Geología de las ultramafitas pre-andinas de Tapo y Acobamba, Tarma, en la Cordillera Oriental de Perú

Ultramafic rocks occur scattered along a 300 km long NNW-SSE trending belt, parallel to the central Peruvian Andes in the Cordillera Oriental, from Tarma (Junín Dept.) to Huancapallac and Tingo María (Huánuco Dept.). The Tarma occurrences (Tapo and Acobamba) are dealt with here, as the first step of a broader research. The Tapo massif comprises strongly tectonised serpentinites with scarce peridotitic relics, amphibolites and podiform chromitites. It was overthrust on early Carboniferous metasedimentary rocks of the Andean basement (Ambo Group), and it shows evidences of a pre-Andean deformational history, not observed in the Ambo Group; the basal thrust plane is folded by the Andean tectonics. The two smaller Acobamba occurrences are also allochtonous and show similar tectonic features. Major and trace element composition of amphibolites point to a tholeiitic basalt (to picrobasalt) protolith, compatible with an ocean-ridge or ocean-island environment. Small podiform chromitite lenses and chromite disseminations also occur; they are strongly deformed, metamorphosed and overprinted by hydrothermal alteration related to deformation, and were the subject of small scale mining. The ores comprise mainly chromite, ferritchromite, spinel, magnetite, ilmenite and scarce sulphides, as well as the secondary minerals stichtite and nimite. Results of this work exclude current interpretations of the Tarma ultramafites as autochtonous igneous intrusives, and point to a new interpretation for their emplacement.

Las mineralizaciones auríferas de Galicia Occidental en la Zona de Cizalla Busto-Limideiro (A Coruña)

Las mineralizaciones de oro de Galicia Occidental ligadas a grandes estructuras comienzan a ser interpretadas de manera más rigurosa, al mismo tiempo que la continuada elevación de las cotizaciones del oro han hecho más atractiva la reactivación de áreas hasta ahora casi olvidadas. El propósito de esta investigación participa de las razones anteriores. La zona de cizalla Busto Limideiro se inscribe en una de estas estructuras, la cizalla Santa Comba-Punta Langosteira, con la que se relacionan un importante número de yacimientos auríferos entre los que destacan Corcoesto y Monte Piñor. Por su situación geológica, estos indicios se enmarcan en el Macizo Ibérico, en la Zona de Galicia Tras-os-Montes. Este trabajo aporta más conocimiento sobre un modelo general del oro de los yacimientos del noroeste español, integrándolo en los yacimientos de oro orogénico del Varisco europeo. Este estudio ha supuesto un importante esfuerzo investigador centrado sobre de los procesos genéticos que han dado lugar a las mineralizaciones auríferas. Los estudios petrográficos, metalogénicos, geoquímicos, microtemométricos y el análisis de isótopos han permitido establecer un modelo general y otros más específicos sobre la existencia y condiciones de formación en la concentración del oro mineralógico. De esta forma se ha caracterizado su mineralogía, quimismo, edad, y naturaleza de los paleofluidos que han intervinieron en su formación. De los resultados obtenidos se destaca que estas mineralizaciones se encuentran fuertemente ligadas a las estructuras y transformaciones físicas y químicas de las rocas afectadas por la banda de cizalla. Derivada de esta situación, se comprende la disposición espacial, a diversas escalas, con estructuras claramente en la transición del dominio dúctil a frágil. Además, resulta evidente, a escala macro y microscópica, el emplazamiento preferente del oro en estructuras de deformación miloníticas. Los estudios anteriores posibilitan formalizar un modelo de génesis para el yacimiento de Monte Piñor que resulta compatible con el establecido por Groves (1998), e incluirlas en un mismo contexto, como yacimientos de oro orogénico mesotermales, válido para el conjunto de todos los de la zona de cizalla Busto Limideiro. El estudio no omite la consideración geoestadística de este yacimiento, justificando la elección de direcciones de anisotropía explicadas por consideraciones de carácter estructural. Con ello, buscando el lado práctico desde el punto de vista minero, esta investigación propone líneas generales de aplicación de actuación con sentido de exploración, contribuyendo a la puesta en valor del conocimiento de las mineralizaciones de oro del noroeste español. ABSTRACT Old and nearly forgotten gold mines from Western Galicia are currently attractive to be recovered due to both, the new strict interpretation of gold mineralization linked to Variscan large structures and the increasing gold prices. The shear zone Busto Limiderio is relevant as a part of a Variscan large structure, Santa Comba-Punta Langosteira, which is related with a high number of gold deposits as Corcoesto and Monte Piñor. For its geological situation, these signs are part of the Iberian Massif in the area of Galicia Tras-os-Montes. Hence, the main aim of this study is to provide additional and important knowledge of Busto Limiderio about the general model of gold deposits in the Spanish northwest, integrating them in the orogenic gold deposits of European Variscan, enabling to analyze the economic recovery possibility of this area. This thesis has been focused on the genetic processes that have led to the gold mineralization. Petrographic studies, metalogenic, geochemical, microthermometric and isotope analysis have allowed to establish a general and specific models about the existence and training conditions in the concentration of mineralogical gold. Consequently, the mineralogy, chemical characteristics, age, and nature of paleofluids that have participated in its formation have been characterized. The results showed that Busto Limiderio gold mineralization are strongly linked to the structures and physical and chemical transformations of affected rocks by the shear band. The mineralization spatial distribution at various scales is due to the link with the large structures in the ductile-to-brittle transition domain. Furthermore, this factor determine at macro and microscopic scale, the preferred location of the gold structures mylonitic deformation. Previous studies have permitted to establish a model of genesis for the site of Monte Piñor which is compatible with the established by Groves (1998), and also to include them in the same context as mesothermal orogenic gold deposits, valid throughout all of Busto Limideiro shear zone. This study does not omit consideration of the geostatistical deposit, justifying the choice of directions of anisotropy explained by structural considerations. This thesis concludes with general action guidelines for mining exploration, contributing to the enhancement of knowledge of Spanish gold mineralization northwest.

Un traité de la vie solitaire. Epistola ad fratres de Monte-Dei.

Attributed to Bernard de Clairvauv, Peter Cellensis and Guigues du Chastel.

La morale monastique du XIe au XVIe siècle : pour l'histoire de la théologie morale /

Includes bibliographical references and index.

Geochemistry of Atlantis Massif crust

The Atlantis Massif (Mid-Atlantic Ridge, 30°N) is an oceanic core complex marked by distinct variations in crustal architecture, deformation and metamorphism over distances of at least 5 km. We report Sr and Nd isotope data and Rare Earth Element (REE) concentrations of gabbroic and ultramafic rocks drilled at the central dome (IODP Hole 1309D) and recovered by submersible from the southern ridge of the massif that underlie the peridotite-hosted Lost City Hydrothermal Field. Systematic variations between the two areas document variations in seawater penetration and degree of fluid-rock interaction during uplift and emplacement of the massif and hydrothermal activity associated with the formation of Lost City. Homogeneous Sr and Nd isotope compositions of the gabbroic rocks from the two areas (87Sr/86Sr: 0.70261-0.70429 and epsilon-Nd: +9.1 to +12.1) indicate an origin from a depleted mantle. At the central dome, serpentinized peridotites are rare and show elevated seawater-like Sr isotope compositions related to serpentinization at shallow crustal levels, whereas unaltered mantle isotopic compositions preserved in the gabbroic rocks attest to limited seawater interaction at depth. This portion of the massif remained relatively unaffected by Lost City hydrothermal activity. In contrast, pervasive alteration and seawater-like Sr and Nd isotope compositions of serpentinites at the southern wall (87Sr/86Sr: 0.70885-0.70918; epsilon-Nd: -4.7 to +11.3) indicate very high fluid-rock ratios (~20 and up to 10**6) and enhanced fluid fluxes during hydrothermal circulation. Our studies show that Nd isotopes are most sensitive to high fluid fluxes and are thus an important geochemical tracer for quantification of water-rock ratios in hydrothermal systems. Our results suggest that high fluxes and long-lived serpentinization processes may be critical to the formation of Lost City-type systems and that normal faulting and mass wasting in the south facilitate seawater penetration necessary to sustain hydrothermal activity.

Behavior of trace elements in quartz from plutons of different geochemical signature: a case study from the Bohemian Massif, Czech Republic

Trace-element content in igneous quartz from granitoids of different geochemical types from Bohemian Massif (Central Evrope) was investigated using the laser ablation ICP-MS technique. Two laboratories (Geological Survey of Norway, Trondheim, and Institute of Geology of the Academy of Science of Czech Republic, Praha) were involved in the trace-element (Li, Be, B, Mn, Ge, Rb, Ba, Pb, Mg, Al, P, Ca, Ti, Fe, and Sn) analyses of quartz (altogether, ~300 analyses of 17 rock samples). About 200 representative analyses of quartz are given in Tables 1 and 2.

Histoire évolutive de la galaxie spirale NGC 5430

La galaxie spirale barrée NGC 5430 est particulière en ce sens qu’elle présente un noeud Wolf-Rayet très lumineux et des bras asymétriques. Des spectres longue-fente le long de la barre et dans le bras déformé ainsi que des données SpIOMM couvrant l’ensemble de la galaxie ont été analysées. L’absorption stellaire sous-jacente a été soustraite des spectres longue-fente à l’aide d’un ajustement de modèles théoriques de populations stellaires fait avec le programme GANDALF. L’absorption a un impact très important sur le calcul de l’extinction ainsi que sur les différents diagnostics propres aux régions HII et aux populations stellaires jeunes. Enfin, cette étude montre que NGC 5430 comporte une composante gazeuse ionisée diffuse sur toute son étendue et qu’il est important d’en tenir compte afin d’appliquer correctement les diagnostics. Un des scénarios évolutifs proposés au terme de cette étude est que le noeud Wolf-Rayet constitue le restant d’une petite galaxie ou d’un nuage intergalactique qui serait entré en collision avec NGC 5430. Une structure englobant le noeud Wolf-Rayet se déplace à une vitesse considérablement inférieure (50 - 70 km s-1) à celle attendue à une telle distance du centre de la galaxie (200 - 220 km s-1). De plus, le noeud Wolf-Rayet semble très massif puisque l’intensité maximale du continu stellaire de cette région est semblable à celle du noyau et est de loin supérieure à celle de l’autre côté de la barre. Le nombre d’étoiles Wolf-Rayet (2150) est aussi considérable. Il n’est toutefois pas exclu que la différence de vitesses observée témoigne d’un écoulement de gaz le long de la barre, qui alimenterait la formation stellaire du noeud Wolf-Rayet ou du noyau.

Étude des rôles de la voie antioxydante Nrf2 et la voie anti-inflammatoire PPARγ dans le contrôle de l’inflammation lors d’infections sévères par l'influenza

Chaque année, la grippe provoque des centaines de milliers de décès dans le monde. Dans le cas d’infections sévères, il a été démontré que la génération excessive de molécules inflammatoires telles que les cytokines et les chimiokines, la sécrétion d’espèces réactives dérivées de l'oxygène ainsi que l’afflux massif de cellules immunitaires innées et adaptatives dans les voies respiratoires contribuent à la génération de dommages pulmonaires aigus et contribuent à l'immunopathologie reliée à l’infection. Tenant compte de ce fait, le défi actuel dans le traitement de la grippe est de contrôler la réponse inflammatoire tout en inhibant la réplication virale afin de permettre à l'organisme de se défendre contre les infections sévères à l'influenza. Des études récentes ont montré que l’activation du récepteur nucléaire PPARγ par ses ligands, tel que la 15d-PGJ[indice inférieur 2], diminuait l’inflammation pulmonaire et améliorait la survie des souris infectées avec des doses létales du virus influenza. Mis à part ses effets sur PPARγ, le ligand 15d-PGJ[indice inférieur 2] est aussi connu pour activer le facteur nucléaire antioxydant Nrf2. Il a été montré que Nrf2 réduit la réplication du virus influenza. Cependant, son mode d'action dans cette fonction nécessite une clarification. De manière intéressante, une étude a montré que Nrf2 réduit l’inflammation pulmonaire en régulant l’expression de PPARγ et ceci dans un modèle murin du syndrome de détresse respiratoire aigu. Les résultats de ces études précédentes mènent à l’hypothèse que les voies de PPARγ et Nrf2 interagissent fonctionnellement et qu'elles sont impliquées dans la réduction de l’inflammation induite lors d'infections sévères causées par l'influenza. L’objectif général de cette étude est donc de mieux comprendre les mécanismes protecteurs de PPARγ et Nrf2 dans la régulation de l’inflammation et la réplication virale suite à une infection par le virus influenza. Nos résultats ont démontré premièrement que le fait de cibler les deux voies moléculaires PPARγ et Nrf2, permet une inhibition significative de l’inflammation et de la morbidité liée à l’infection. Dans un deuxième temps, nos résultats dévoilent le mécanisme antiviral de Nrf2 et démontrent que l’activation de cette voie réduit la réplication du virus influenza d’une façon dépendante de l’expression de l’antiprotéase SLPI.

U-Pb geochronology and Nd isotope contributions to the interpretation of a peculiar ring massif: the Santa Eulália plutonic complex (SW Iberia, Portugal)

The Santa Eulalia plutonic complex (SEPC) is a late-Variscan granitic body placed in the Ossa-Morena Zone. The host rocks of the complex belong to metamorphic formations from Proterozoic to Lower Paleozoic. The SEPC is a ring massif (ca. 400 km2 area) composed by two main granitic facies with different colours and textures. From the rim to the core, there is (i) a peripheral pink medium- to coarse-grained granite (G0 group) involving large elongated masses of mafic and intermediate rocks, from gabbros to granodiorites (M group), and (ii) a central gray medium-grained granite (G1 group). The mafic to intermediate rocks (M group) are metaluminous and show wide compositions: 3.34–13.51 wt% MgO; 0.70–7.20 ppm Th; 0.84–1.06 (Eu/Eu*)N (Eu* calculated between Sm and Tb); 0.23–0.97 (Nb/Nb*)N (Nb* calculated between Th and La). Although involving the M-type bodies and forming the outer ring, the G0 granites are the most differentiated magmatic rocks of the SEPC, with a transitional character between metaluminous and peraluminous: 0.00–0.62 wt% MgO; 15.00–56.00 ppm Th; and 0.19–0.42 (Eu/Eu*)N ; 0.08–0.19 (Nb/Nb*)N [1][2]. The G1 group is composed by monzonitic granites with a dominant peraluminous character and represents the most homogeneous compositional group of the SEPC: 0.65–1.02 wt% MgO; 13.00–16.95 ppm Th; 0.57–0.70 (Eu/Eu*)N ; 0.14–0.16 (Nb/Nb*)N . According to the SiO2 vs. (Na2O+K2O–CaO) relationships, the M and G1 groups predominantly fall in the calc-alkaline field, while the G0 group is essencially alkali-calcic; on the basis of the SiO2 vs. FeOt/(FeOt+MgO) correlation, SEPC should be considered as a magnesian plutonic association [3]. New geochronological data (U-Pb on zircons) slightly correct the age of the SEPC, previously obtained by other methods (290 Ma, [4]). They provide ages of 306  2 Ma for the M group, 305  6 Ma for the G1 group, and 301  4 Ma for the G0 group, which confirm the late-Variscan character of the SEPC, indicating however a faintly older emplacement, during the Upper Carboniferous. Recent whole-rock isotopic data show that the Rb-Sr system suffered significant post-magmatic disturbance, but reveal a consistent set of Sm-Nd results valuable in the approach to the magmatic sources of this massif: M group (2.9 < Ndi < +1.8); G1 group (5.8 < Ndi < 4.6); G0 group (2.2 < Ndi < 0.8). These geochemical data suggest a petrogenetic model for the SEPC explained by a magmatic event developed in two stages. Initially, magmas derived from long-term depleted mantle sources (Ndi < +1.8 in M group) were extracted to the crust promoting its partial melting and extensive mixing and/or AFC magmatic evolution, thereby generating the G1 granites (Ndi < 4.6). Subsequently, a later extraction of similar primary magmas in the same place or nearby, could have caused partial melting of some intermediate facies (e.g. diorites) of the M group, followed by magmatic differentiation processes, mainly fractional crystallization, able to produce residual liquids compositionally close to the G0 granites (Ndi < 0.8). The kinetic energy associated with the structurally controlled (cauldron subsidence type?) motion of the G0 liquids to the periphery, would have been strong enough to drag up M group blocks as those occurring inside the G0 granitic ring.