The Iron and Manitou Islands complexes are 560 m.y. old. They were associated with a magma chamber lying at moderate depth below these complexes, On a regional scale the emplacement is controlled by the Nipissing graben system, an extension of the St. Lawrence rift system, along which an alkaline igneous province, 560 m.y. old, is well developed. A variety of rock types is developed in these complexes in spite of their small size. This is a result of extensive differentiation, interaction of late fractions with already crystallized early fractions, interaction of a "fluid phase" with country rocks, partial melting of country rocks, and finally various late hydrothermal alterations. The high degree of differentiation is probably a consequence of the high amount of volatile components in the magma which lowers its viscosity, extends its crystallization range, and consequently enhances fractional crystallization. In addition, liquid immiscibility played an important role in the differentiation. During differentiation the pyroxenes changed in composition from Ca-rich varieties through aegirine-augite to acmite, There is no evidence of an immiscibility gap between Ca-rich and Na-rich pyroxenes as has been proposed by Aoki (1964) but criticized by later investigators, Members of the phlogopite-biotite solid solution series exhibit a compositional range from annite-12 to annite-63. The characteristic assemblage melilite; Ca-rich pyroxene, and olivine (partially or completely replaced olivine phenocrysts) occurring in some lamprophyres indicates low silica activity, 10^(-1.6) to 10^(-1.2). However, the silica activity of the Lamprophyres is not restricted to the above range since the presence of sphene in some Lamprophyre dykes indicates silica activity above this range. The required condition of excess sodium silicate for the crystallization of acmite in synthetic melts seems to be required in nature too. Lamprophyres have a crystallization temperature of about 950°C. Fenitization of the country rocks takes place from relatively low temperature, probably 480°F, to about 740°C where partial melting of the rocks occur. The development of the graben system and the alkaline igneous activity are both believed to be related to devolatilization processes in the mantle. / Thesis / Master of Science (MSc)

Thesis. 1975. Ph.D.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences. / Bibliography: leaves 124-128. / by James R. Besancon. / Ph.D.

Ce travail apporte de nouvelles contraintes sur les interactions entre déformation et processus d'hydratation et de percolation de magma ou de fluides et leurs implications sur les propriétés sismiques dans le coin mantellique. Il se base sur l'analyse de péridotites à spinelle provenant du massif de Ronda (Espagne) et deux séries de xénolites issues de zones de subduction actives (Kamchatka, Papouasie-Nouvelle-Guinée). L'étude structurale, pétrologique et géochimique de ces échantillons montrent qu'ils ont subi une percolation réactive de magma ou de fluide synchrone d'une déformation de haute température basse contrainte cohérente avec les condition PT de la base de la lithosphère ou de l'asthénosphère. Cette percolation réactive est responsable d'un enrichissement en pyroxènes localisés dans des bandes parallèles aux structures de déformation. Cet enrichissement est associé à la décroissance et à la désorientation des cristaux d'olivine. Le système de glissement dominant dans l'olivine est {0kl}[100], cela implique que la direction de polarisation rapide des ondes S dans la partie supérieure du coin mantellique est parallèle à la direction d'écoulement du manteau. L'enrichissement en pyroxène associé à une décroissance de l'intensité des OPR de l'olivine a pour conséquence une baisse non négligeable de l'anisotropie qui peut induire jusqu'à 33% d'erreur sur l'interprétation de la couche anisotrope. Un enrichissement en orthopyroxène peut entraîner une baisse du rapport Vp/Vs, mais ne peut expliquer des Vp/Vs <1,7 cartés dans certains avant-arcs. Cependant de telles valeurs peuvent être expliquées si l'anisotropie des péridotites du coin mantellique est prise en compte. / This work provides new constraints on the interactions between deformation and hydration process and the percolation of melt or fluids, and their implications for seismic properties of the mantle wedge. It is based on the analysis of spinel peridotites from the massif of Ronda (Spain) and two xenolith suites from active subduction zones (Kamchatka, Papua New Guinea). The structural, petrological and geochemical of these samples show that they underwent a reactive percolation of melt or fluid, which was synchronous to a deformation event occuring under high temperature and low stress consistent with the PT conditions of the base of the lithosphere or in the asthenosphere. This reactive percolation is responsible for pyroxenes enrichment localized in bands parallel to the deformation structures. This enrichment is associated with the grain size recuction and the disorientation of the crystals of olivine. The dominant slip system in olivine is {0 kl}[100], which results in fast S-wave polarization parallel to the flow direction in the mantle. The enrichment in pyroxene, associated with a decrease in the intensity of the olivine crystal preferred orientations, results in a significant decrease of the anisotropy that may induce error on the interpretation of the anisotropic layer (up to 33%). The observed orthopyroxene enrichment also lowers the Vp/Vs ratio, but cannot explain Vp/Vs < 1.7 mapped in some fore-arc mantles. Such low Vp/Vs ratios may however be explained by considering the intrinsic anisotropy of the peridotites, which is generally ignored in large-scale Vp/Vs ratio mapping of the mantle wedge.

Os nefelina sienitos miasquíticos a intermediários do Maciço Alcalino Poços de Caldas (MAPC), em especial o tipo da Pedreira, possuem enclaves microgranulares félsicos e máficoultramáficos intrigantes. O nefelina sienito da Pedreira (NeS) pode ser divido em duas fácies texturais: uma de granulação média-grossa a grossa (NeS-g), outra de granulação média-fina a fina (NeS-f). O NeSg possui, mais comumente, enclaves microgranulares félsicos (EMF), de composição fonolítica. Estes enclaves podem envolver enclaves menores, máfico-ultramáficos, gerando enclaves duplos. O NeSf apresenta mais tipicamente enclaves microgranulares máfico-ultramáficos (EMM), ora com feições de rompimento em estado plástico, ora com bordas angulosas e lineares. Diques de composição fonolítica cortam o NeS-g. As rochas estudadas neste trabalho são constituídas por nefelina, feldspato alcalino e clinopiroxênio. Como fase acessória, têm-se titanita, magnetita e biotita-flogopita. Apatita ocorre também como mineral acessório, com exceção para o NeS-g. No NeS-g, no NeS-f e nos EMF, o clinopiroxênio possui duas fases texturais: uma prismática, verde (egirina-augita) que também pode ter núcleo róseo/incolor (diopsídio, mais comum no NeS-f e no EMF); outra fibrosa, também verde, porém fortemente pleocroica (egirina). Os EMM são constituídos essencialmente por diopsídio, com M(médio)~80. Quando porfirítico, o enclave possui macrocristais de diopsídio róseo/incolor (#mg~0,9) imersos numa matriz de diopsídio verde (#mg~0,8), ambos prismáticos. Magnetita dos NeS possui pouca variação, com teores baixos de Ti, diferente da magnetita dos enclaves. A assinatura química da nefelina dos EMM é equivalente à do NeS-f, com mais Fe3+ e menos K em relação ao NeS-g. Feldspato alcalino tende a ser mais potássico nos EMF e apresenta maior variação composicional nos EMM (Ab10-33Or72-80). Biotita está presente somente nos EMF e flogopita somente nos EMM. O padrão de elementos terras raras (ETR) do clinopiroxênio róseo/incolor do NeS-f é semelhante ao do EMM. Egirina-augita e egirina possuem enriquecimento em ETR pesados. Os enclaves máfico-ultramáficos são ultrabásicos, classificados como tefritos/basanitos (Le Bas et al., 1986) ou nefelinitos/ankaratritos (De La Roche et al., 1980), enquanto as rochas félsicas são intermediárias, correspondentes a fonolitos ou nefelina sienitos, dependendo da granulometria. Os diques e o NeS-f são peralcalinos, enquanto o EMF, o NeS-g e os EMM são peralcalinos/metaluminosos. As rochas ultramáficas/ultrabásicas, aflorantes na porção noroeste do Maciço Alcalino Poços de Caldas (Ulbrich et al., 2002), possuem padrões de ETR que indicam que estas rochas podem estar geneticamente ligadas aos enclaves máfico-ultramáficos. De uma forma geral, as características estruturais, texturais e químicas das rochas estudadas corroboram com a hipótese de coexistência de pelo menos dois magmas distintos: um félsico sienítico insaturado outro ultramáfico/ultrabásico, que teriam interagido e formado os os EMM e o NeSf, principalmente. Enquanto num estágio posterior de cristalização do magma, porém ainda em estado plástico, o dique teria se colocado, com parcial absorção da rocha pelos nefelina sienitos, formando os EMF. / The miaskitic to intermediate nepheline syenites of Poços de Caldas Alkaline Massif, especially the Pedreira type, have intriguing felsic and mafic-ultramafic microgranular enclaves. The Pedreiras nepheline syenite type (NeS) can be divided into two textural facies: one that is medium-coarse to coarse grained (NeS-c) and the other that varies between medium-fine to fine grained (NeS-f). It is common among the NeS-c microgranular felsic enclaves (MFE) with phonolitic composition. These enclaves may develop smaller ones maficultramafic, generating double enclaves. The NeS-f usually presents mafic-ultramafic enclaves (MME), sometimes showing disrupted features in plastic stage and sometimes angular and linear edges. Phonolitic dykes cut the NeS-c. The rocks studied in this work are formed by nepheline, alkali-feldspar and clinopyroxene. The accessory phase is characterized by titanite, magnetite and biotite-phlogopite. In exception to the NeS-c, apatite also occurs as an accessory mineral. In the NeS-c, NeS-f and MFE, the clinopyroxene presents two textural phases: a green prismatic one (aegirine-augite), which also may have a pinkish/colourless core (diopsyde, which is common in the NeS-f and MFE); the other one is fibrous, also green, however with strongly pleocroism (aegirine). Essencially, the MME are formed by diopsyde, with M(medium)~80. When porphyritic, the enclave has macrocrystals of pinkish/colourless diopsyde (with mg#~0,9) in a green diopsyde (mg#~0,8) matrix, both prismatic. In the NeS, the magnetite varies little: with low levels of Ti, differently from the enclaves magnetite. The chemical signature of the nepheline in the MME equals to the one present in the NeS-f and has more Fe3+ and less K when compared to the NeS-c. The alkaline feldspar in the MFE has more potassium in its structure and presents a higher compositional variation in the MME (Ab10-33Or72-80). It is also noticeable that biotite is a component only to the MFE, while the phlogopite occurs in the MME. The rare earth elements (REE) pattern in the pinkish/colourless clinopyroxene of the NeS-f is similar to the MME. Both aegirine-augite and aegirine present an enrichment regarding the heavy REE. The MME are ultrabasic, classified as tephrite/basanite (Le Bas et al., 1986) or nephelinite/ankaratrites (De La Roche et al., 1980), while the felsic rocks are intermediate, corresponding to phonolite and nepheline syenite, depending on the grain size. The dykes and the NeS-f are peralkaline, while the MFE, NeS-c and the MME are peralkaline/metaluminous. The ultrabasic/ultrapotassic rocks, outcropping in the northwestern portion of the PCAM (Ulbrich et al., 2002), have REE patterns wich indicate that these rocks may be genetically related to mafic-ultramafic enclaves. Generally, the structural, textural and chemical signatures of the rocks studied in this work confirm the hypothesis of the coexistence of at least two different magmas: a syenitic undersaturated felsic one and a ultramafic/ultrabasic one, and their interaction resulted in the MME and, above all, the NeS-f. While in a late stage of magma cristalization, but still in the plastic state, the dike would be placed, with partial absorption of the rock by the nepheline syenite, resulting in the EMF.

Os nefelina sienitos miasquíticos a intermediários do Maciço Alcalino Poços de Caldas (MAPC), em especial o tipo da Pedreira, possuem enclaves microgranulares félsicos e máficoultramáficos intrigantes. O nefelina sienito da Pedreira (NeS) pode ser divido em duas fácies texturais: uma de granulação média-grossa a grossa (NeS-g), outra de granulação média-fina a fina (NeS-f). O NeSg possui, mais comumente, enclaves microgranulares félsicos (EMF), de composição fonolítica. Estes enclaves podem envolver enclaves menores, máfico-ultramáficos, gerando enclaves duplos. O NeSf apresenta mais tipicamente enclaves microgranulares máfico-ultramáficos (EMM), ora com feições de rompimento em estado plástico, ora com bordas angulosas e lineares. Diques de composição fonolítica cortam o NeS-g. As rochas estudadas neste trabalho são constituídas por nefelina, feldspato alcalino e clinopiroxênio. Como fase acessória, têm-se titanita, magnetita e biotita-flogopita. Apatita ocorre também como mineral acessório, com exceção para o NeS-g. No NeS-g, no NeS-f e nos EMF, o clinopiroxênio possui duas fases texturais: uma prismática, verde (egirina-augita) que também pode ter núcleo róseo/incolor (diopsídio, mais comum no NeS-f e no EMF); outra fibrosa, também verde, porém fortemente pleocroica (egirina). Os EMM são constituídos essencialmente por diopsídio, com M(médio)~80. Quando porfirítico, o enclave possui macrocristais de diopsídio róseo/incolor (#mg~0,9) imersos numa matriz de diopsídio verde (#mg~0,8), ambos prismáticos. Magnetita dos NeS possui pouca variação, com teores baixos de Ti, diferente da magnetita dos enclaves. A assinatura química da nefelina dos EMM é equivalente à do NeS-f, com mais Fe3+ e menos K em relação ao NeS-g. Feldspato alcalino tende a ser mais potássico nos EMF e apresenta maior variação composicional nos EMM (Ab10-33Or72-80). Biotita está presente somente nos EMF e flogopita somente nos EMM. O padrão de elementos terras raras (ETR) do clinopiroxênio róseo/incolor do NeS-f é semelhante ao do EMM. Egirina-augita e egirina possuem enriquecimento em ETR pesados. Os enclaves máfico-ultramáficos são ultrabásicos, classificados como tefritos/basanitos (Le Bas et al., 1986) ou nefelinitos/ankaratritos (De La Roche et al., 1980), enquanto as rochas félsicas são intermediárias, correspondentes a fonolitos ou nefelina sienitos, dependendo da granulometria. Os diques e o NeS-f são peralcalinos, enquanto o EMF, o NeS-g e os EMM são peralcalinos/metaluminosos. As rochas ultramáficas/ultrabásicas, aflorantes na porção noroeste do Maciço Alcalino Poços de Caldas (Ulbrich et al., 2002), possuem padrões de ETR que indicam que estas rochas podem estar geneticamente ligadas aos enclaves máfico-ultramáficos. De uma forma geral, as características estruturais, texturais e químicas das rochas estudadas corroboram com a hipótese de coexistência de pelo menos dois magmas distintos: um félsico sienítico insaturado outro ultramáfico/ultrabásico, que teriam interagido e formado os os EMM e o NeSf, principalmente. Enquanto num estágio posterior de cristalização do magma, porém ainda em estado plástico, o dique teria se colocado, com parcial absorção da rocha pelos nefelina sienitos, formando os EMF. / The miaskitic to intermediate nepheline syenites of Poços de Caldas Alkaline Massif, especially the Pedreira type, have intriguing felsic and mafic-ultramafic microgranular enclaves. The Pedreiras nepheline syenite type (NeS) can be divided into two textural facies: one that is medium-coarse to coarse grained (NeS-c) and the other that varies between medium-fine to fine grained (NeS-f). It is common among the NeS-c microgranular felsic enclaves (MFE) with phonolitic composition. These enclaves may develop smaller ones maficultramafic, generating double enclaves. The NeS-f usually presents mafic-ultramafic enclaves (MME), sometimes showing disrupted features in plastic stage and sometimes angular and linear edges. Phonolitic dykes cut the NeS-c. The rocks studied in this work are formed by nepheline, alkali-feldspar and clinopyroxene. The accessory phase is characterized by titanite, magnetite and biotite-phlogopite. In exception to the NeS-c, apatite also occurs as an accessory mineral. In the NeS-c, NeS-f and MFE, the clinopyroxene presents two textural phases: a green prismatic one (aegirine-augite), which also may have a pinkish/colourless core (diopsyde, which is common in the NeS-f and MFE); the other one is fibrous, also green, however with strongly pleocroism (aegirine). Essencially, the MME are formed by diopsyde, with M(medium)~80. When porphyritic, the enclave has macrocrystals of pinkish/colourless diopsyde (with mg#~0,9) in a green diopsyde (mg#~0,8) matrix, both prismatic. In the NeS, the magnetite varies little: with low levels of Ti, differently from the enclaves magnetite. The chemical signature of the nepheline in the MME equals to the one present in the NeS-f and has more Fe3+ and less K when compared to the NeS-c. The alkaline feldspar in the MFE has more potassium in its structure and presents a higher compositional variation in the MME (Ab10-33Or72-80). It is also noticeable that biotite is a component only to the MFE, while the phlogopite occurs in the MME. The rare earth elements (REE) pattern in the pinkish/colourless clinopyroxene of the NeS-f is similar to the MME. Both aegirine-augite and aegirine present an enrichment regarding the heavy REE. The MME are ultrabasic, classified as tephrite/basanite (Le Bas et al., 1986) or nephelinite/ankaratrites (De La Roche et al., 1980), while the felsic rocks are intermediate, corresponding to phonolite and nepheline syenite, depending on the grain size. The dykes and the NeS-f are peralkaline, while the MFE, NeS-c and the MME are peralkaline/metaluminous. The ultrabasic/ultrapotassic rocks, outcropping in the northwestern portion of the PCAM (Ulbrich et al., 2002), have REE patterns wich indicate that these rocks may be genetically related to mafic-ultramafic enclaves. Generally, the structural, textural and chemical signatures of the rocks studied in this work confirm the hypothesis of the coexistence of at least two different magmas: a syenitic undersaturated felsic one and a ultramafic/ultrabasic one, and their interaction resulted in the MME and, above all, the NeS-f. While in a late stage of magma cristalization, but still in the plastic state, the dike would be placed, with partial absorption of the rock by the nepheline syenite, resulting in the EMF.

Les péridotites, roches du manteau terrestre, sont instables en présence d'eau et peuvent se transformer en un minéral hydraté la serpentine, qui a la capacité remarquable de générer de l'hydrogène H2; cette réaction s'appelle la serpentinisation. Au niveau des dorsales médio-océaniques, la circulation d'eau dans ces roches conduit à la formation de larges systèmes hydrothermaux. Ils montrent différentes conditions de température et de pH des fluides, bien qu'ils conduisent tous à la formation abiotique d'H2, de méthane CH4 et possiblement d'autres hydrocarbures légers.Cette thèse est dédiée à l'étude du rôle de la composition chimique du fluide hydrothermal sur la cinétique et les mécanismes de serpentinisation des roches ultrabasiques à différentes conditions de P-T. L'interaction entre l'olivine et/ou l'orthopyroxène a été analysée avec une solution aqueuse simulant une eau de mer enrichie en aluminium et/ou en ions bicarbonates, à différents pH. Une première série d'expériences a été réalisée à 200, 340 °C et 200 MPa en lp-DAC à l'ESRF en France. Elle a permis de quantifier les paramètres cinétiques de réaction, de déterminer un effet opposé de l'aluminium sur la cinétique de ces deux minéraux et l'accélération de la réaction en conditions alcalins. Autres expériences ont été réalisée à Pamb et 80 °C en flacons de verre. Elles ont conduit, pour la première fois, à la formation de serpentine ainsi qu'à la formation d'H2 et de CH4. Ces résultats montrent qu'une chimie plus complexe du fluide hydrothermal peut avoir un impact majeur sur la cinétique de la serpentinisation pour l'accélérer et la rendre plus accessible à une échelle de temps industrielle / Peridotites, Earth's mantle rocks, are unstable in the presence of water and can be transformed into a hydrated mineral, serpentine, which has the remarkable ability to generate hydrogen H2; this reaction is called serpentinization. At the mid-ocean ridges, the circulation of water in these rocks leads to the formation of large hydrothermal systems. They show great variability of temperature and fluids’pH conditions, although they all lead to the abiotic formation of H2, methane CH4 and eventually other light hydrocarbons. This PhD thesis is dedicated to the study of the chemical composition role of the hydrothermal fluid on the kinetics and mechanisms of serpentinization of ultramafic rocks to different conditions of P-T. The interaction between olivine and/or orthopyroxene was analyzed with an aqueous solution to simulate sea water which is rich in aluminum and/or bicarbonate ions, with different pH values. A first series of experiments was carried out at 200, 340 °C and 200 MPa in lp-DAC at the ESRF in France. It was used to quantify the kinetic parameters of the reaction, to determine an opposite effect of aluminum on the kinetics these two minerals and the acceleration of the reaction under alkaline conditions. Other experiments were performed in glass bottles at Pamb and 80 °C. They led, for the first time, to the formation of serpentine, as well as to the formation of H2 and CH4. These results show that the slightly more complex chemistry of the hydrothermal fluid can have a major impact on the kinetics of serpentinization to speed and make it more accessible to industrial time scale

Determining mafic mineral composition of asteroid bodies is a topic reviewed by M.J. Gaffey et al. (2002). The iterative procedure discussed can be implemented as an algorithm, and such efforts revealed weaknesses that are examined in this work. We seek to illustrate the limits of this method and graphically determine its predictions. There are boundaries in the formulae given where the equations break down. In ranges where mafic mixtures are predicted, a method is illustrated that allows a decoupling of these mixtures into the constituents.

Contents of major, minor and trace elements in clinopyroxenes and clinoamphiboles of basanites, volcanoclastics, essexites, sodalitic syenites, and monzodiorites of the České středohoří Mts. has been determined using an electrone microprobe and LA-ICP-MS techniques. Composition of clinopyroxenes corresponds to either diopside or augite and clinoamphiboles can be classified as kaersutite or pargasite. Some pyroxenes display pronounced sector zoning showing increased contents of Mg and Si in pyramidal sectors whereas prismatic sectors show Fe, Ti and Al enrichment. Chemical composition of both sectors corresponds to diopside. Growth zoning has been found in the samples from basanites and volcanoclastics. Grain cores display the chemistry of augite and towards the rim the chemical composition changes to diopside. Samples have also been analyzed by powder and single crystal X-ray diffraction techniques. Samples of pyroxenes appear to be either pure or they contain negligible admixtures of phlogopite. Samples of amphiboles are also either without any admixtures or they show contamination by low amounts of diopside or augite, or phlogopite may rarely be encountered. Mutual relationship between the size of the unit cell parameters b and and substitutions in M1,2,3 and A sites has been observed. Longer mean T-O...

Les laves d'arc ont une géochimie complexe du fait de l'hétérogénéité des magmas primitifs et de leur transformation dans la croûte. L'identification des magmas primitifs dans les arcs continentaux est difficile du fait de l'épaisseur de la croûte continentale, qui constitue un filtre mécanique et chimique à l'ascension des magmas. En Équateur, cette problématique est particulièrement critique du fait de la grande épaisseur de la croûte (≈ 50-60 km) et de la rareté des magmas primitifs arrivant en surface. Cette thèse a pour but de déterminer la composition des liquides primitifs dans l'arc équatorien, à l'échelle de l'arc entier, et à celle de deux édifices volcaniques : le Pichincha et le Tungurahua. Elle vise également à mieux comprendre comment ces liquides primitifs évoluent à travers la croûte continentale. En Équateur, le pendage, le relief et l'âge de la plaque plongeante varient du nord au sud de l'arc. Ainsi, la première partie de la thèse aborde la question de l'influence de ces paramètres sur la géochimie des magmas, via une étude sur roches totales couvrant la totalité de l'arc. Elle confirme les variations géochimiques décrites à travers l'arc par les études précédentes : augmentation de la teneur en éléments incompatibles et diminution de l'enrichissement en éléments "mobiles" d'est en ouest. L'étude identifie des variations géochimiques le long du front volcanique (e.g., rapport Ba/Th), liées au changement de nature des fluides métasomatiques, qui sont aqueux au centre de l'arc (environ 0,5°S) et silicatés au Nord et possiblement au Sud. Ce changement est attribué à la jeunesse du plancher océanique dans le nord de l'arc, qui pourrait promouvoir la fusion de la plaque plongeante. Enfin, il semble que la contamination par la croûte inférieure augmente vers le sud du front volcanique. Dans un deuxième temps, les produits émis par le Tungurahua lors de ses derniers 3000 ans d'activité sont étudiés. À cette échelle de temps, les paramètres tectoniques de la première étude sont constants. Ce travail détaille le rôle de la croûte dans la production des magmas différenciés, qui sont systématiquement associés à des éruptions plus explosives. Elle conclut que les andésites ont des compositions isotopiques hétérogènes (206Pb/204Pb = 18,834 - 19,038), acquises en profondeur (manteau ou croûte inférieure), qui se restreignent lors de la différenciation des andésites en dacites (206Pb/204Pb = 18,965 - 19,030), par cristallisation fractionnée et assimilation de la croûte supérieure locale (7-9 %). Enfin, la troisième partie de la thèse se focalise sur l'hétérogénéité des magmas primitifs. Des études sur minéraux individuels ont été effectuées au Pichincha et au Tungurahua, et montrent que la majorité des minéraux sont en déséquilibre avec la roche hôte (jusqu'à 8600 ppm en 206Pb/204Pb). Au Pichincha, la diversité des minéraux échantillonnés permet d'identifier la diversité des liquides mantelliques (206Pb/204Pb = 18,816 - 19,007), qui s'alignent dans les espaces Pb-Pb. Comme dans le cas des roches totales du Tungurahua, l'assimilation crustale écrase cette diversité isotopique lors de la différenciation des liquides primitifs, dont la signature n'est pas préservée dans les roches. Au Tungurahua, les minéraux individuels montrent que l'hétérogénéité des signatures est acquise en profondeur. L'analyse de deux lots d'olivines met en évidence une signature radiogénique dans les liquides primitifs du Tungurahua, interprétée comme la présence de croûte délaminée dans la source mantellique du Tungurahua. Enfin, l'étude de lots d'olivines provenant de sept volcans équatoriens montre qu'il n'existe pas de signature primitive unique dans l'arc. La totalité de l'hétérogénéité isotopique des magmas est héritée du manteau (206Pb/204Pb = 18,583 - 19,000). Les compositions des liquides primitifs sont ensuite déviées par la contamination crustale, dans la majorité des cas, vers des signatures plus radiogéniques. / Arc lavas display a complex geochemistry resulting from the heterogeneity of primitive magmas and their transformation within the crust. Identifying primitive magma compositions in continental arcs is challenging because continental crust is thick and acts as a mechanical and chemical filter for ascending magmas. This issue is particularly criticial in Ecuador owing to the great thickness of the continental crust (≈ 50-60 km) and the scarcity of erupted primitive magmas. This thesis aims to determine the composition of primitive silicate melts in the Ecuadorian arc, on the scale of the whole arc, as well as on the scale of two volcanic edifices: the Pichincha and the Tungurahua. This study also intends to better understand how those primitive melts evolve during their journey through the continental crust. In Ecuador, slab dip, relief and age change from north to south. Hence, the first part of the PhD focuses on the influence of those parameters on magma geochemistry, through a whole rock study covering the entire arc. It confirms the across-arc geochemical variations described by previous studies: an increase of incompatible element contents and a decrease of fluid-mobile over fluid-immobile element ratios from west to east. We identify along-arc geochemical variations in the volcanic front (e.g. Ba/Th), related to the changing nature of metasomatic fluids, which are aqueous fluids at the centre of the arc (around 0.5°S) and silicate melts to the north and probably to the south. This change may be due to the subduction of a younger and warmer oceanic crust to the north, which might promote slab melting. Lastly, it seems that deep crustal contamination increases towards the south of the volcanic front. Secondly, volcanic products emitted for the last 3,000 years at Tungurahua are studied. On this timescale, the tectonic parameters of the first study are constant. This work details the role of continental crust in the production of differentiated magmas, which are systematically associated with more explosive eruptions. We conclude that andesites have heterogeneous isotopic compositions (206Pb/204Pb = 18.834 - 19.038), acquired at depth (mantle or deep crust), that homogeneize through andesite differentiation to dacite (206Pb/204Pb = 18.965 - 19.030) by fractional crystallization and assimilation of the local upper crust (7-9 %). Lastly, the third part of the PhD focuses on the heterogeneity of primitive magmas. We study individual minerals from Pichincha and Tungurahua volcanoes and show that most minerals are in disequilibrium with their host rock (up to 8,600 ppm for 206Pb/204Pb). The diversity of Pichincha minerals allows the identification of mantle melt diversity (206Pb/204Pb = 18.816 - 19.007), with compositions forming a tight trend in Pb-Pb isotope spaces. As for Tungurahua whole rocks, crustal assimilation erases the diversity of primitive melt isotope signatures through differentiation, so that primitive melt signatures are not preserved in whole rock samples. At Tungurahua, individual minerals show that the heterogeneity of isotope compositions is acquired at depth. The analysis of two olivine fractions reveals the existence of a radiogenic signature in the mantle source of Tungurahua volcano, interpreted as the presence of delaminated crust within the mantle beneath its edifice. Finally, olivine fractions from seven Ecuadorian volcanoes highlight the fact that no unique primitive signature exists in the arc. Isotopic heterogeneity is entirely inherited from the mantle (206Pb/204Pb = 18.583 - 19.000). Primitive melt compositions are then shifted by continental crust contamination which, in most cases, results in more radiogenic signatures.