Caledonian Orogeny.

Os Plutons Palermo (ca. 250 km2) e Rio Negro (ca. 130 km2) afloram na região Alto Rio Negro (PR) e fazem parte da Província Graciosa, uma província Neoproterozóica (ca. 580 Ma) constituída por granitos e sienitos na região S-SE do Brasil. Em ambos os plutons afloram variedades de rochas graníticas, predominantes, e gabro-dioríticas, bem como rochas híbridas, principalmente granodioritos. Estes plutons apresentam zonamento em geral bem marcado, que é tipicamente inverso caso do Pluton Rio Negro. As rochas graníticas principais correspondem a sieno- e monzogranitos predominantes e álcali-feldspato granitos e quartzo monzonitos subordinados de natureza metaluminosa a levemente peraluminosa. São rochas com estruturas maciças e texturas variadas que apresentam como associação mineral máfica típica hb + bi ± all + zr + ap ± ti + mt + ilm); as rochas gabro-dioríticas incluem gabro-dioritos e quartzo monzogabro-dioritos metaluminosos com estruturas maciças e granulações fina a média, caracterizadas pela associação cpx ± opx + hb + bt ± ti ± ap ± zr. A composição dos plagioclásios nestas rochas varia no intervalo de labradorita a andesina. As rochas híbridas são principalmente granodioritos que se caracterizam por uma variedade de estruturas e texturas indicativas de desequilíbrio, compatíveis com processos de coexistência e mistura parcial entre líquidos ácidos e básico-intermediários que formaram os granitos principais e os gabro-dioritos. Estas rochas são mais comuns no Pluton Rio Negro. A associação mineral máfica é similar, mas com abundâncias distintas de fases, à observada para os granitos principais. Nas rochas graníticas os anfibólios são Fe-hornblenda e Fe-edenita, com valores 0,65 < fe# < 0,95, os valores mais elevados ocorrendo nos álcali-feldspato granitos, as biotitas apresentam 0,71 < fe# < 0,99, observando-se que o componente annítico é também maior nestas últimas rochas. No caso das rochas gabro-dioríticas, os valores fe# variam entre 0,48 e 0,59, 0,41 e 0,56, 0,47 e 0,53 e 0,54 a 0,57 para ortopiroxênio, clinopiroxênio, anfibólio e biotita, respectivamente. As composições médias de orto- e clinopiroxênio coexistentes são \'Wo IND.46\'\' En IND.30\'\' Fe IND.24\' e \'Wo IND.3\'\' En IND.42\'\'Fe IND.55\' e a sugerem uma possível afinidade toleítica, ou cálcio-alcalina, para magma original. Os padrões de elementos terras raras revelam fatores de enriquecimento entre 1-10, 50-70, 100-300 em relação à composição condrítica para ortopiroxênio, clinopiroxênio e anfibólio nas rochas estudadas, com fracionamento bem marcado dos elementos leves em relação aos pesados no ortopiroxênio, não observado no caso de clinopiroxênio e anfibólio. Todos os padrões são caracterizados por anomalia negativa bem marcada de Eu. As pressões de cristalização dos magmas foram estimadas entre 1-3,5 kbar, mas os valores acima de ca. 2 kbar possivelmente não tenham significado real, dadas as composições mais ferroanas dos anfibólios. Temperaturas de saturação de zircão e/ou apatita e de equilíbrio entre orto- e clinopiroxênio, anfibólio-plagioclásio indicam intervalos de cristalização entre ca. 1000 e 750° C para as rochas gabro-dioríticas e entre ca. 900 e 670° C para os granitos principais. As paragêneses minerais e os valores obtidos para o número fe# em biotita em equilíbrio com feldspato alcalino e magnetita apontam para condições de cristalização relativamente oxidantes para as rochas félsicas, exceto os álcali-feldspato granitos, e máfico-intermediárias, superiores ao tampão QFM. / The Palermo (ca. 250 km2) and Rio Negro (ca. 130 km2) Plutons crop out in the so called Alto Rio Negro region , Parana state, making part of the Graciosa Province, a NeoProterozoic province (ca. 580 Ma) constituted by granites and syenites in S-SE Brazil. The plutons are made predominant granitic rocks, gabbro-diorites, as well as hybrid rocks constituted mainly by granodiorites. Both plutons show compositional a zoning pattern, which is inversed in the case of the Rio Negro Pluton. The main granitid rocks are mainly metaluminous to slightly peraluminous syeno- and monzogranites with subordinate quartz monzonites and alkcali-feldspar granites. They show a massive structure and a variety of textures, with hb + bi ± all + zr + ap ± ti + mt + ilm as the typical mafic mineral association. Gabbro-dioritic rocks include fine- to medium-grained metaluminous gabro-diorites and quartz monzogabrros and diorites with massive strucure characterized by the mafic mineral associations with cpx ± opx + hb + bt ± ti ± ap ± zr. In these rocks, the plagioclase compositions vary between labradorite and andesine. Hybrid rocks are mainly granodiorites characterized by several strucures and textures indicative of desiquilibrium and mingling/partial mixing between the silicic and basic-intermediate melts that formed the mainn granites and the gabbro-diorites. Such rocks are more abundant in the Rio Negro Pluton. The mafic mineral association is similar, but in contrasted relative abundance, to the ones found in the main granites. In the main granites the amphiboles are Fe-horblende and Fe-edenite, with 0.65 < fe# < 0.95, the higher among these values appearing in the alkali-feldspar granites. Biotite present 0.70 < fe# < 0.99 and the annitic component are also higher in the later rocks. In the case of the gabbro-dioritic rocks, the fe# numbers range between 0.48 and 0.59, 0.41 and 0.56, 0.47 and 0.53 and 0.54 and 0.57 in ortopyroxene, clinopyroxene, amphibole and biotite, respectively. The averaged compositions of coexisting orto- and clinopyroxene are \'Wo IND.46\'\'En IND.30\'\'Fe IND.24\' and \'Wo IND.3\'\'En IND.42\'\'Fe IND.55\' and suggest a tholeiitic or calk-alkaline nature of the original melts. Rare earth element patterns reveal enrichment factors up to 1-10, 50-70, 100-300 relative to the chondritic composition in ortopyroxene, clinopyroxene and amphibole, respectively, with a well marked fractionation of the heavy over the light rare earths in the case of the ortopyroxene, a feature not observed in clinopyroxene and amphibole. All patterns show a notable Eu negative anomaly. Melts crystallization pressures were estimated to be between 1 and 3.5 kbar; however values higher than ca. 2 kbar seems to be unrealistic given the ferroan compositions of some amphiboles. Zircon and apatite saturation temperatures coupled with ortopyroxene-clinopyroxene and amphibole-plagioclase equilibrium temperatures suggest crystallization intervals between ca. 1000 - 750° C in the case of the gabbro-diorites and ca. 900 - 670° C in the case of the main granites. Mineral paragenesis and fe# values in biotite in equilibrium with alkali-feldspar and magnetite suggests relative oxidizing crystallization conditions for the acid and basic-intermediate melts, higher than the QFM buffer, the alkali-feldspat granites being a possible exeption.

Os Plutons Palermo (ca. 250 km2) e Rio Negro (ca. 130 km2) afloram na região Alto Rio Negro (PR) e fazem parte da Província Graciosa, uma província Neoproterozóica (ca. 580 Ma) constituída por granitos e sienitos na região S-SE do Brasil. Em ambos os plutons afloram variedades de rochas graníticas, predominantes, e gabro-dioríticas, bem como rochas híbridas, principalmente granodioritos. Estes plutons apresentam zonamento em geral bem marcado, que é tipicamente inverso caso do Pluton Rio Negro. As rochas graníticas principais correspondem a sieno- e monzogranitos predominantes e álcali-feldspato granitos e quartzo monzonitos subordinados de natureza metaluminosa a levemente peraluminosa. São rochas com estruturas maciças e texturas variadas que apresentam como associação mineral máfica típica hb + bi ± all + zr + ap ± ti + mt + ilm); as rochas gabro-dioríticas incluem gabro-dioritos e quartzo monzogabro-dioritos metaluminosos com estruturas maciças e granulações fina a média, caracterizadas pela associação cpx ± opx + hb + bt ± ti ± ap ± zr. A composição dos plagioclásios nestas rochas varia no intervalo de labradorita a andesina. As rochas híbridas são principalmente granodioritos que se caracterizam por uma variedade de estruturas e texturas indicativas de desequilíbrio, compatíveis com processos de coexistência e mistura parcial entre líquidos ácidos e básico-intermediários que formaram os granitos principais e os gabro-dioritos. Estas rochas são mais comuns no Pluton Rio Negro. A associação mineral máfica é similar, mas com abundâncias distintas de fases, à observada para os granitos principais. Nas rochas graníticas os anfibólios são Fe-hornblenda e Fe-edenita, com valores 0,65 < fe# < 0,95, os valores mais elevados ocorrendo nos álcali-feldspato granitos, as biotitas apresentam 0,71 < fe# < 0,99, observando-se que o componente annítico é também maior nestas últimas rochas. No caso das rochas gabro-dioríticas, os valores fe# variam entre 0,48 e 0,59, 0,41 e 0,56, 0,47 e 0,53 e 0,54 a 0,57 para ortopiroxênio, clinopiroxênio, anfibólio e biotita, respectivamente. As composições médias de orto- e clinopiroxênio coexistentes são \'Wo IND.46\'\' En IND.30\'\' Fe IND.24\' e \'Wo IND.3\'\' En IND.42\'\'Fe IND.55\' e a sugerem uma possível afinidade toleítica, ou cálcio-alcalina, para magma original. Os padrões de elementos terras raras revelam fatores de enriquecimento entre 1-10, 50-70, 100-300 em relação à composição condrítica para ortopiroxênio, clinopiroxênio e anfibólio nas rochas estudadas, com fracionamento bem marcado dos elementos leves em relação aos pesados no ortopiroxênio, não observado no caso de clinopiroxênio e anfibólio. Todos os padrões são caracterizados por anomalia negativa bem marcada de Eu. As pressões de cristalização dos magmas foram estimadas entre 1-3,5 kbar, mas os valores acima de ca. 2 kbar possivelmente não tenham significado real, dadas as composições mais ferroanas dos anfibólios. Temperaturas de saturação de zircão e/ou apatita e de equilíbrio entre orto- e clinopiroxênio, anfibólio-plagioclásio indicam intervalos de cristalização entre ca. 1000 e 750° C para as rochas gabro-dioríticas e entre ca. 900 e 670° C para os granitos principais. As paragêneses minerais e os valores obtidos para o número fe# em biotita em equilíbrio com feldspato alcalino e magnetita apontam para condições de cristalização relativamente oxidantes para as rochas félsicas, exceto os álcali-feldspato granitos, e máfico-intermediárias, superiores ao tampão QFM. / The Palermo (ca. 250 km2) and Rio Negro (ca. 130 km2) Plutons crop out in the so called Alto Rio Negro region , Parana state, making part of the Graciosa Province, a NeoProterozoic province (ca. 580 Ma) constituted by granites and syenites in S-SE Brazil. The plutons are made predominant granitic rocks, gabbro-diorites, as well as hybrid rocks constituted mainly by granodiorites. Both plutons show compositional a zoning pattern, which is inversed in the case of the Rio Negro Pluton. The main granitid rocks are mainly metaluminous to slightly peraluminous syeno- and monzogranites with subordinate quartz monzonites and alkcali-feldspar granites. They show a massive structure and a variety of textures, with hb + bi ± all + zr + ap ± ti + mt + ilm as the typical mafic mineral association. Gabbro-dioritic rocks include fine- to medium-grained metaluminous gabro-diorites and quartz monzogabrros and diorites with massive strucure characterized by the mafic mineral associations with cpx ± opx + hb + bt ± ti ± ap ± zr. In these rocks, the plagioclase compositions vary between labradorite and andesine. Hybrid rocks are mainly granodiorites characterized by several strucures and textures indicative of desiquilibrium and mingling/partial mixing between the silicic and basic-intermediate melts that formed the mainn granites and the gabbro-diorites. Such rocks are more abundant in the Rio Negro Pluton. The mafic mineral association is similar, but in contrasted relative abundance, to the ones found in the main granites. In the main granites the amphiboles are Fe-horblende and Fe-edenite, with 0.65 < fe# < 0.95, the higher among these values appearing in the alkali-feldspar granites. Biotite present 0.70 < fe# < 0.99 and the annitic component are also higher in the later rocks. In the case of the gabbro-dioritic rocks, the fe# numbers range between 0.48 and 0.59, 0.41 and 0.56, 0.47 and 0.53 and 0.54 and 0.57 in ortopyroxene, clinopyroxene, amphibole and biotite, respectively. The averaged compositions of coexisting orto- and clinopyroxene are \'Wo IND.46\'\'En IND.30\'\'Fe IND.24\' and \'Wo IND.3\'\'En IND.42\'\'Fe IND.55\' and suggest a tholeiitic or calk-alkaline nature of the original melts. Rare earth element patterns reveal enrichment factors up to 1-10, 50-70, 100-300 relative to the chondritic composition in ortopyroxene, clinopyroxene and amphibole, respectively, with a well marked fractionation of the heavy over the light rare earths in the case of the ortopyroxene, a feature not observed in clinopyroxene and amphibole. All patterns show a notable Eu negative anomaly. Melts crystallization pressures were estimated to be between 1 and 3.5 kbar; however values higher than ca. 2 kbar seems to be unrealistic given the ferroan compositions of some amphiboles. Zircon and apatite saturation temperatures coupled with ortopyroxene-clinopyroxene and amphibole-plagioclase equilibrium temperatures suggest crystallization intervals between ca. 1000 - 750° C in the case of the gabbro-diorites and ca. 900 - 670° C in the case of the main granites. Mineral paragenesis and fe# values in biotite in equilibrium with alkali-feldspar and magnetite suggests relative oxidizing crystallization conditions for the acid and basic-intermediate melts, higher than the QFM buffer, the alkali-feldspat granites being a possible exeption.

No description available.

English abstract The thesis is devoted to the interpretation of gravity data in granitic intrusions of Moldanubian Pluton near Kaplice This research was based on gravimetric field measurements taken on two parallel profiles in April 2016. Data from the profiles were then processed and geologically interpreted. Evaluate of derived gravity data showed that the positions of increased gravity field gradient roughly correspond to mapped geological interface. Individual rock types can therefore be distinguished using gravimetry.