951 resultados para Génération de textures


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The ancient southern highlands on Mars (~3.5 Gyr old) contain > 600 regions that display spectral evidence in the infrared for the presence of chloride-bearing materials. Many of these locations were previously reported to display polygonal cracking patterns. We studied more than 80 of the chloride-bearing terrains using high-resolution (0.25-0.5 m/pixel) images, as well as near-infrared spectral data, to characterize the surface textures and the associated cracking patterns and mineralogies. Our study indicates that ~75% of the studied locations display polygonal cracks that resemble desiccation cracks, while some resemble salt expansion/thrust polygons. Furthermore, we detect, spectrally, the presence of smectites in association with ~30% of the studied fractured terrains. We note that smectites are a special class of swelling clay minerals that can induce formation of large desiccation cracks. As such, we suggest that the cracking patterns are indicative of the presence of smectite phyllosilicates even in the absence of spectral confirmation. Our results suggest that many chloride-bearing terrains have a lacustrine origin and a geologic setting similar to playas on Earth. Such locations would have contained ephemeral lakes that may have undergone repeated cycles of desiccation and recharging by a near-surface fluctuating water table in order to account for the salt-phyllosilicates associations. These results have notable implications for the ancient hydrology of Mars. We propose that the morphologies and sizes of the polygonal cracks can be used as paleoenvironmental, as well as lithological, indicators that could be helpful in planning future missions.

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We have measured the bidirectional reflectance of analogs of dry, wet, and frozen Martian soils over a wide range of phase angles in the visible spectral range. All samples were produced from two geologic samples: the standard JSC Mars-1 soil simulant and Hawaiian basaltic sand. In a first step, experiments were conducted with the dry samples to investigate the effects of surface texture. Comparisons with results independently obtained by different teams with similar samples showed a satisfying reproducibility of the photometric measurements as well as a noticeable influence of surface textures resulting from different sample preparation procedures. In a second step, water was introduced to produce wet and frozen samples and their photometry investigated. Optical microscope images of the samples provided information about their microtexture. Liquid water, even in relatively low amount, resulted in the disappearance of the backscattering peak and the appearance of a forward-scattering peak whose intensity increases with the amount of water. Specular reflections only appeared when water was present in an amount large enough to allow water to form a film at the surface of the sample. Icy samples showed a wide variability of photometric properties depending on the physical properties of the water ice. We discuss the implications of these measurements in terms of the expected photometric behavior of the Martian surface, from equatorial to circum-polar regions. In particular, we propose some simple photometric criteria to improve the identification of wet and/or icy soils from multiple observations under different geometries.

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Microstructures and textures of calcite mylonites from the Morcles nappe large-scale shear zone in southwestern Switzerland develop principally as a function of 1) extrinsic physical parameters including temperature, stress, strain, strain rate and 2) intrinsic parameters, such as mineral composition. We collected rock samples at a single location from this shear zone, on which laboratory ultrasonic velocities, texture and microstructures were investigated and quantified. The samples had different concentration of secondary mineral phases (< 5 up to 40 vol.%). Measured seismic P wave anisotropy ranges from 6.5% for polyphase mylonites (~ 40 vol.%) to 18.4% in mylonites with < 5 vol.% secondary phases. Texture strength of calcite is the main factor governing the seismic P wave anisotropy. Measured S wave splitting is generally highest in the foliation plane, but its origin is more difficult to explain solely by calcite texture. Additional texture measurements were made on calcite mylonites with low concentration of secondary phases (≤ 10 vol.%) along the metamorphic gradient of the shear zone (15 km distance). A systematic increase in texture strength is observed moving from the frontal part of the shear zone (anchimetamorphism; 280 °C) to the higher temperature, basal part (greenschist facies; 350–400 °C). Calculated P wave velocities become increasingly anisotropic towards the high-strain part of the nappe, from an average of 5.8% in the frontal part to 13.2% in the root of the basal part. Secondary phases raise an additional complexity, and may act either to increase or decrease seismic anisotropy of shear zone mylonites. In light of our findings we reinterpret the origin of some seismically reflective layers in the Grône–Zweisimmen line in southwestern Switzerland (PNR20 Swiss National Research Program). We hypothesize that reflections originate in part from the lateral variation in textural and microstructural arrangement of calcite mylonites in shear zones.

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La présente contribution porte sur le passage dans le degré tertiaire en tenant compte de l’intrication des inégalités liées au sexe et au contexte migratoire. L’étude, qui repose sur des concepts de la théorie décisionnelle, s’articule principalement sur une comparaison entre la Suisse (TREE), l’Allemagne (élèves pouvant prétendre aux études supérieures 2002 HIS) et la France (Panel d'élèves du second degré 1995). Les résultats révèlent qu’en Suisse et en Allemagne, indépendamment de l’origine sociale, les jeunes hommes appartenant à certains groupes de migrants socialement défavorisés (2e génération) affichent un taux de passage dans le supérieur plus élevé que leurs camarades nationaux. Ils mettent par ailleurs en évidence que, ni en Suisse, ni en Allemagne, ni en France, les migrantes de deuxième génération issues de pays fortement marqués par le modèle patriarcal sont désavantagées.

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1944/1945 wurde in Cham-Hagendorn eine Wassermühle ausgegraben, die dank ihrer aussergewöhnlich guten Holzerhaltung seit langem einen prominenten Platz in der Forschung einnimmt. 2003 und 2004 konnte die Kantonsarchäologie Zug den Platz erneut archäologisch untersuchen. Dabei wurden nicht nur weitere Reste der Wassermühle, sondern auch Spuren älterer und jüngerer Anlagen geborgen: eine ältere und eine jüngere Schmiedewerkstatt (Horizont 1a/Horizont 3) sowie ein zweiphasiges Heiligtum (Horizonte 1a/1b). All diese Anlagen lassen sich nun in das in den neuen Grabungen erkannte stratigraphische Gerüst einhängen (s. Beil. 2). Dank der Holzerhaltung können die meisten Phasen dendrochronologisch datiert werden (s. Abb. 4.1/1a): Horizont 1a mit Schlagdaten zwischen 162(?)/173 und 200 n. Chr., Horizont 1b um 215/218 n. Chr. und Horizont 2 um 231 n. Chr. Ferner konnten in den neuen Grabungen Proben für mikromorphologische und archäobotanische Untersuchungen entnommen werden (Kap. 2.2; 3.11). In der vorliegenden Publikation werden der Befund und die Baustrukturen vorgelegt, (Kap. 2), desgleichen sämtliche stratifizierten Funde und eine umfassende Auswahl der 1944/1945 geborgenen Funde (Kap. 3). Dank anpassender Fragmente, sog. Passscherben, lassen sich diese zum Teil nachträglich in die Schichtenabfolge einbinden. Die mikromorphologischen und die archäobotanischen Untersuchungen (Kap. 2.2; 3.11) zeigen, dass der Fundplatz in römischer Zeit inmitten einer stark vom Wald und dem Fluss Lorze geprägten Landschaft lag. In unmittelbarer Nähe können weder eine Siedlung noch einzelne Wohnbauten gelegen haben. Die demnach nur gewerblich und sakral genutzten Anlagen standen an einem Bach, der vermutlich mit jenem Bach identisch ist, der noch heute das Groppenmoos entwässert und bei Cham-Hagendorn in die Lorze mündet (s. Abb. 2.4/1). Der antike Bach führte wiederholt Hochwasser ─ insgesamt sind fünf grössere Überschwemmungsphasen auszumachen (Kap. 2.2; 2.4). Wohl anlässlich eines Seehochstandes durch ein Überschwappen der Lorze in den Bach ausgelöst, müssen diese Überschwemmungen eine enorme Gewalt entwickelt haben, der die einzelnen Anlagen zum Opfer fielen. Wie die Untersuchung der Siedlungslandschaft römischer Zeit rund um den Zugersee wahrscheinlich macht (Kap. 6 mit Abb. 6.2/2), dürften die Anlagen von Cham-Hagendorn zu einer in Cham-Heiligkreuz vermuteten Villa gehören, einem von fünf grösseren Landgütern in diesem Gebiet. Hinweise auf Vorgängeranlagen fehlen, mit denen die vereinzelten Funde des 1. Jh. n. Chr. (Kap. 4.5) in Verbindung gebracht werden könnten. Diese dürften eher von einer der Überschwemmungen bachaufwärts weggerissen und nach Cham-Hagendorn eingeschwemmt worden sein. Die Nutzung des Fundplatzes (Horizont 1a; s. Beil. 6) setzte um 170 n. Chr. mit einer Schmiedewerkstatt ein (Kap. 2.5.1). Der Fundanfall, insbesondere die Schmiedeschlacken (Kap. 3.9) belegen, dass hier nur hin und wieder Geräte hergestellt und repariert wurden (Kap. 5.2). Diese Werkstatt war vermutlich schon aufgelassen und dem Verfall preisgegeben, als man 200 n. Chr. (Kap. 4.2.4) auf einer Insel zwischen dem Bach und einem Lorzearm ein Heiligtum errichtete (Kap. 5.3). Beleg für den sakralen Status dieser Insel ist in erster Linie mindestens ein eigens gepflanzter Pfirsichbaum, nachgewiesen mit Pollen, einem Holz und über 400 Pfirsichsteinen (Kap. 3.11). Die im Bach verlaufende Grenze zwischen dem sakralen Platz und der profanen Umgebung markierte man zusätzlich mit einer Pfahlreihe (Kap. 2.5.3). In diese war ein schmaler Langbau integriert (Kap. 2.5.2), der an die oft an Temenosmauern antiker Heiligtümer angebauten Portiken erinnert und wohl auch die gleiche Funktion wie diese gehabt hatte, nämlich das Aufbewahren von Weihegaben und Kultgerät (Kap. 5.3). Das reiche Fundmaterial, das sich in den Schichten der ersten Überschwemmung fand (s. Abb. 5./5), die um 205/210 n. Chr. dieses Heiligtum zerstört hatte, insbesondere die zahlreiche Keramik (Kap. 3.2.4), und die zum Teil auffallend wertvollen Kleinfunde (Kap. 3.3.3), dürften zum grössten Teil einst in diesem Langbau untergebracht gewesen sein. Ein als Glockenklöppel interpretiertes, stratifiziertes Objekt spricht dafür, dass die fünf grossen, 1944/1945 als Stapel aufgefundenen Eisenglocken vielleicht auch dem Heiligtum zuzuweisen sind (Kap. 3.4). In diesen Kontext passen zudem die überdurchschnittlich häufig kalzinierten Tierknochen (Kap. 3.10). Nach der Überschwemmung befestigte man für 215 n. Chr. (Kap. 4.2.4) das unterspülte Bachufer mit einer Uferverbauung (Kap. 2.6.1). Mit dem Bau eines weiteren, im Bach stehenden Langbaus (Kap. 2.6.2) stellte man 218 n. Chr. das Heiligtum auf der Insel in ähnlicher Form wieder her (Horizont 1b; s. Beil. 7). Von der Pfahlreihe, die wiederum die sakrale Insel von der profanen Umgebung abgrenzte, blieben indes nur wenige Pfähle erhalten. Dennoch ist der sakrale Charakter der Anlage gesichert. Ausser dem immer noch blühenden Pfirsichbaum ist es ein vor dem Langbau aufgestelltes Ensemble von mindestens 23 Terrakottafigurinen (s. Abb. 3.6/1), elf Veneres, zehn Matres, einem Jugendlichen in Kapuzenmantel und einem kindlichen Risus (Kap. 3.6; s. auch Kap. 2.6.3). In den Sedimenten der zweiten Überschwemmung, der diese Anlage um 225/230 n. Chr. zum Opfer gefallen war, fanden sich wiederum zahlreiche Keramikgefässe (Kap. 3.2.4) und zum Teil wertvolle Kleinfunde wie eine Glasperle mit Goldfolie (Kap. 3.8.2) und eine Fibel aus Silber (Kap. 3.3.3), die wohl ursprünglich im Langbau untergebracht waren (Kap. 5.3.2 mit Abb. 5/7). Weitere Funde mit sicherem oder möglichem sakralem Charakter finden sich unter den 1944/1945 geborgenen Funden (s. Abb. 5/8), etwa ein silberner Fingerring mit Merkurinschrift, ein silberner Lunula-Anhänger, eine silberne Kasserolle (Kap. 3.3.3), eine Glasflasche mit Schlangenfadenauflage (Kap. 3.8.2) und einige Bergkristalle (Kap. 3.8.4). Im Bereich der Terrakotten kamen ferner mehrere Münzen (Kap. 3.7) zum Vorschein, die vielleicht dort niedergelegt worden waren. Nach der zweiten Überschwemmung errichtete man um 231 n. Chr. am Bach eine Wassermühle (Horizont 2; Kap. 2.7; Beil. 8; Abb. 2.7/49). Ob das Heiligtum auf der Insel wieder aufgebaut oder aufgelassen wurde, muss mangels Hinweisen offen bleiben. Für den abgehobenen Zuflusskanal der Wassermühle verwendete man mehrere stehen gebliebene Pfähle der vorangegangenen Anlagen der Horizonte 1a und 1b. Obwohl die Wassermühle den 28 jährlichen Überschwemmungshorizonten (Kap. 2.2) und den Funden (Kap. 4.3.2; 4.4.4; 45) zufolge nur bis um 260 n. Chr., während gut einer Generation, bestand, musste sie mindestens zweimal erneuert werden – nachgewiesen sind drei Wasserräder, drei Mühlsteinpaare und vermutlich drei Podeste, auf denen jeweils das Mahlwerk ruhte. Grund für diese Umbauten war wohl der weiche, instabile Untergrund, der zu Verschiebungen geführt hatte, so dass das Zusammenspiel von Wellbaum bzw. Sternnabe und Übersetzungsrad nicht mehr funktionierte und das ganze System zerbrach. Die Analyse von Pollen aus dem Gehhorizont hat als Mahlgut Getreide vom Weizentyp nachgewiesen (Kap. 3.11.4). Das Abzeichen eines Benefiziariers (Kap. 3.3.2 mit Abb. 3.3/23,B71) könnte dafür sprechen, dass das verarbeitete Getreide zumindest zum Teil für das römische Militär bestimmt war (s. auch Kap. 6.2.3). Ein im Horizont 2 gefundener Schreibgriffel und weitere stili sowie eine Waage für das Wägen bis zu 35-40 kg schweren Waren aus dem Fundbestand von 1944/1945 könnten davon zeugen, dass das Getreide zu wägen und zu registrieren war (Kap. 3.4.2). Kurz nach 260 n. Chr. fiel die Wassermühle einem weiteren Hochwasser zum Opfer. Für den folgenden Horizont 3 (Beil. 9) brachte man einen Kiesboden ein und errichtete ein kleines Gebäude (Kap. 2.8). Hier war wohl wiederum eine Schmiede untergebracht, wie die zahlreichen Kalottenschlacken belegen (Kap. 3.9), die im Umfeld der kleinen Baus zum Vorschein kamen. Aufgrund der Funde (Kap. 4.4.4; 4.5) kann diese Werkstatt nur kurze Zeit bestanden haben, höchstens bis um 270 n. Chr., bevor sie einem weiteren Hochwasser zum Opfer fiel. Von der jüngsten Anlage, die wohl noch in römische Zeit datiert (Horizont 4; Beil. 10), war lediglich eine Konstruktion aus grossen Steinplatten zu fassen (Kap. 2.9.1). Wozu sie diente, muss offen bleiben. Auch der geringe Fundanfall spricht dafür, dass die Nutzung des Platzes, zumindest für die römische Zeit, allmählich ein Ende fand (Kap. 4.5). Zu den jüngsten Strukturen gehören mehrere Gruben (Kap. 2.9.2), die vielleicht der Lehmentnahme dienten. Mangels Funden bleibt ihre Datierung indes ungewiss. Insbesondere wissen wir nicht, ob sie noch in römische Zeit datieren oder jünger sind. Spätestens mit der fünften Überschwemmung, die zur endgültigen Verlandung führte und wohl schon in die frühe Neuzeit zu setzen ist, wurde der Platz aufgelassen und erst mit dem Bau der bestehenden Fensterfabrik Baumgartner wieder besetzt.

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In 1884, Lorenzen proposed the formula MgAI2SiO6 for his new mineral kornerupine from Fiskenæsset and did not suspect it to contain boron. Lacroix and de Gramont (1919) reported boron in Fiskenæsset kornerupine, while Herd (1973) found none. New analyses (ion microprobe mass analyser and spectrophotometric) of kornerupine in three specimens from the type locality, including the specimens analysed by Lorenzen and Herd, indicate the presence of boron in all three, in amounts ranging from 0.50 to 1.44 wt.% B203, e.g. (Li0.04 Na0.01 Ca0.01) (Mg3.49 Mn0.01 Fe0.17 Ti0.01 Al5.64)Σ9.30 (Si3.67 Al1.02 B0.31)Σ5 O21 (OH0.99 F0.01) for Lorenzen's specimen. Textures and chemical compositions suggest that kornerupine crystallized in equilibrium in the following assemblages, all with anorthite (An 92-95) and phlogopite (XFe = atomic Fe/(Fe + Mg) = 0.028-0.035): (1) kornerupine (0.045)-gedrite (0.067); (2) kornerupine (0.038-0.050)-sapphirine (0.032-0.035); and (3) kornerupine (0.050)-hornblende. Fluorine contents of kornerupine range from 0.01 to 0.06%, of phlogopite, from 0.09 to 0.10%. In the first assemblage, sapphirine (0.040) and corundum are enclosed in radiating bundles of kornerupine; additionally sapphirine, corundum, and/or gedrite occur with chlorite and pinite (cordierite?) as breakdown products of kornerupine. Kornerupine may have formed by reactions such as: gedrite + sapphirine + corundum + B203 (in solution) + H20 = kornerupine + anorthite + Na-phlogopite under conditions of the granulite facies. Boron for kornerupine formation was most likely remobilized by hydrous fluids from metasedimentary rocks occurring along the upper contact of the Fiskenæsset gabbro-anorthosite complex with amphibolite.

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K-feldspar (Kfs) from the Chain of Ponds Pluton (CPP) is the archetypal reference material, on which thermochronological modeling of Ar diffusion in discrete “domains” was founded. We re-examine the CPP Kfs using cathodoluminescence and back-scattered electron imaging, transmission electron microscopy, and electron probe microanalysis. 40Ar/39Ar stepwise heating experiments on different sieve fractions, and on handpicked and unpicked aliquots, are compared. Our results reproduce the staircase-shaped age spectrum and the Arrhenius trajectory of the literature sample, confirming that samples collected from the same locality have an identical Ar isotope record. Even the most pristine-looking Kfs from the CPP contains successive generations of secondary, metasomatic/retrograde mineral replacements that post-date magmatic crystallization. These chemically and chronologically distinct phases are responsible for its staircase-shaped age spectra, which are modified by handpicking. While genuine within-grain diffusion gradients are not ruled out by these data, this study demonstrates that the most important control on staircase-shaped age spectra is the simultaneous presence of heterochemical, diachronous post-magmatic mineral growth. At least five distinct mineral species were identified in the Kfs separate, three of which can be traced to external fluids interacting with the CPP in a chemically open system. Sieve fractions have size-shifted Arrhenius trajectories, negating the existence of the smallest “diffusion domains”. Heterochemical phases also play an important role in producing non-linear trajectories. In vacuo degassing rates recovered from Arrhenius plots are neither related to true Fick’s Law diffusion nor to the staircase shape of the age spectra. The CPP Kfs used to define the "diffusion domain" model demonstrates the predominance of metasomatic alteration by hydrothermal fluids and recrystallization in establishing the natural Ar distribution amongst different coexisting phases that gives rise to the staircase-shaped age spectrum. Microbeam imaging of textures is as essential for 40Ar-39Ar hygrochronology as it is for U-Pb geochronology.

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Hellas basin is a large impact basin situated in the southern highlands of Mars. The north-western part of the basin has the lowest elevation (-7.5 km) on the planet and contains a possibly unique terrain type, which we informally call “banded terrain”. The banded terrain is made up of smooth-looking banded deposits that display signs of viscous behavior and a paucity of superimposed impact craters. In this study, we use newly acquired high spatial resolution images from the High Resolution Imaging Science Experiment (HiRISE) in addition to existing datasets to characterize the geomorphology, the morphometry and the architecture of the banded terrain. The banded terrain is generally confined to the NW edge of the Alpheus Colles plateau. The individual bands are ~3–15 km-long, ~0.3 km-wide and are separated by narrow inter-band depressions, which are ~65 m-wide and ~10 m-deep. The bands display several morphologies that vary from linear to concentric forms. Morphometric analysis reveals that the slopes along a given linear or lobate band ranges from 0.5° to 15° (average~6°), whereas the concentric bands are located on flatter terrain (average slope~2–3°). Crater-size frequency analysis yields an Amazonian-Hesperian boundary crater retention age for the terrain (~3 Gyr), which together, with the presence of very few degraded craters, either implies a recent emplacement, resurfacing, or intense erosion. The apparent sensitivity to local topography and preference for concentrating in localized depressions is compatible with deformation as a viscous fluid. In addition, the bands display clear signs of degradation and slumping at their margins along with a suite of other features that include fractured mounds, polygonal cracks at variable size-scales, and knobby/hummocky textures. Together, these features suggest an ice-rich composition for at least the upper layers of the terrain, which is currently being heavily modified through loss of ice and intense weathering, possibly by wind.

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The chemical compositions and crystal structures of Mn3+-containing minerals from the epidote group in Greenland rocks are investigated and described in detail. They occur in hydrothermally altered Archaean mafic sequences within the gneissic complex of the North Atlantic craton of West Greenland. The Mn-containing minerals have a characteristic red to pink colour. A detailed microchemical study shows a significant inter- and intra-sample variation in Mn content. The samples from different parageneses can be classified as Mn-bearing epidote and Mn-bearing clinozoisite. The intra-sample variation in the content of Al, Fe and Mn is on a very fine scale, but still allows for identification of a negative correlation between Mn and Fe. Textures indicate different stages of growth. Crystal chemical data are compared with literature data and illustrate the basic systematic differences between the influence of Fe and Mn on the crystal structure of the epidote group minerals.

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We present a novel algorithm to reconstruct high-quality images from sampled pixels and gradients in gradient-domain rendering. Our approach extends screened Poisson reconstruction by adding additional regularization constraints. Our key idea is to exploit local patches in feature images, which contain per-pixels normals, textures, position, etc., to formulate these constraints. We describe a GPU implementation of our approach that runs on the order of seconds on megapixel images. We demonstrate a significant improvement in image quality over screened Poisson reconstruction under the L1 norm. Because we adapt the regularization constraints to the noise level in the input, our algorithm is consistent and converges to the ground truth.

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The Zr-in-rutile geothermometer is potentially a widely applicable tool to estimate peak metamorphic temperatures in rocks from diverse geological settings. In order to evaluate its usefulness and reliability to record and preserve high temperatures in granulite facies rocks, rutile from UHT rocks was investigated to assess different mechanisms of Zr (re-)distribution following cooling from high temperature. Granulite facies paragneisses from the lowermost part of the Ivrea Zone, Italy, incorporated as thin sheets into the extensive basaltic body of the Mafic Complex were selected for this study. The results show that Zr-in-rutile thermometry, if properly applied, is well suited to identify and study UHT terranes as it preserves a record of temperatures up to 1190 °C, although the thermometer is susceptible to partial post-peak metamorphic resetting by Zr diffusion. Texturally homogeneous rutile grains preserve Zr concentrations corresponding to temperatures of prograde rutile growth. Diverse rutile textures and relationships between some rutile host grains and included or adjacent Zr-bearing phases bear testimony to varying mechanisms of partial redistribution and resetting of Zr in rutile during cooling and link Zr-in-rutile temperatures to different steps of the metamorphic evolution. Rutile grains that equilibrated their Zr concentrations at temperatures above 1070 °C (i.e. 1.1 wt% Zr) could not retain all Zr in the rutile structure during cooling and exsolved baddeleyite (ZrO2). By subsequent reaction of baddeleyite exsolution lamellae with SiO2, zircon needles formed before the system finally closed at 650–700 °C without significant net loss of Zr from the whole host rutile grain. By reintegration of zircon exsolution needles, peak metamorphic temperatures of up to 1190 °C are derived for the studied rocks, which demonstrates the suitability of this solution thermometer to record UHT conditions and also confirms the extraordinary geological setting of the lowermost part of the Ivrea Zone.

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Images of comet 67P/Churyumov-Gerasimenko acquired by the OSIRIS (Optical, Spectroscopic and Infrared Remote Imaging System) imaging system onboard the European Space Agency's Rosetta spacecraft at scales of better than 0.8 meter per pixel show a wide variety of different structures and textures. The data show the importance of airfall, surface dust transport, mass wasting, and insolation weathering for cometary surface evolution, and they offer some support for subsurface fluidization models and mass loss through the ejection of large chunks of material.

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The 16 samples of Deep Sea Drilling Project (DSDP) Leg 89 basalts that we analyzed for whole rock major and trace elements and for mineralogic compositions are identical to some of the basalts recovered during Leg 61. Leg 89 samples are mostly olivine-plagioclase-clinopyroxene sparsely phyric basalts and exhibit a wide variety of textures. These basalts have lower TiO2 at a given Mg/(Mg+Fe2+)*100 than MORB (midocean ridge basalt). We recognize three major chemical types of basalts in the Nauru Basin. We believe that different degrees of partial melting, modified by fractional crystallization and possibly by magma mixing at shallow depths, can explain the chemical differences among the three groups. This petrogenetic model is consistent with the observed downhole chemical-chronostratigraphic relations of the samples. New 87Sr/86Sr and U3Nd/144Nd analyses of basalt samples from DSDP Site 462 indicate that the Nauru Basin igneous complex is within the Sr-Nd isotopic range of ocean island basalt. Thus the Nauru Basin igneous complex resembles MORB in many aspects of its chemistry, morphology, and secondary alteration patterns (Larson, Schlanger, et al., 1981), but not in its isotopic characteristics. If it were not for the unambiguous evidence that the Nauru Basin complex was erupted off-ridge, the complex could easily be interpreted as normal oceanic layer 2. For this reason, we speculate that the Nauru Basin igneous complex was produced in an oceanic riftlike environment when multiple, fast-propagating rifts were formed during the fast seafloor spreading episode in the Cretaceous.

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Grain-size analyses by sieve and Sedigraph are presented for 115 samples of core from CRP-3, 12 km off the coast of south Victoria Land. The data provide a useful check on visual core descriptions. The geographic setting for the strata sampled, some 790 m of early Oligocene nearshore marine sediments with a persistent glacial influence, is reviewed, and sediment textures interpreted in that context. Sand textures from the CRP-3 samples in the lower part of the core suggest that deposition was initially primarily wave-dominated, but that at times the influence of the waves was over-ridden by episodes of rapid sedimentation. Sedimentary cycles, recognised in the visual description of the core above 485 mbsf, show an increasing proportion of mudstone in the middle of each cycle above 330 mbsf that is interpreted to record periodic sedimentation in deeper water. Sandstone textures in the lower and upper parts of each cycle are interpreted to record departure from and return to shoreface deposition with changes in sea level. Mudstone textures above 176 mbsf indicate sedimentation below wave base. Many of the textures in both sand and mud samples show the coarse 'tail' characteristic of ice-rafted debris, but others do not, indicating ice-free periods. Many sandstones below c. 200 mbsf have virtually no silt, but significant amounts of clay (6 to 17%) that is thought to be of post-depositional origin.

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Collisional and post-collisional volcanic rocks in the Ulubey (Ordu) area at the western edge of the Eastern Pontide Tertiary Volcanic Province (EPTVP) in NE Turkey are divided into four suites; Middle Eocene (49.4-44.6 Ma) aged Andesite-Trachyandesite (AT), Trachyandesite-Trachydacite-Rhyolite (TTR), Trachydacite-Dacite (TD) suites, and Middle Miocene (15.1 Ma) aged Trachybasalt (TB) suite. Local stratigraphy in the Ulubey area starts with shallow marine environment sediments of the Paleocene-Eocene time and then continues extensively with sub-aerial andesitic to rhyolitic and rare basaltic volcanism during Eocene and Miocene time, respectively. Petrographically, the volcanic rocks are composed primarily of andesites/trachyandesites, with minor trachydacites/rhyolites, basalts/trachybasalts and pyroclastics, and show porphyric, hyalo-microlitic porphyric and rarely glomeroporphyric, intersertal, intergranular, fluidal and sieve textures. The Ulubey (Ordu) volcanic rocks indicate magma evolution from tholeiitic-alkaline to calc-alkaline with medium-K contents. Primitive mantle normalized trace element and chondrite normalized rare earth element (REE) patterns show that the volcanic rocks have moderate light rare earth element (LREE)/heavy rare earth element (HREE) ratios relative to E-Type MORB and depletion in Nb, Ta and Ti. High Th/Yb ratios indicate parental magma(s) derived from an enriched source formed by mixing of slab and asthenospheric melts previously modified by fluids and sediments from a subduction zone. All of the volcanic rocks share similar incompatible element ratios (e.g., La/Sm, Zr/Nb, La/Nb) and chondrite-normalized REE patterns, indicating that the basic to acidic rocks originated from the same source. The volcanic rocks were produced by the slab dehydration-induced melting of an existing metasomatized mantle source, and the fluids from the slab dehydration introduced significant large ion lithophile element (LILE) and LREE to the source, masking its inherent HFSE-enriched characteristics. The initial 87Sr/86Sr (0.7044-0.7050) and eNd (-0.3 to +3.4) ratios of the volcanics suggest that they originated from an enriched lithospheric mantle source with low Sm/Nd ratios. Integration of the geochemical, petrological and isotopical with regional and local geological data suggest that the Tertiary volcanic rocks from the Ulubey (Ordu) area were derived from an enriched mantle, which had been previously metasomatized by fluids derived from subducted slab during Eocene to Miocene in collisional and post-collisional extension-related geodynamic setting following Late Mesozoic continental collision between the Eurasian plate and the Tauride-Anatolide platform.