Paleoambiente da formação mosquito e a implantação do sistema desértico úmido da formação corda, jurássico superior, Centro-Oeste da Bacia do Parnaíba

O Mesozóico foi marcado por mudanças geológicas significativas, decorrentes de soerguimentos resultante da orogenia Gonduanide, que possibilitou a implantação de sistemas desérticos concomitantemente com expressivos eventos magmáticos. Na Bacia do Parnaíba, Nordeste do Brasil, estes eventos estão registrados nas unidades siliciclásticas do Triássico, os arenitos da Formação Sambaíba, representadas pelos derrames basálticos e arenitos fluviais e eólicos subordinados da Formação Mosquito e pelos arenitos flúvio-eólicos da Formação Corda. O estudo de fácies e estratigráfico realizado em afloramentos e testemunhos de sondagem na região entre Formosa da Serra Negra e Montes Altos, Estado do Maranhão, possibilitou reconstituir o paleoambiente do topo da Formação Mosquito e da Formação Corda, e inferir condições paleoclimáticas para a porção centro-oeste da Bacia do Parnaíba durante o Jurássico. Foram identificadas vinte fácies sedimentares agrupadas em cinco associações de fácies (AF) representativas de uma planície vulcânica com depósitos fluviais esporádicos e arenitos eólicos subordinados (AF1-Formação Mosquito), sucedida pela instalação de um sistema desértico úmido (AF2-AF5; Formação Corda). A planície vulcânica (AF1) constitui derrames basálticos intercalados com arenitos finos a grossos (arenitos intertrap) compostos por grãos arredondados a subangulosos de quartzo, feldspatos e fragmentos de vidro vulcânico. Os arenitos apresentam estratificações plano-paralela e cruzada de baixo ângulo, preenchendo geometria de canal ou em corpos tabulares. Depósitos de canal fluvial entrelaçado (AF2) consistem em conglomerados polimíticos, com grânulos e seixos subarredondados a angulosos de basalto, e arenitos grossos com estratificação cruzada acanalada e acamamento maciço. Os lençóis arenosos (AF3) foram divididos em dois elementos arquiteturais (EA), o primeiro (EA1) consistem em arenitos finos a muitos com geometria tabular e estruturas de deformação, o segundo (EA2) é composto por arenito fino a grosso com estratificação cruzada acanalada e laminação cruzada cavalgante, gutter cast de pequeno porte. O campo de dunas (AF4) foi subdividido em dois conjuntos de fácies (C), o primeiro (CI) é caracterizado por arenitos com estratificações cruzadas tabular e tangencial de pequeno a médio porte, estratificação planoparalela e laminação cruzada cavalgante transladante subcrítica. O segundo (CII) consiste de arenitos finos a médios, moderadamente selecionados, laminação ondulada e estruturas de adesão e gretas de contração com rip-up clast, curled mud flakes, forma ciclos de raseamento centimétricos, com topo marcado por horizontes mosqueados, ricos em óxido/hidróxido de ferro, bioturbações e gretas de contração, interpretados como depósitos de interdunas úmidas. Os lobos de suspensão (AF5) consistem em arenitos finos intercalados com pelitos e arenito/pelito com estratificação cruzada complexa. A abundância de esmectita na AF4 aponta para condições de clima semiárido. No Jurássico, a região centro-oeste da Bacia do Parnaíba, foi submetida a movimentos distensivos com recorrência de derrames básicos advindos de fissuras na crosta. Durante os intervalos de aquiescência sedimentos de rios efêmeros preenchiam depressões ou espraiavam-se na planície vulcânica. O final da atividade magmática foi sucedido pela implantação do desérto Corda com campo de dunas e canais fluviais efêmeros (wadi) que retrabalharam parte da planície vulcânica e esporadicamente invadiam os lençóis arenosos. Comparado aos ergs do Permo-Triássico (Formação Sambaíba), o deserto Jurássico da Formação Corda foi mais úmido e menos extenso precedendo os sistemas fluviais e costeiros de clima mais ameno do Cretáceo da Bacia do Parnaíba.

Geologia, petrografia e geoquímica das rochas vulcânicas Uatumã na área sul de São Félix do Xingu (PA), Província Carajás

As rochas vulcânicas da área sul de São Félix do Xingu, estado do Pará, estão inseridas no contexto geológico da província geocronológica Amazônia Central, sudeste do cráton Amazônico. Estas rochas são dominantemente relacionadas à Formação Sobreiro e, subordinadamente, à Formação Santa Rosa, ambas pertencentes ao Grupo Uatumã de idade Paleoproterozoica. A Formação Sobreiro apresenta três fácies: fácies de fluxo de lavas subaérea de composição subalcalina; fácies de fluxo de lavas subaérea de composição calcioalcalina a shoshonítica; fácies vulcanoclástica subaérea. As rochas da Formação Santa Rosa são enquadradas em uma única fácies denominada fácies de fluxo de lavas subaérea. Na Formação Sobreiro são encontrados andesitos basálticos, andesitos, traquiandesitos, traquitos, tufos de cristais félsicos, lapili-tufos e brechas polimíticas. Os litotipos da Formação Santa Rosa são riolitos. Os dados geoquímicos mostram que os conteúdos de SiO2 das rochas da Formação Sobreiro variam de 52,14 a 69,21% e as razões K2O/Na2O de 0,16 a 1,62. Por outro lado, os vulcanitos da Formação São Rosa formam uma série evoluída com teores de SiO2 entre 72,27 e 77,14% e razões K2O/Na2O entre 1,50 e 2,12. A Formação Sobreiro tem caráter essencialmente calcioalcalino, discretamente transicional de calcioalcalino a shoshonítico, composição metaluminosa a fracamente peraluminosa e assinatura tectônica de ambiente de arco vulcânico. A Formação Santa Rosa apresenta composição peraluminosa a fracamente metaluminosa, assinatura tipo A e afinidade tectônica intraplacas. As rochas vulcânicas da área sul apresentam perfeita correlação petrográfica, geoquímica e tectônica com os vulcanitos da área oeste/sudoeste de São Félix do Xingu.

Química mineral do vulcano-plutonismo paleoproterozoico da região de São Félix do Xingu (PA), Cráton Amazônico

As formações Sobreiro e Santa Rosa são resultado de intensas atividades vulcânicas paleoproterozoicas na região de São Félix do Xingu (PA), SE do Cráton Amazônico. A Formação Sobreiro é composta por rochas de fácies de fluxo de lava andesítica, com dacito e riodacito subordinados, além de rochas que compõem a fácies vulcanoclástica, caracterizadas por tufo, lapilli-tufo e brecha polimítica maciça. Essas rochas exibem fenocristais de clinopiroxênio, anfibólio e plagioclásio em uma matriz microlítica ou traquítica. O clinopiroxênio é classificado predominantemente como augita, com diopsídio subordinado, e apresenta caracterísiticas geoquímicas de minerais gerados em rochas de arco magmático. O anfibólio, representado pela magnesiohastingsita, foi formado sob condições oxidantes e apresenta texturas de desequilíbrio, como bordas de oxidação vinculadas à degaseificação por alívio de pressão. As rochas da Formação Santa Rosa foram extravasadas em grandes fissuras crustais de direção NE-SW, têm características de evolução polifásica e compõem uma fácies de fluxo de lava riolítica e riodacítica e uma fácies vulcanoclástica de ignimbritos, lapilli-tufos, tufos de cristais félsicos e brechas polimíticas maciças. Diques métricos e stocks de pórfiros graníticos e granitoides equigranulares completam essa suíte. Fenocristais de feldspato potássico, plagioclásio e quartzo dispersos em matriz de quartzo e feldspato potássico intercrescidos ocorrem nessas rochas. Por meio de análises químicas pontuais dos fenocristais em microssonda eletrônica, foram estimadas as condições de pressão e temperatura de sua formação, sendo que o clinopiroxênio das rochas intermediárias da Formação Sobreiro indica profundidade de formação variável entre 58 e 17,5 km (17,5 - 4,5 kbar), a temperaturas entre 1.294 e 1.082 ºC, enquanto o anfibólio cristalizou-se entre 28 e 15 km (7,8 - 4,1 kbar), o que sugere uma evolução polibárica. Assim, propõe-se um modelo de geração de magma basáltico hidratado com base na fusão parcial de cunha mantélica e no acúmulo na crosta inferior em uma zona quente, a partir da qual os magmas andesíticos e dacíticos são formados pela assimilação de crosta continental e cristalização fracionada.

Reconstruction of Etna recent flank eruptions for assessing diversion barrier project

The thesis contributed to the volcanic hazard assessment through the reconstruction of some historical flank eruptions of Etna in order to obtain quantitative data (volumes, effusion rates, etc.) for characterizing the recent effusive activity, quantifying the impact on the territory and defining mitigation actions for reducing the volcanic risk as for example containment barriers. The reconstruction was based on a quantitative approach using data extracted from aerial photographs and topographic maps. The approach allows to obtain the temporal evolution of the lava flow field and estimating the Time Average Discharge Rate (TADR) by dividing the volume emplaced over a given time interval for the corresponding duration. The analysis concerned the 2001, 1981 and 1928 Etna eruptions. The choice of these events is linked to their impact on inhabited areas. The results of the analysis showed an extraordinarily high effusion rate for the 1981 and 1928 eruptions (over 600 m^3/s), unusual for Etna eruptions. For the 1981 Etna eruption an eruptive model was proposed to explain the high discharge rate. The obtained TADRs were used as input data for simulations of the propagation of the lava flows for evaluating different scenarios of volcanic hazard and analyse different mitigation actions against lava flow invasion. It was experienced how numerical simulations could be adopted for evaluating the effectiveness of barrier construction and for supporting their optimal design. In particular, the gabions were proposed as an improvement for the construction of barriers with respect to the earthen barriers. The gabion barriers allow to create easily modular structures reducing the handled volumes and the intervention time. For evaluating operational constrain an experimental test was carried out to test the filling of the gabions with volcanic rock and evaluating their deformation during transport and placement.

Petrologisch-geochemische Charakterisierung quartärer Laven der Eifel als Grundlage zur archäometrischen Herkunftsbestimmung römischer Mühlsteine

Lava aus der quartären Vulkanregion der Eifel wurde in römischer Zeit großmaßstäblich abgebaut, um daraus Mühlsteine hoher Qualität herzustellen, die in großen Mengen in weite Teile des Römischen Reiches exportiert wurden. Somit erweisen sich diese Mühlsteine als ideale Indikatoren für Handelsgebiete und –wege dieser Zeit. Für eine erfolgreiche Herkunftsanalyse von Fundstücken ist eine genaue Charakterisierung der infrage kommenden Rohstoffe die unbedingte Voraussetzung. Aus diesem Grund konzentriert sich diese Arbeit auf die geochemische Definition der 16 bekannten römischen „Basalt“-Abbaustellen in den Vulkanfeldern der Ost- und Westeifel, mit dem vorrangigen Ziel, eine möglichste eindeutige Charakterisierung der einzelnen Abbaustellen zu erreichen. Auf dieser Basis wird eine Vorgehensweise zur folgenden Provenienzanalyse der Mühlsteine entwickelt. Um die geochemische Variabilität der Laven zu erfassen wurden die Abbaustellen großflächig beprobt. Die Proben wurden zunächst petrographisch bestimmt und der Phasenbestand mittels Röntgendiffraktometrie (XRD) untersucht. Die Haupt- und Spurenelement-Zusammensetzung wurde anhand von Röntgenfluoreszenzanalysen und Laser-Massenspektrometrie mit induktiv gekoppeltem Plasma (LA-ICP-MS) ermittelt, die Sr-Nd-Pb-Isotopie ausgewählter Proben mittels Thermo-Ionen-Massenspektrometrie (TIMS). Es zeigte sich, dass auf Grundlage der Haupt- und Spurenelementzusammensetzung, gemessen mit RFA, eine Abgrenzung der Abbaustellen zueinander mittels einer Kombination aus geochemischer Diskriminierung mit Cluster- und Diskriminanzanalysen gelingt. Die anschließende Provenienzanalyse der Mühlsteinfundstücke erfolgt analog zur Charakterisierung der Abbaustellen. Im ersten Schritt wird eine geochemische Zuordnung des Fundstücks vorgenommen, um zu überprüfen, ob eine Eifeler Herkunft überhaupt in Frage kommt. Lässt der geochemische Vergleich mit den Referenzdaten aus dem Gelände eine Eifeler Herkunft zu, kommt im zweiten Schritt die Clusteranalyse zum Einsatz. Hier wird auf multivariater Ebene geprüft, ob das Fundstück einer Eifeler Abbaustelle oder einem Cluster von Eifeler Abbaustellen zugeordnet werden kann. Bei einer positiven Zuordnung wird ergänzend als dritter Schritt die Diskriminanzanalyse angewendet, anhand der das Mühlstein-Fundstück einer Abbaustelle mit einer bestimmten Wahrscheinlichkeit zugewiesen wird. Bei 68 analysierten Mühlsteinen aus verschiedenen Regionen Mitteleuropas konnte so für 49 Fundstücke eine Eifeler Provenienz festgestellt werden. Alle römischen Eifeler Mühlsteine entstammen dem Bellerberg bei Mayen, ein mittelalterliches Stück aus dem Niedermendiger Lavastrom. Die Zuordnung der übrigen 19 Mühlsteine zu anderen möglichen Abbaugebieten erfolgt anhand geochemischer Daten aus der Literatur. Aufgrund der unzureichenden Datenlage sind im Falle dieser Proben jedoch im Gegensatz zur Lavastrom-genauen Zuordnung der Eifeler Mühlen lediglich Vermutungen über die Herkunftsregionen möglich. Damit zeigt sich, dass eine ausführliche Referenzdatenbank der in Frage kommenden Rohstoffe die erforderliche Basis für erfolgreiche Provenienzanalysen ist. Die Möglichkeit der genauen Zuordnungen von Mühlsteinen zu den Eifeler Abbaustellen belegt, dass die Verbindung von geochemischer Auswertung mit Cluster- und Diskriminanzanalysen ein hilfreiches Verfahren zur Provenienzanalyse darstellt.

Paleoenvironment and Paleoecology of a Late Paleocene High-Latitude Terrestrial Succession, Arkose Ridge Formation at Box Canyon, Southern Talkeetna Mountains, Alaska

Paleogene sedimentary rocks of the Arkose Ridge Formation (Talkeetna Mountains, Alaska) preserve a record of a fluvial-lacustrine depositional environment and its forested ecosystem in an active basin among the convergent margin tectonic processes that shaped southern Alaska. An -800 m measured succession at Box Canyon indicates braid-plain deposition with predominantly gravelly deposits low in the exposure to sandy and muddy facies associations below an overlying lava flow sequence. U-Pb geochronology on zircons from a tuff and a sandstone within the measured section, as well as an Ar/Ar date from the overlying lava constrain the age of the sedimentary succession to between similar to 59 Ma and 48 Ma Fossil plant remains occur throughout the Arkose Ridge Formation as poorly-preserved coalified woody debris and fragmentary leaf impressions. At Box Canyon, however, a thin la-custrine depositional lens of rhythmically laminated mudrocks yielded fish fossils and a well-preserved floral assemblage including foliage and reproductive organs representing conifers, sphenopsids, monocots, and dicots. Leaf physiognomic methods to estimate paleoclimate were applied to the dicot leaf collection and indicate warm temperate paleotemperatures (-11-15 +/- -4 degrees C MAT) and elevated paleoprecipitation (-120 cm/yr MAP) estimates as compared to modem conditions; results that are parallel with previously published estimates from the partly coeval Chickaloon Formation deposited in more distal depositional environments in the same basin. The low abundance of leaf herbivory in the Box Canyon dicot assemblage (-9% of leaves damaged) is also similar to the results from assemblages in the meander-plain depositional systems of the Chickaloon. This new suite of data informs models of the tectonostratigraphic evolution of southern Alaska and the developing understanding of terrestrial paleoecology and paleoclimate at high latitudes during the Late Paleocene-Early Eocene greenhouse climate phase. (c) 2014 Elsevier B.V. All rights reserved.

Dynamics and kinematics of eruptive activity at Fuego volcano, Guatemala 2005-2009

Volcanoes are the surficial expressions of complex pathways that vent magma and gasses generated deep in the Earth. Geophysical data record at least the partial history of magma and gas movement in the conduit and venting to the atmosphere. This work focuses on developing a more comprehensive understanding of explosive degassing at Fuego volcano, Guatemala through observations and analysis of geophysical data collected in 2005 – 2009. A pattern of eruptive activity was observed during 2005 – 2007 and quantified with seismic and infrasound, satellite thermal and gas measurements, and lava flow lengths. Eruptive styles are related to variable magma flux and accumulation of gas. Explosive degassing was recorded on broadband seismic and infrasound sensors in 2008 and 2009. Explosion energy partitioning between the ground and the atmosphere shows an increase in acoustic energy from 2008 to 2009, indicating a shift toward increased gas pressure in the conduit. Very-long-period (VLP) seismic signals are associated with the strongest explosions recorded in 2009 and waveform modeling in the 10 – 30 s band produces a best-fit source location 300 m west and 300 m below the summit crater. The calculated moment tensor indicates a volumetric source, which is modeled as a dike feeding a SW-dipping (35°) sill. The sill is the dominant component and its projection to the surface nearly intersects the summit crater. The deformation history of the sill is interpreted as: 1) an initial inflation due to pressurization, followed by 2) a rapid deflation as overpressure is explosively release, and finally 3) a reinflation as fresh magma flows into the sill and degasses. Tilt signals are derived from the horizontal components of the seismometer and show repetitive inflation deflation cycles with a 20 minute period coincident with strong explosions. These cycles represent the pressurization of the shallow conduit and explosive venting of overpressure that develops beneath a partially crystallized plug of magma. The energy released during the strong explosions has allowed for imaging of Fuego’s shallow conduit, which appears to have migrated west of the summit crater. In summary, Fuego is becoming more gas charged and its summit centered vent is shifting to the west - serious hazard consequences are likely.

Composition and age of volcanic rocks from the Sinii Utes Depression, Southern Primoye

New data are reported on structure of sections, chemical composition, and age of volcano-sedimentary and volcanic rocks from the Sinii Utes Depression in the Southern Primorye region. The Sinii Utes Depression is filled with two sequences: the lower sequence composed of sedimentary-volcanogenic coaliferous rocks (the stratotype of the Sinii Utes Formation) and the upper sequence consisting of tephroid with overlying basalts. This work considers chemical composition and problems of K-Ar dating of basalts. The uppermost basaltic flow has K-Ar age 22.0±1.0 Ma. The dates obtained for the middle and upper parts of lava flows are underestimated. It is explained by their heating due to combustion of brown coals of the Sinii Utes Formation underlying the lava flow. Calculations show that argon could only partly have been removed from the basalts owing to conductive heat transfer and was lost largely due to infiltration of hot gases in heterogeneous fissured medium. Basaltic volcanism on continental margins of the southern Primorye region and the adjacent Korean and Chinese areas at the Oligocene-Miocene boundary preceded Early-Middle Miocene spreading and formation of the Sea of Japan basin. Undifferentiated moderately alkaline basalts of intraplate affinity developed in the Amba Depression and some other structures of the southern Primorye region and intraplate alkali basalts of the Phohang Graben in the Korean Peninsula serve as indicators of incipient spreading regime in the Sea of Japan. Potassic basalt-trachybasalt eruptions occurred locally in riftogenic depressions and shield volcanoes. In some structures this volcanism was terminated by eruptions of intermediate and acid lavas. Such evolution of volcanism is explained by selective contamination of basaltic melts during their interaction with crustal acid material and generation of acid anatectic melts.

Paleomagnetic of basalts from ODP Site 145-883 on Detroit Seamount

Paleomagnetic data were measured from basaltic flows cored by the Ocean Drilling Program (ODP) at Site 883 on the summit of Detroit Seamount, located in the northernmost Emperor seamounts. These data are important because they reflect the paleolatitude of Hawaiian volcanism for the Late Cretaceous and bear upon geodynamic models of hotspot drift. A total of 143 samples were measured, from cores acquired at two ~20-30 m apart. Most samples gave apparently reliable magnetic directions that were analyzed in a tiered fashion to compute a composite inclination vs. depth curve. One hole gave 13 distinct inclination groups, the other 10, and the two were combined into nine groups thought to represent independent measurements of paleofield direction. These data indicate normal magnetic polarity and give a mean inclination of 61.5+10.6°/-6.4° and paleolatitude of 42.8+13.2°/-7.6° (95% confidence limits). This paleolatitude is 6.2° higher than results from another ODP site (884) drilled on the lower flank of the same seamount. The difference is thought to result partly from an age difference (1-3 Myr) and partly from incomplete averaging of paleosecular variation at both drill sites. Together, the data from the two sites reinforce the conclusion that the northern Emperor seamounts were formed far north of the present-day hotspot latitude (~19.5°N) and suggest prior estimates of the amount and rate of southward drift may have been low. This analysis also illustrates uncertainties in determining paleolatitude from a small number of lava flow units from a single drill site.

Geochemistry and mineralogy of ODP Leg 107 basalts

During ODP Leg 107, the basement of the Tyrrhenian Sea was drilled at Site 650, located in the Marsili basin, and at Sites 651 and 655, both located in the Vavilov basin. In addition, a lava flow was drilled at Site 654 on the Sardinia rifted margin. Mineral and whole rock major and trace element chemistry, including rare earth element (REE) and Sr and Nd isotopic ratios, were determined in samples of these rocks. Site 654 lava was sampled within uppermost Pliocene postrift sediments. This lava is a basaltic andesite of intraplate affinity, and is analogous to some Plio-Pleistocene tholeiitic lavas from Sardinia. Site 650 basalts, drilled beneath 1.7-1.9-Ma-old basal sediment, are strongly altered and vesicular suggesting a rapid subsidence of the Marsili basin. Based on incompatible trace elements, these basalts show calc-alkaline affinity like some products of the Marsili Seamount and the Eolian arc. The basement of the two sites drilled within Vavilov basin shows contrasting petrologies. Site 655, located along the Gortani ridge in the western part of the basin, drilled a 116-m-thick sequence of basalt flows beneath 3.4-3.6-Ma-old basal sediments. These basalts are chemically relatively homogeneous and show affinity to transitional MORB. Four units consisting of slightly differentiated basaltic lavas, have been identified. Site 655 basalts are geochemically similar to the high Ti lavas from DSDP Leg 42, Site 373 (Vavilov Basin). The basement at Site 651, overlain by 40 m of metalliferous dolostone covered by fossiliferous sediments with an age of 2 Ma, consists of two basalt units separated by a dolerite-albitite intrusive body; serpentinized harzburgites were drilled for 30 m at the base of the hole. The two basalt units of Site 651 are distinct petrochemically, though both show incompatible elements affinity with high-K calc-alkaline/calc-alkaline magmas from Eolian arc. The cpx chemistry and high K/Na ratio of the lower unit lavas suggest a weak alkaline tendency of potassic lineage. Leg 107 basement rock data, together with data from DSDP Site 373 and from dredged samples, indicate that the deepest basins of the central Tyrrhenian Sea are underlain by a complex back-arc basin crust produced by magmas with incompatible element affinities to transitional MORB (Site 655 and DSDP Site 373), and to calc-alkaline and high-K calc-alkaline converging plate margin basalts (Sites 650 and 651). This petrogenetic complexity is in accordance with the back-arc setting of the Vavilov and Marsili basins. Other back-arc basin basalts, particularly those from ensialic basins such as the Bransfield Strait (Antarctica), show a comparable petrogenetic complexity (cf., Sounders and Tarney, 1984).

Major elements oxides and mineralogy of primary minerals in ODP Hole 195-1201D basalts

The basement cored at Site 1201 (west Philippine Basin) during Ocean Drilling Program Leg 195 consists of a 91-m-thick sequence of basalts, mostly pillow lavas and perhaps one sheet lava flow, with a few intercalations of hyaloclastite and interpillow sedimentary material. Hydrothermal alteration pervasively affected the basalt sequence, giving rise to a variety of secondary minerals such as K-Fe-Mg-clay minerals, oxyhydroxides and clay minerals mixtures, natrolite group zeolites, analcite, alkali feldspar, and carbonate. The primary minerals of pillow and sheet basalts that survived the intense hydrothermal alteration were investigated by electron microprobe with the aim of characterizing their chemical composition and variability. The primary minerals are mostly plagioclase, ranging in composition from bytownite through labradorite to andesine, chromian-magnesian-diopside, and spinels, both Ti magnetite (partially maghemitized) and chromian spinel. Overall, the chemical features of the primary minerals of Site 1201 basalts correspond to the primitive character of the bulk rocks, suggesting that the parent magma of these basalts was a mafic tholeiitic magma that most likely only suffered limited fractional crystallization and crystallized at high temperatures (slightly below 1200°C) and under increasing fO2 conditions. The major element composition of clinopyroxene suggests a backarc affinity of the mantle source of Site 1201 basement.

Nannofossil abundance and lithologic description of ODP Hole 197-1203A and Site 197-1204

Calcareous nannofossils occur in numerous layers within a thick volcaniclastic succession encountered on the Detroit Seamount. Nannofossils present in a given bed confirm a marine depositional environment for the bed, add to our understanding of depositional events occurring between times of lava flow, and contribute to the interpretation of the overall physical volcanological history of the seamount.

(Supplemet S1) Silicon oxide and Potassium + Sodium oxide from the PACManus hydrothermal area

This study presents a systematic analysis and interpretation of autonomous underwater vehicle-based microbathymetry combined with remotely operated vehicle (ROV) video recordings, rock analyses and temperaturemeasurements within the PACManus hydrothermal area located on Pual Ridge in the Bismarck Sea of eastern Manus Basin. The data obtained during research cruise Magellan-06 and So-216 provides a framework for understanding the relationship between the volcanism, tectonismand hydrothermal activity. PACManus is a submarine felsic vocanically-hosted hydrothermal area that hosts multiple vent fields locatedwithin several hundredmeters of one another but with different fluid chemistries, vent temperatures and morphologies. The total area of hydrothermal activity is estimated to be 20,279m**2. Themicrobathymetrymaps combinedwith the ROV video observations allow for precise high-resolution mapping estimates of the areal extents of hydrothermal activity.We find the distribution of hydrothermal fields in the PACManus area is primarily controlled by volcanic features that include lava domes, thick andmassive blocky lava flows, breccias and feeder dykes. Spatial variation in the permeability of local volcanic facies appears to control the distribution of venting within a field.We define a three-stage chronological sequence for the volcanic evolution of the PACManus based on lava flow morphology, sediment cover and lava SiO2 concentration. In Stage-1, sparsely to moderately porphyritic dacite lavas (68-69.8 wt.% SiO2) erupted to form domes or cryptodomes. In Stage-2, aphyric lava with slightly lower SiO2 concentrations (67.2-67.9 wt.% SiO2) formed jumbled and pillowed lava flows. In the most recent phase Stage-3, massive blocky lavaswith 69 to 72.5wt.% SiO2were erupted throughmultiple vents constructing a volcanic ridge identified as the PACManus neovolcanic zone. The transition between these stages may be gradual and related to progressive heating of a silicic magma following a recharge event of hot, mantle-derived melts.

Geochemistry of Pleistocene volcanic rocks in the Mariana Forearc

Geophysical surveys of the Mariana forearc, in an area equidistant from the Mariana Trench and the active Mariana Island Arc, revealed a 40-m-deep graben about 13 km northwest of Conical Seamount, a serpentine mud volcano. The graben and its bounding horst blocks are part of a fault zone that strikes northwest-southeast beneath Conical Seamount. One horst block was drilled during Leg 125 of the Ocean Drilling Program (Site 781). Three lithologic units were recovered at Site 781: an upper sedimentary unit, a middle basalt unit, and a lower sedimentary unit. The upper unit, between 0 and 72 mbsf, consists of upper Pliocene to Holocene diatomaceous and radiolarian-bearing silty clay that grades down into vitric silty clay and vitric clayey silt. The middle unit is a Pleistocene vesicular, porphyritic basalt, the top of which corresponds to a high-amplitude reflection on the reflection profiles. The lower unit is a middle to upper (and possibly some lower) Pliocene vitric silty clay and vitric clayey silt similar to the lower part of the upper unit. The thickness of the basalt unit can only be estimated to be between 13 and 25 m because of poor core recovery (28% to 55%). The absence of internal flow structures and the presence of an upper glassy chilled zone and a lower, fine-grained margin suggest that the basalt unit is either a single lava flow or a near-surface sill. The basalt consists of plagioclase phenocrysts with subordinate augite and olivine phenocrysts and of plagioclase-augite-olivine glomerocrysts in a groundmass of plagioclase, augite, olivine, and glass. The basalt is an island arc tholeiite enriched in large-ion-lithophile elements relative to high-field-strength elements, similar to the submarine lavas of the southern arc seamounts. In contrast, volcanic rocks from the active volcanoes on Pagan and Agrigan islands, 100 km to the west of the drill site, are calc-alkaline. The basalt layer, the youngest in-situ igneous layer reported from the Izu-Bonin and Mariana forearcs, is enigmatic because of its location more than 100 km from the active volcanic arc. The sediment layers above and below the basalt unit are late Pliocene in age (about 2.5 Ma) and normally magnetized. The basalt has schlierenlike structures, reverse magnetization, and a K-Ar age of 1.68±0.37 Ma. Thus, the basalt layer is probably a sill fed by magma intruded along a fault zone bounding the horst and graben in the forearc. The geochemistry of the basalt is consistent with a magma source similar to that of the active island arc and from a mantle source above the subducting Pacific plate.