ALBERT

Description: Although rising global sea levels will affect the shape of coastlines over the coming decades1, 2, the most severe and catastrophic shoreline changes occur as a consequence of local and regional-scale processes. Changes in sediment supply3 and deltaic subsidence4, 5, both natural or anthropogenic, and the occurrences of tropical cyclones4, 5 and tsunamis6 have been shown to be the leading controls on coastal erosion. Here, we use satellite images of South American mangrove-colonized mud banks collected over the past twenty years to reconstruct changes in the extent of the shoreline between the Amazon and Orinoco rivers. The observed timing of the redistribution of sediment and migration of the mud banks along the 1,500 km muddy coast suggests the dominant control of ocean forcing by the 18.6 year nodal tidal cycle7. Other factors affecting sea level such as global warming or El Niño and La Niña events show only secondary influences on the recorded changes. In the coming decade, the 18.6 year cycle will result in an increase of mean high water levels of 6 cm along the coast of French Guiana, which will lead to a 90 m shoreline retreat.

Description: THE rare deep-sea octopod Cirrothauma murrayi Chun 1910 was first described from a single specimen caught during the Michael Sars Expedition of 1910 (ref. 1). Until now it has been caught only four more times2. We describe here three specimens of this species that were recently caught during biological cruises of RRS Discovery (Fig. 1). All of these animals, including the Discovery ones, have been caught at depths of more than 1,500 m, except one that was dip-netted through the ice of the Arctic Ocean3.

Description: We examined the physiological responses of steady-state iron (Fe)-replete and Fe-limited cultures of the biogeochemically critical marine unicellular diazotrophic cyanobacterium Crocosphaera at glacial (19 Pa; 190 ppm), current (39 Pa; 380 ppm), and projected year 2100 (76 Pa; 750 ppm) CO2 levels. Rates of N2 and CO2 fixation and growth increased in step with increasing partial pressure of CO2 (pCO2), but only under Fe-replete conditions. N2 and carbon fixation rates at 75 Pa CO2 were 1.4-1.8-fold and 1.2-2.0-fold higher, respectively, relative to those at present day and glacial pCO2 levels. In Fe-replete cultures, cellular Fe and molybdenum quotas varied threefold and were linearly related to N2 fixation rates and to external pCO2. However, N2 fixation and trace metal quotas were decoupled from pCO2 in Fe-limited Crocosphaera. Higher CO2 and Fe concentrations both resulted in increased cellular pigment contents and affected photosynthesis vs. irradiance parameters. If these results also apply to natural Crocosphaera populations, anthropogenic CO2 enrichment could substantially increase global oceanic N2 and CO2 fixation, but this effect may be tempered by Fe availability. Possible biogeochemical consequences may include elevated inputs of new nitrogen to the ocean and increased potential for Fe and/or phosphorus limitation in the future high-CO2 ocean, and feedbacks to atmospheric pCO2 in both the near future and over glacial to interglacial timescales.

Description: Zircon is a common mineral in continental crustal rocks. As it is not easily altered in processes such as erosion or transport, this mineral is often used in the reconstruction of geological processes such as the formation and evolution of the continents. Zircon can also survive under conditions of the Earth’s mantle, and rare cases of zircons crystallizing in the mantle significantly before their entrainment into magma and eruption to the surface have been reported1,2,3. Here we analyse the isotopic and trace element compositions of large zircons of gem quality from the Eger rift, Bohemian massif, and find that they are derived from the mantle. (U–Th)/He analyses suggest that the zircons as well as their host basalts erupted between 29 and 24 million years ago, but fragments from the same xenocrysts reveal U–Pb ages between 51 and 83 million years. We note a lack of older volcanism and of fragments from the lower crust, which suggests that crustal residence time before eruption is negligible and that most rock fragments found in similar basalts from adjacent volcanic fields equilibrated under mantle conditions. We conclude that a specific chemical environment in this part of the Earth’s upper mantle allowed the zircons to remain intact for about 20–60 million years.

Description: THE Sierra Leone Rise, located in the east equatorial Atlantic, forms a discontinuous chain of seamounts as shallow as 2 km extending with a general NE–SW trend from near the Sierra Leone coast of Africa, to the St Paul fracture zone near the Mid-Atlantic Ridge (Fig. 1). The origin of this feature has remained a topic of discussion. Sheridan et al.1 have hypothesised that the Sierra Leone Rise is a volcanic structure formed at the beginning of the opening of the Atlantic in the early Cretaceous period. The twin features of the Sierra Leone and the Ceara Rises are probably of oceanic origin and were created 80 Myr ago or later in their present-day position with respect to Africa and South America2. The Atlantic ocean exhibits several similar aseismic structures which appear symmetrically oriented with respect to the mid-oceanic ridge, such as the Walvis–Rio Grande Rise and the Iceland Faeroes–Iceland Greenland Ridges. These structures are volcanic edifices having a composition similar to that found in their associated islands3–7. Deep sea drilling of the Ceara Rise8,9 penetrated a basaltic basement of the upper Cretaceous period (Maestrichtian) (Leg 39, Site 354). Similarly, a DSDP hole (Leg 41, Site 366) on the Sierra Leone Rise, penetrated sediments of the same period, without reaching basement10. We report here the discovery of alkali-rich volcanics in an area of the Sierra Leone Rise. The sediment overlying the rock fragments is aged ∼45 Myr.

Description: Scattered groups of these ancient fish may all stem from a single remote population. Coelacanths were discovered in the Comoros archipelago to the northwest of Madagascar in 1952. Since then, these rare, ancient fish have been found to the south off Mozambique, Madagascar and South Africa, and to the north off Kenya and Tanzania — but it was unclear whether these are separate populations or even subspecies. Here we show that the genetic variation between individuals from these different locations is unexpectedly low. Combined with earlier results from submersible and oceanographic observations1, 2, our findings indicate that a separate African metapopulation is unlikely to have existed and that locations distant from the Comoros were probably inhabited relatively recently by either dead-end drifters or founders that originated in the Comoros.

Description: As the complex interplay of forces in the ocean responds to climate change, the dynamics of global ocean circulation are shifting.

Description: Der 3. Fahrtabschnitt der 1. Reise des neuesten deutschen Forschungsschiffes Maria S. Merian führt in die Schlammvulkanprovinz des Golf von Cadiz. Hier sollen Untersuchungen von biogeochemischen Stoffumsätzen, Fluid- und Gas-Flüssen an spezifischen Ökosystemen wie anoxischen Lebensgemeinschaften und azooxanthellaten Steinkorallen durchgeführt werden. Die Fahrt, die in 2 Unterabschnitte geteilt ist, beginnt in Kiel gefolgt von einem Zwischenstopp in Cadiz (Spanien) und endet in Lissabon (Portugal). MSM- 1/3 ist eine multidisziplinäre Expedition mit biologischen, geologischen und hydrographischen Fragestellungen. Ein Teil der Untersuchungen wird im Rahmen des „Geotechnologien” Programms des BMBF und der DFG für den Schwerpunkt „Methan im Geo-/Biosystem” durch das am IFM-GEOMAR koordinierte und für das ebenfalls hier schwerpunktmäßig angesiedelte Programm COMET (Controls on methane fluxes and their climatic relevance in marine gas hydrate-bearing environments) durchgeführt. Ein weiterer Teil der Ausfahrt dient den Untersuchungen im Rahmen des FP-6 Programms der EU HERMES (Hotspot Ecosystem Research on the Margins of European Seas). Aus dem HERMES-Programm nehmen 6 Partner teil. Beide Forschungsvorhaben sind sehr umfangreich und in ihrer Thematik komplex. Es gibt neben der geographischen Orientierung auf das Gebiet des Golf von Cadiz eine Vielzahl von inhaltlichen, personellen und logistischen Verbindungen zwischen beiden Programmen. Golf von Cadiz: Geologischer Hintergrund Die Region des Golf von Cadiz hat eine sehr komplexe geologische Geschichte. Sie ist seit der Trias durch mehrere tektonische Phasen mit Extension, Kompression und Lateralverschiebungen gekennzeichnet. Während des Mesozoikums und frühen Känozoikums bildeten sich in diesem Gebiet Bruchzonen mit Halbgraben-Strukturen und Karbonatplattformen. Im Torton verlagerte sich der Gibraltar-Bogen nach Westen. Dadurch wurde der Golf von Cadiz zu einem Forearc-Becken, in das Olistostrome (Rutschmassen) hineinglitten. In diesem Ablagerungsmilieu, das sonst für Akkretionskeile charakteristisch ist, wurden die Sedimente des südiberischen und nordafrikanischen Kontinentalrandes der damaligen Tethys stark deformiert. Die Olistostrom-Bildung war im oberen Miozän beendet. Gleichzeitig nahm die Subsidenz des Gebietes zu, und es kam zur Ausbildung von mächtigen Abfolgen progradierender und aggradierender Vorschüttfächer. Die geodynamische Interpretation dieser tektonisch sehr komplexen Region ist bis heute kontrovers. Der Gibraltarbogen liegt am östlichen Ausläufer der Azoren-Gibraltar Transformstörung, die als transpressionelle Grenze der iberischen und afrikanischen Platte gesehen wird. Die NW-SE gerichtete Konvergenz dieser beiden Platten zeigt sehr langsame Relativbewegungen von nur 4 mm pro Jahr. Die Ergebnisse neuester geophysikalischer Untersuchungen weisen jedoch darauf hin, dass auch eine ostwärtige Subduktion unter den Gibraltar-Bogen die gegensätzlichen Beobachtungen tektonischer Phänomene aus dem Riffgebirge und der Bethischen Kordillere erklären kann. Eine westwärts gerichtete Gegenrotation erzeugt Krustendehnung und damit Subsidenz in der Alboran See, während die damit verbundene westwärtige Verlagerung des Gibraltar-Bogens eine kompressionelle Deformation des Atlantis-Akkretionskeiles bewirkt. Es ist zu erwarten, dass die aktive Subduktion im Golf von Cadiz einen starken Einfluss auf das natürliche Gefahrenpotential dieser Region ausübt. Sie muss beispielsweise als Ursache für das große Erdbeben von 1755 gesehen werden (Stärke 8.5), durch das und den nachfolgenden Tsunami schwere Schäden in Lissabon und im angrenzenden Küstengebiet des Golf von Cadiz verursacht wurden. Diese historischen Ereignisse sind ein gewichtiger Grund dafür, dass der Golf von Cadiz eine Schlüsselregion für Europäische Forschungsaktivitäten und instrumenteller Langzeitbeobachtungen im Rahmen der EU-Programme ESONET, HERMES und EuroSEIZE bildet. Aus den Ergebnissen verschiedener Expeditionen ergeben sich viele Hinweise auf weit verbreitete Fluidaustritte, Karbonatmounds mit Tiefwasserkorallen (Lophelia-Skelette), Kohlenwasserstoff-Gasaustritte und Schlammdiapirismus am portugiesischen, spanischen und marokkanischen Kontinentalrand des Golf von Cadiz. Diese Phänomene wurden als Indikatoren für die weit verbreitete Existenz von gasübersättigten Sedimenten und der Migration von Fluiden diffusiv durch die Sedimente oder advektiv entlang von tektonischen Störungen interpretiert.

Description: A SIMPLE model for continental basement structures at rifted continental margins comprises large fault blocks which trend approximately parallel to, and step down towards, the continental–ocean boundary (for example, see ref. 1). These blocks may be cut by faults which strike across the margin, and, in many theoretical discussions, are shown as being separated from the true oceanic crust by an intermediate zone (see transitional crust of Fig. 3, ref. 2). On many rifted margins these features are deeply buried by young sediments and cannot be stutied in detail. On Goban Spur (Fig. 1), a marginal plateau south-west of Ireland, the young sediment cover is abnormally thin, however, and we have been able to map in detail a 150 km wide continental basement fracture pattern of horsts and grabens using a simple seismic reflection system (160 inch3 air-gun and two-channel hydrophone array). We also suggest a location for the continent–ocean boundary between the Spur and Porcupine Abyssal Plain. There are few previously published data from Goban Spur relevant to our study, although valuable sampling3 and geophysical3–5 results have been obtained north and south of the area.