Well-preserved Late Paleoproterozoic volcanic centers in the Sao Felix do Xingu region, Amazonian Craton, Brazil

The Amazonian craton in the Sao Felix do Xingu city, southeast region of the Para state, north of Brazil, hosts exceptionally well-preserved Paleoproterozoic bimodal magmatic units grouped in the Sobreiro and Santa Rosa formations. These formations are correlated to the Uatuma magmatic event, which is largely distributed in the Amazonian craton occupying more than 1,500,000 km(2). Geological mapping and petrographical observations reveal distinct spectra of volcanic facies in both formations. The basal calc-alkaline Sobreiro Formation is composed mainly of andesitic and dacitic lava flows and associated volcaniclastic facies of autoclastic origin, with subordinate pyroclastic flow deposits. This formation shows inferred eruption style that is similar to those in Flood Basalt Provinces, with rare scutulum-type lava shields. The upper A-type Santa Rosa Formation was generated by multicyclic explosive and effusive episodes predominantly associated with large fissures and is materialized by voluminous ignimbrites with subordinated ash-fall tuff, crystal tuff, lapilli-tuff, co-ignimbritic breccias, rhyolitic dikes and domes, and associated granitic porphyries and equigranular granitic intrusions. Ignimbrite and rhyolite dikes reveal conspicuous vertical flow pattern pointing to a fissure-controlled eruption, similar to Sierra Madre Occidental ignimbrite province. The proposed evolutionary model for the Sao Felix do Xingu units differs from those of other occurrences related to the Uatuma magmatic event in the Amazonian craton, characterized by predominance of A-type volcanism and contemporaneous granites. (C) 2010 Elsevier B.V. All rights reserved.

Caracterização geológica e geotécnica dos complexos vulcânicos antigo e intermédio da Ilha da Madeira

Este trabalho pretende contribuir para aprofundar o conhecimento geológico e geotécnico das formações vulcânicas da ilha da Madeira. Por razões de ordem técnica, apenas foi possível proceder à caracterização geológica e geotécnica de três dos cinco afloramentos, inicialmente previstos. As amostras estudadas pertencem aos Complexos Vulcânicos Antigo e Intermédio, definidos pela nova vulcano-estratigrafia da ilha da Madeira, cuja carta geológica se encontra em fase de publicação. Foca-se, inicialmente, a ilha da Madeira, enquadrando-a no espaço e no tempo geológico e apresentando a sua vulcano-estratigrafia. Seguem-se os estudos geológicos e geotécnicos, indispensáveis, para caracterizar as amostras escolhidas. Neste capítulo e numa primeira fase, é efectuada uma caracterização geológica das amostras em estudo, sendo, seguidamente, abordado o acompanhamento realizado durante a execução dos ensaios realizados in situ e em laboratório, bem como, os resultados obtidos, segundo as normas em vigor, com vista a caracterizar geotecnicamente as amostras escolhidas. Na fase de discussão, faz-se uma análise aos resultados obtidos das caracterizações geológicas e geotécnicas, procurando relações existentes e comparando-as a outras já existentes na ilha da Madeira e no arquipélago das Canárias. Por fim apresenta-se a caracterização geológica e geotécnica das três amostras. A ter em consideração que o presente trabalho, representa apenas um pequeno contributo, pretendendo acrescentar os resultados obtidos a alguns já existentes e a outros que advirão, tendo em conta que a este nível existe pouca informação relativa a arquipélago da Madeira.

Morfometria e descrição de otólitos de dourada (Brachyplatystoma rosseauxii) (Castelnau, 1855) e de piramutaba (B. vaillantii) (Valenciennes, 1840) (Siluriformes: pimelodidae) e verificação de anéis de crescimento em otólitos de juvenis de dourada e de piramutaba na Ilha de Colares - Baía de Marajó-PA

A dourada (Brachyplatystoma rousseauxii) e a piramutaba (B. vaillantii), são dois bagres migradores de água doce, exploradas pela pesca comercial artesanal e industrial na Amazônia. São de grande importância para a pesca comercial nesta região e atualmente seus estoques estão em estado de sobrexplotação. A literatura cientifica não registra trabalhos sobre a biologia e ecologia referentes aos estágios juvenis destes bagres. Em estudos de dinâmica populacional, a correta estimação da idade é essencial na estimativa dos parâmetros de crescimento, que são essenciais para a avaliação dos estoques. Os estudos de determinação de idade geralmente são feitos em espécimes subadultos e adultos e a idade dos juvenis é retrocalculada. O que pode levar aos erros de avaliação. A presente pesquisa teve como objetivos: (1) descrever e estimar as relações entre as medidas morfométricas dos otólitos lapillus com as medidas corporais de dourada e de piramutaba, e (2) verificar o surgimento dos primeiros anéis de crescimento nos espécimes juvenis. Para o estudo da morfometria e descrição foram utilizados otólitos de dourada e de piramutaba juvenis, sub-adultos e adultos provenientes dos Municípios de Colares (PA), Almeirim (PA), Santarém (PA), Manaus (AM), do Distrito de Mosqueiro (PA), e do estuário amazônico. O período de coletas foi diferente para cada local, e de setembro de 1996 a janeiro de 2006. As seguintes relações foram estimadas: comprimento furcal dos espécimes (CF) x peso total dos espécimes (PT); CF x comprimento máximo do otólito (CMO); CF x largura máxima do otólito (LMO); CF x peso total do otólito (PTO); PT x CMO; PT x LMO e PT x PTO. E as equações estimadas foram: Dourada: PT = 9,5 x 10-6 x Cf 3,0279, CF = 25,259 * CMO1,1571, CF = 40,626 * LMO1,2127, CF = 840,419 * PTO0,4077, PT = 0,125 * CMO3,6547, PT = 0,568 * LMO3,8294, PT = 7549,98 * PTO1,2651; Piramutaba: PT = 5,4 x 10-6 x Cf 3,1441, CF = 31,871 * CMO1,3381, CF = 55,852 * LMO1,3722, CF = 1641,064 * PTO0,4686, PT = 0,3127 * CMO4,1857, PT = 1,823 * LMO4,2788, PT = 66675,977 * PTO1,4508. A descrição dos otólitos classificou os lapilli de dourada e de piramutaba em três categorias conforme seu desenvolvimento e CF dos espécimes: dourada I (60 a 80 mm), dourada II (80 a 110 mm), dourada III (110 a 210 mm), piramutaba I (65 a 80 mm), piramutaba II (80 a 110 mm), e piramutaba III (110 a 190 mm). E no estudo da verificação de anéis de crescimento em lapillus foram utilizados somente os juvenis, com CF £ 200 mm. Na baía de Marajó, a dourada e a piramutaba forma o primeiro anel de crescimento com CF médio de 175,03 mm e 171,03 mm, respectivamente. E as duas espécies têm entre nove e doze meses de idade quando formam o primeiro anel de crescimento. Os raios médios do primeiro anel hialino do corte transversal do lapillus de dourada e de piramutaba foram 0,36 mm (± 0,03) e 0,33 mm (± 0,01), respectivamente. O raio total médio do corte transversal do lapillus de dourada foi de 0,64 mm (± 0,14) e o da piramutaba foi de 0,53 mm (± 0,09). A equação obtida entre o raio total do corte transversal do lapillus de juvenis de dourada com seu CF foi CF = 248,589 * Rt1,1901. E a equação estimada para a piramutaba foi CF = 400,494 * Rt1,7178. Douradas e piramutabas com CF de 60-70 mm têm idade de três a seis meses, com CF de 70-110 mm têm de seis a nove meses e com CF de 110-200 mm têm de nove a doze meses.

Vulcanismo félsico paleoproterozoico do Grupo Iricoumé, Domínio Erepecuru-Trombetas, Província Amazônia Central: dados de campo, caracterização petrográfica e geocronologia Pb-Pb em zircão

O Grupo Iricoumé compreende rochas vulcânicas efusivas e piroclásticas, com texturas e estruturas bastante preservadas, que pertence a um extenso evento vulcano-plutônico que marcou a região central do Cráton Amazônico durante o Orosiriano. Tais rochas estão expostas no noroeste do estado do Pará, na porção meridional do sudoeste do Domínio Erepecuru-Trombetas, sul do Escudo das Guianas. Estudos petrográficos permitiram distinguir um vulcanismo explosivo, predominante e representado por rochas piroclásticas (ignimbritos, reoignimbritos, tufo coignimbrítico de queda e lápili-tufo relacionado a surge), e um efusivo, subordinado, representado por fluxos de lavas coerentes e rochas hipabissais (andesitos, lamprófiros espessartíticos e latitos). A maioria das rochas piroclásticas exibe feições diagnósticas da deposição dos piroclastos sob altas temperaturas, sugerindo que as rochas vulcânicas estão provavelmente relacionadas a ambientes de geração de caldeiras. As idades Pb-Pb de 1888 ± 2,5 e 1889 ± 2 Ma obtidas em zircão de ignimbritos traquidacíticos confirmam que a maioria das rochas estudadas pertence ao Grupo Iricoumé. Por outro lado, a idade Pb-Pb de 1992 ± 3 Ma obtida em zircão de um andesito evidencia um episódio vulcânico efusivo orosiriano mais antigo, já reconhecido, localmente, mais a sul, no Domínio Tapajós. Os dados obtidos demonstram a ampla extensão do vulcanismo Iricoumé e rochas vulcânicas correlatas na porção central do Cráton Amazônico, e constituem argumentos favoráveis para associar esse episódio vulcânico e rochas magmáticas correlatas a uma silicic large igneous province (SLIP), como já vem sendo descrito por alguns autores.

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.

Caracterización del comportamiento hidráulico y químico del picón como material para la depuración natural del estiércol líquido de rumiantes

[ES] Los efluentes ganaderos constituyen un beneficioso aporte de nutrientes para los cultivos, que es fundamental a la hora de garantizar la sostenibilidad de la gestión de las explotaciones ganaderas, pudiendo ocasionar graves problemas ambientales si se emplean mal. La intensificación agraria ha convertido los efluentes ganaderos de subproducto a residuo. Su tratamiento con materiales locales y tecnologías de baja intensidad es una solución de bajo coste financiero y energético. En el proyecto REAGUA se plantea la posibilidad de utilizar el “picón” (lapilli) como material para el tratamiento del estiércol líquido de rumiantes, para su posterior empleo en el riego enterrado de especies forrajeras y biocombustibles, actuando el suelo como medio de depuración avanzado. Para ello, se diseña un sistema en el que se aporte el efluente con un flujo subsuperficial vertical en un medio no saturado, que circule por tres fases (en serie). Para determinar las condiciones de manejo que optimicen el filtrado se caracterizó el comportamiento hidráulico del picón y su capacidad de eliminar sustancias. Utilizando tres columnas rellenas de picón y un efluente de rumiantes, las reducciones de la DQO, DBO5 y amonio, fósforo y SS superaron el 80, 90% y 95% respectivamente, obteniéndose valores asumibles para inyectarse al riego.

Fossil bubble in porphyritic basaltic pyroclasts produced by small and large strombolian eruption at Pacaya, Guatemala

We investigate compositionally monotonous, but energetically diverse, tephra samples from Pacaya to see if fossil bubbles in pyroclasts could reflect eruptive style. Bubble size distributions (BSD) were determined for four ash to lapilli size tephra samples using an adapted version of stereology conversion by Sahagian and Proussevitch (1998). Eruptions range from very weak to very energetic. Hundreds of ESEM BSEs images were processed throughout ImageJ software for a robust and statistically correct data set of vesicles (minimum 700 bubbles per sample). Qualitative textural analysis and major element chemical compositions were also executed. There is higher vesicularity for explosive pyroclasts and an inverse correlation between bubble number density (NV) and explosivity.

Determination of sulfite and manganese in sediments from the K/T boundary

The solid-state-physics technique of electron spin resonance (ESR) has been employed in an exploratory study of marine limestones and impact-related deposits from Cretaceous-Tertiary (KT) boundary sites including Spain (Sopelana and Caravaca), New Jersey (Bass River), the U.S. Atlantic continental margin (Blake Nose, ODP Leg 171B/1049/A), and several locations in Belize and southern Mexico within -600 km of the Chicxulub crater. The ESR spectra of SO3(1-) (a radiation-induced point defect involving a sulfite ion substitutional for CO3(2-) which has trapped a positive charge) and Mn(2+) in calcite were singled out for analysis because they are unambiguously interpretable and relatively easy to record. ESR signal strengths of calcite-related SO3(1-) and Mn(2+) have been studied as functions of stratigraphic position in whole-rock samples across the KT boundary at Sopelana, Caravaca, and Blake Nose. At all three of these sites, anomalies in SO3(1-) and/or Mn(2+) intensities are noted at the KT boundary relative to the corresponding background levels in the rocks above and below. At Caravaca, the SO3(1-) background itself is found to be lower by a factor of 2.7 in the first 30,000 years of the Tertiary relative to its steady-state value in the last 15,000 years of the Cretaceous, indicating either an abrupt and quasi-permanent change in ocean chemistry (or temperature) or extinction of the marine biota primarily responsible for fixing sulfite in the late Cretaceous limestones. An exponential decrease in the Mn(2+) concentration per unit mass calcite, [Mn(2+)], as the KT boundary at Caravaca is approached from below (1/e characteristic length =1.4 cm) is interpreted as a result of post-impact leaching of the seafloor. Absolute ESR quantitative analyses of proximal impact deposits from Belize and southern Mexico group naturally into three distinct fields in a twodimensional [SO3(1-)]-versus-[Mn(2+)] scatter plot. These fields contain (I) limestone ejecta clasts, (II) accretionary lapilli, and (III) a variety of SO3(1-) -depleted/Mn(2+) enriched impact deposits. Data for the investigated non-impact-related Cretaceous and Tertiary marine limestones (Spain and Blake Nose) fall outside of these three fields. With reference to thes enon-impact deposits, fields I, II, and III can be respectively characterized as Mn(2+) -depleted, SO3(1-) -enhanced, and SO3(1-) -depleted. It is proposed that (1) field I represents calcites from the Yucatin Platform, and that the Mn(2+) -depleted signature can be used as an indicator of primary Chicxulub ejecta in deep marine environments and (2) field II represents calcites that include a component formed in the vapor plume, either from condensation in the presence of CO2/SO3(1-) -rich vapors, or reactions between CaO and CO2/SO3 rich vapors, and that this SO3(1-) -enhanced signature can be used as an indicator of impact vapor plume deposits. Given these two propositions, the ESR data for the Blake Nose deposits are ascribed to the presence of basal coarse calcitic Chicxulub ejecta clasts, while the finer components that are increasingly represented toward the top are interpreted to contain high- SO3(1-) calcite from the vapor plume. The apparently-undisturbed Bass River deposit may contain even higher concentrations of vapor-plume calcite. None of the three components included in field III appear to be represented at distal, deep marine KT-boundary sites; this field may include several types of impact-related deposits of diverse origins and diagenetic histories.

Preliminary results and documentation of sediment cores CRP2 and CRP-2A from the Ross Sea off Cape Roberts, Antarctica

The site for CRP-2, 14 km east of Cape Roberts (77.006°S; 163.719°E), was selected to overlap the early Miocene strata cored in nearby CRP-1, and to sample deeper into the east-dipping strata near the western margin ofe he Victoria Land Basin to investigate Palaeogene climatic and tectonic history. CRP-2 was cored from 5 to 57 mbsf (metres below the sea floor) (core recovery 91 %), with a deviation resulting in CRP-2A being cored at the same site. CRP-2A reached down to 624mbsf (recovery 95%), and to strata with an age of c. 33-35 Ma. Drilling took place from 16 October to 25 November 1998, on 2.0-2.2 m of sea ice and through 178 m of water. Core fractures and other physical properties, such as sonic velocity, density and magnetic susceptibility, were measured throughout the core. Down-hole logs for these and other properties were run from 63 to 167 mbsf and subsequently from 200 to 623 mbsf, although density and velocity data could be obtained only to 440 mbsf because of hole collapse. Sonic velocity averages c. 2.0 km S-1 for the upper part of the hole, but there is an sharp increase to c. 3.0 km s-1 and also a slight angular unconformity, at 306 mbsf, corresponding most likely to the early/late Oligocene boundary (c. 28-30 Ma). Velocity then increases irregularly to around 3.6 km s-1 at the bottom of the hole, which is estimated to lie 120 m above the V4/V5 boundary. The higher velocities below 306 mbsf probably reflect more extensive carbonate and common pyrite cementation, in patches, nodules, bedding-parallel masses and as vein infills. Dip of the strata also increases down-hole from 3° in the upper 300 in to over 10° at the bottom. Temperature gradient is 21° k-1. Over 2 000 fractures were logged through the hole. Borehole televiewer imagery was obtained for the interval from 200 to 440 mbsf to orient the fractures for stress field analysis. Lithostratigraphical descriptions on a scale of 1:20 are presented for the full length of the core, along with core box images, as a 200 page supplement to this issue. The hole initially passed through a layer of muddy gravel to 5.5 mbsf (Lithological Sub-Unit or LSU 1.1), and then into a Quaternary diatom-bearing clast-rich diamicton to 21 mbsf (LSU 2. l), with an interval of alternating compact diamicton and loose sand, and containing a rich Pliocene foraminiferal fauna, to 27 mbsf (LSU 2.2). The unit beneath this (LSU 3.1) has similar physical properties (sonic velocity, porosity, magnetic susceptibility) and includes diamictites of similar character to those of LSU 2.1 and 2.2, but an early Miocene (c. 19 Ma) diatom assemblage at 28 mbsf (top of LSU 3.1) shows that this sub-unit is part of the older section. The strata beneath 27 mbsf, primary target for the project, extend from early Miocene to perhaps latest Eocene age, and are largely cyclic glacimarine nearshore to offshore sediments. They are described as 41 lithological sub-units and interpreted in terms of 12 recurrent lithofacies. These are 1) mudstone, 2) inter-stratified mudstone and sandstone, 3) muddy very fine to coarse sandstone, 4) well-sorted stratified fine sandstone, 5) moderately to well-sorted, medium-grained sandstone, 6) stratified diamictite, 7) massive diamictite, 8) rhythmically inter-stratified sandstone and mudstone, 9) clast-supported conglomerate, 10) matrix-supported conglomerate, 11) mudstone breccia and 12) volcaniclastic sediment. Sequence stratigraphical analysis has identified 22 unconformity-bounded depositional sequences in pre- Pliocene strata. They typically comprise a four-part architecture involving, in ascending order, 1) a sharp-based coarse-grained unit (Facies 6,7,9 or 10), 2) a fining-upward succession of sandstones (Facies 3 and 4), 3) a mudstone interval (Facies l), in some cases coarsening upward to muddy sandstones (Facies 3), and 4) a sharp-based sandstone dominated succession (mainly Facies 4). The cyclicity recorded by the strata is interpreted in terms of a glacier ice margin retreating and advancing from land to the west, and of rises and falls in sea level. Analysis of sequence periodicity awaits afirmer chronology. However, apreliminary spectral analysis of magnetic susceptibility for a deepwater mudstone within one of the sequences (from 339 to 347 mbsf) reveals ratios between hierarchical levels that are similar to those of the three Milankovitch orbital forcing periodicities. The strata contain a wide range of fossils, the most abundant being marine diatoms. These commonly form up to 5% of the sediment, though in places the core is barren (notably between 300 and 412 mbsf). Fifty samples out of 250 reviewed were studied in detail. The assemblages define ten biostratigraphical zones, some of them based on local or as yet undescribed forms. The assemblages are neritic, and largely planktonic, suggesting that the sea floor was mostly below the photic zone throughout deposition of the corcd sequence. Calcareous nannofossils, representing incursions of ocean surface waters, are much less common (72 out of 183 samples examined) and restricted to mudstone intervals a few tens of metres thick, but are important for dating. Foraminifera are also sparse (73 out of 135 samples) and represented only by calcareous benthic species. Changing assemblages indicate a shift from inshore environments in the early Oligocenc to outer shelf in the late Oligocenc, returning to inshore in the early Miocene. Marine palynomorplis yielded large numbers of well-preserved forms from most of the 116 samples examined. The new in situ assemblagc found last year in CRP-1 is extended down into the late Oligocene and a further new assemblage is found in the early Oligoccnc. Many taxa are new, and cannot us yet contribute to an improved understanding of chronology or ecology. Marine invertebrate macrofossils, mostly molluscs and serpulid tubes, are scattered throughout the core. Preservation is good in mudstones but poor in other lithologies. Climate on land is reflected in the content of terrestrial palynomorphs, which are extremely scarce down to c. 300 mbsf. Some forms are reworked, and others represent a low growing sparse tundra with at least one species of Nothofagus. Beneath this level, a significantly greater diversity and abundance suggests a milder climate and a low diversity woody vegetation in the early Oligocene, but still far short of the richness found in known Eocene strata of the region. Sedimentary facies in the oldest strata also suggest a milder climate in the oldest strata cored, with indications of substantial glacial melt-water discharges, but are typical of a coldcr climate in late Oligocene and early Miocene times. Clast analyses from diamictites reveal weak to random fabrics, suggesting either lack of ice-contact deposition or post-depositional modification, but periods when ice grounded at the drill site are inferred from thin zones of in-situ brecciated rock and soft-sediment folding. These are more common above c. 300 mbsf, perhaps reflecting more extensive glacial advances during deposition of those strata. Erosion of the adjacent Transantarctic Mountains through Jurassic basalt and dolerite-intruded Beacon strata into basement rocks beneath is recorded by petrographical studies of clast and sand grain assemblages. Core below 310 mbsf contains a dominance of fine-grained Jurassic dolerite and basalt fragments along with Beacon-derived coal debris and rounded quartz grains, whereas the strata above this level have a much higher proportion of basement derived granitoids, implying that the large areas of the adjacent mountains had been eroded to basement by the end of the early Oligocene. There is little indication of rift-related volcanism below 310 mbsf. Above this, however, basaltic and trachytic tephras are common, especially from 280 to 200 mbsf, from 150 to 46 mbsf, and in Pliocene LSU 2.2 from 21 to 27 mbsf. The largest volcanic eruptions generated layers of coarse (up to 1 cm) trachytic pumice lapilli between 97 and 114 mbsf. The thickest of these (1.2 m at 112 mbsf) may have produced an eruptive column extending tens of km into the stratosphere. A source within a few tens of km of the drill site is considered most likely. Present age estimates for the pre-Pliocene sequence are based mainly on biostratigraphy (using mainly marine diatoms and to a lesser extent calcareous nannofossils), with the age of the tephra from 112 to 114 mbsf (21.44k0.05 Ma from 84 crystals by Ar-Ar) as a key reference point. Although there are varied and well-preserved microfossil assemblages through most of the sequence (notably of diatoms and marine palynomorphs), they comprise largely taxa either known only locally or as yet undescribed. In addition, sequence stratigraphical analysis and features in the core itself indicate numerous disconformities. The present estimate from diatom assemblages is that the interval from 27 to 130 mbsf is early Miocene in age (c. 19 to 23.5 Ma), consistent with the Ar-Ar age from 112 to 114 mbsf. Diatom assemblages also indicate that the late Oligocene epoch extends from c. 130 to 307 mbsf, which is supported by late Oligocene nannofossils from 130 to 185 mbsf. Strata from 307 to 412 mbsf have no age-diagnostic assemblages, but below this early Oligocene diatoms and nannofossils have been recovered. A nannoflora at the bottom of the hole is consistent with an earliest Oligocene or latest Eocene age. Magnetostratigraphical studies based on about 1000 samples, 700 of which have so far undergone demagnetisation treatment, have provided a polarity stratigraphy of 12 pre-Pliocene magnetozones. Samples above 270 mbsf are of consistently high quality. Below this, magnetic behaviour is more variable. A preliminary age-depth plot using the Magnetic Polarity Time Scale (MPTS) and constrained by biostratigraphical data suggests that episodes of relatively rapid sedimentation took place at CRP-2 during Oligocene times (c. 100 m/My), but that more than half of the record was lost in a few major and many minor disconformities. Age estimates from Sr isotopes in shell debris and further tephra dating are expected to lead to a better comparison with the MPTS. CRP-2/2A has recorded a history of subsidence of the Victoria Land Basin margin that is similar to that found in CIROS-170 km to the south, reflecting stability in both basin and the adjacent mountains in late Cenozoic times, but with slow net accumulation in the middle Cenozoic. The climatic indicators from both drill holes show a similar correspondence, indicating polar conditions for the Quaternary but with sub-polar conditions in the early Miocene-late Oligocene and indications of warmer conditions still in the early Oligocene. Correlation between the CRP-2A core and seismic records shows that seismic units V3 and V4, both widespread in the Victoria Land Basin, represent a period of fluctuating ice margins and glacimarine sedimentation. The next drill hole, CRP-3, is expected to core deep into V5 and extend this record of climate and tectonics still further back in time.

Geochemistry of felsic rocks and minerals of ODP Hole 135-841B

A felsic volcanic series (605-825 mbsf) overlain by upper Eocene shallow-water sediments (500-605 mbsf) and basalticandesitic sills that intruded into sediments of Holocene to Miocene age (0-500 mbsf) was drilled in the forearc region of the Lau Basin at a water depth of 4810 m. The volcanic sequence at Site 841 includes altered and mineralized calc-alkaline rhyolites and dacites, dacitic tuffs, lapilli tuffs, flow breccias, and welded tuffs. These rocks formed subaerially or in a very shallow-water environment suffering a subsidence of >5000 m since Eocene times. Calculations of gains and losses of the major components during alteration show most pronounced changes in the uppermost 70 m of the volcanic sequence. Here, Al, Fe, Mg, and K are enriched, whereas Si and Na are strongly depleted. Illite, vermiculite, chlorite, and hematite predominate in this part of the hole. Throughout the section, quartz, plagioclase, kaolinite, and calcite are present. Sulfide mineralization (up to 10 vol%) consisting mainly of disseminated pyrite (with minor pyrrhotite inclusions) and marcasite together with minor amounts of chalcopyrite is pervasive throughout. Locally, a few sulfide-bearing quartz-carbonate veins as well as Ti-amphibole replacement by rutile and then by pyrite were observed. Strong variations in the As content of sulfides (from 0 to 0.69 wt%) from the same depth interval and local enrichments of Co, Ni, and Cu in pyrite are interpreted to result from fluctuations in fluid composition. Calculations of oxygen and sulfur fugacities indicate that fO2 and fS2 were high at the top and lower at the bottom of the sequence. Sulfur isotope determinations on separated pyrite grains from two samples give d34S values of +6.4ë and +8.4ë, which are close to those reported from Kuroko and Okinawa Trough massive sulfide deposits and calc-alkaline volcanic rocks of the Japanese Ryukyu Island Arc. Calculated chlorite formation temperatures of 265°-290°C at the top of the sequence are consistent with minimum formation temperatures of fluid inclusions in secondary quartz, revealing a narrow range of 270°-297°C. Chlorite formation temperatures are constant downhole and do not exceed 300°C. The presence of marcasite and 4C-type pyrrhotite indicates a formation temperature of <= 250°C. At a later stage, illite was formed at the top of the volcanic series at temperatures well below 200°C.

Sediments and tephra layers from the southern Tyrrhenian abyssal plain near Marsili Seamount

From the south-eastern Tyrrhenian deep-sea floor, four sediment cores of "Meteor" cruise 22 (1971) are described. These cores were taken in the basin between the Aeolian Islands and the Marsili Seamount, an elevation of more tha 3000 m above the sea floor. The sedimentation of the deep-sea basin is distinguished by a sequence of turbidites with a high sedimentation rate. The composition of the clastic material and the position of the cores in the mouth area of the morphologically very pronounced Stromboli Canyon suggest an interpretation of the turbidite sequence as fan of this canyon onto the deep-sea floor. A white rhyolitic pumice-tephra at the base of the 4 m thick sequence of turbidites in core M22-102 has been correlated with the Pelato eruption of the island of Liparo in the 6th century A.D. At the foot of the Marsili Seamount - apparently in morphologically elevated positions - the influence of the turbidite sedimentation increases, the rate of sedimentation is lower and stratigraphic omissions are probable. Here, rather compacted globigerina marls have been found in only 15 -25 cm depth. In addition, volcanic material in the form of lapilli layers, palagonitized ashes and detrital volcanic sands of the Marsili Seamount have been encountered in this area. An up to 3 cm thick layer of completely palagonitized basaltic ash intercalates with the marls at the base of two cores. Layers of very fresh olivine basaltic lapilli in core 103 and palagonitized lapilli of latitic composition in core 104 testify to an explosive submarine volcanism of the Marsili Seamount. According to the stratigraphy of core 103, the latest manifestations of this basaltic volcanism belong to the late Pleistocene (Emiliana huxleyi-zone of Nannoplankton stratigraphy) The basaltic lapilli are glassy to perhyaline with phenocrysts or microphenocrysts predominantely of olivine. The petrological character of the basaltic volcanites with high MgO, Ni, Cr and high MgO/FeO- and Ni/Co-ratios exhibits primitive basaltic features. These basalts clearly differ from basalts of the ocean floors, mid-ocean ridges and marginal basins. Prominent features are a missing iron-enrichment trend and low TiO2. Al2O3 tends to be high, as well as K2O and related trace elements (Ba, Sr). In spite of silica undrsaturation and high color index, the Marsili basalt exhibit some analogies with the calcalkaline basalts of the Aeolian arc, as well as the undersaturated basalts of some other circumoceanic areas.