scholarly journals Tracing Mercury Pollution along the Norwegian Coast via Elemental, Speciation, and Isotopic Analysis of Liver and Muscle Tissue of Deep-Water Marine Fish (Brosme brosme)

2019 ◽  
Vol 53 (4) ◽  
pp. 1776-1785 ◽  
Author(s):  
Ana Rua-Ibarz ◽  
Eduardo Bolea-Fernandez ◽  
Amund Maage ◽  
Sylvia Frantzen ◽  
Monica Sanden ◽  
...  

2017 ◽  
Vol 123 (1-2) ◽  
pp. 279-285 ◽  
Author(s):  
Pierre Cresson ◽  
Morgane Travers-Trolet ◽  
Manuel Rouquette ◽  
Charles-André Timmerman ◽  
Carolina Giraldo ◽  
...  


Eos ◽  
2020 ◽  
Vol 101 ◽  
Author(s):  
Carolyn Wilke

Isotopic analysis indicates that mercury found in deep-sea organisms may have an origin in carrion from near the surface.



2006 ◽  
Vol 81 (2-3) ◽  
pp. 251-257 ◽  
Author(s):  
Diana L. Watters ◽  
Donna E. Kline ◽  
Kenneth H. Coale ◽  
Gregor M. Cailliet


2019 ◽  
Vol 198 ◽  
pp. 230-238 ◽  
Author(s):  
T. A. Davletshina ◽  
L. V. Shulgina ◽  
K. G. Pavel ◽  
I. V. Maltzev

Antimora microlepis is considered as a new object of deep-water fishery. Its body length in the catches of 2018 was 40–80 cm, on average 56 cm, weight — 570–5670 g, on average 2170 g. Water content of its meat was 81.6 % that is similar to the meat of cod (82.1 %) but lower than the water content for other deep-water fish species. The muscle tissue of А. microlepis is lowcalorie and distinguished by medium protein content (17.1 %) and low fat content (0.4 %). The proteins have standard number and ratio of essential amino acids, the index of ECB is 114.8 %. Among fatty acids of the meat lipids, PUFAs dominate (49.4 %), mainly omega-3 family, but their content does not exceed 0.2 g per 100 g of meat because of low fat content. The meat of A. microlepis could be a source of sodium and copper, these metals content in 100 g of muscle tissue satisfies the daily needs of human body by 14.1 % and 18.0 %, respectively. Because of high protein content and low fat content, the meat of A. microlepis can be considered as a dietary fish raw material for both general and specialized products.



2010 ◽  
Vol 61 (5) ◽  
pp. 365-381 ◽  
Author(s):  
Alexander Lukeneder ◽  
Eva Halásová ◽  
Andreas Kroh ◽  
Susanne Mayrhofer ◽  
Petr Pruner ◽  
...  

High resolution stratigraphy of the Jurassic-Cretaceous boundary interval in the Gresten Klippenbelt (Austria)The key objective of investigation of hemipelagic sediments from the Gresten Klippenbelt (Blassenstein Formation, Ultrahelvetic paleogeographic realm) was to shed light on environmental changes around the Jurassic-Cretaceous (J/K) boundary on the northern margin of the Penninic Ocean. This boundary is well exposed in a newly discovered site at Nutzhof. Around the critical interval including the boundary, this new outcrop bears a rich microplanktonic assemblage characterized by typical J/K (Tithonian/Berriasian) boundary faunas. The Nutzhof section is located in the Gresten Klippenbelt (Lower Austria) tectonically wedged into the deep-water sediments of the Rhenodanubian Flysch Zone. In Late Jurassic-Early Cretaceous time the Penninic Ocean was a side tract of the proto-North Atlantic Oceanic System, intercalated between the European and the Austroalpine plates. Its opening started during the Early Jurassic, induced by sea floor spreading, followed by Jurassic-Early Cretaceous deepening of the depositional area of the Gresten Klippenbelt. These tectonically induced paleogeographic changes are mirrored in the lithology and microfauna that record a deepening of the depositional environment from Tithonian to Berriasian sediments of the Blassenstein Formation at Nutzhof. The main lithological change is observed in the Upper TithonianCrassicollariaZone, in Chron M20N, whereas the J/K boundary can be precisely fixed at theCrassicollaria-Calpionellaboundary, within Chron M19n.2n. The lithological turnover of the deposition from more siliciclastic pelagic marl-limestone cycles into deep-water pelagic limestones is correlated with the deepening of the southern edge of the European continent at this time. Within the Gresten Klippenbelt Unit, this transition is reflected by the lithostratigraphic boundary between siliciclastic-bearing marl-limestone sedimentation in the uppermost Jurassic and lowermost Cretaceous limestone formation, both within the Blassenstein Formation. The cephalopod fauna (ammonites, belemnites, aptychi) and crinoids from the Blassenstein Formation, correlated with calcareous microfossil and nannofossil data combined with isotope and paleomagnetic data, indicate the Tithonian to middle Berriasian (Hybonoticeras hybonotumZone up to theSubthurmannia occitanicaZone; M17r-M21r). The succession of the Nutzhof section thus represents deposition of a duration of approximately 7 Myr (ca. 150-143 Ma). The deposition of the limestone, marly limestone and marls in this interval occurred during tectonically unstable conditions reflected by common allodapic material. Along with the integrated biostratigraphic, geochemical and isotopic analysis, the susceptibility and gamma-ray measurements were powerful stratigraphic tools and important for the interpretation of the paleogeographic setting. Two reverse magneto-subzones, Kysuca and Brodno, were detected within magnetozones M20n and M19n, respectively.



2012 ◽  
Vol 46 (14) ◽  
pp. 7836-7843 ◽  
Author(s):  
Jan Ove Bustnes ◽  
Katrine Borgå ◽  
Tim Dempster ◽  
Elisabeth Lie ◽  
Torgeir Nygård ◽  
...  


2012 ◽  
pp. 495-517 ◽  
Author(s):  
Vladimir N. Epov ◽  
Sylvain Berail ◽  
Christophe Pécheyran ◽  
David Amouroux ◽  
Olivier F. X. Donard


1988 ◽  
Vol 62 (01) ◽  
pp. 1-8 ◽  
Author(s):  
Ronald E. Martin

The utility of benthic foraminifera in bathymetric interpretation of clastic depositional environments is well established. In contrast, bathymetric distribution of benthic foraminifera in deep-water carbonate environments has been largely neglected. Approximately 260 species and morphotypes of benthic foraminifera were identified from 12 piston core tops and grab samples collected along two traverses 25 km apart across the northern windward margin of Little Bahama Bank at depths of 275-1,135 m. Certain species and operational taxonomic groups of benthic foraminifera correspond to major near-surface sedimentary facies of the windward margin of Little Bahama Bank and serve as reliable depth indicators. Globocassidulina subglobosa, Cibicides rugosus, and Cibicides wuellerstorfi are all reliable depth indicators, being most abundant at depths >1,000 m, and are found in lower slope periplatform aprons, which are primarily comprised of sediment gravity flows. Reef-dwelling peneroplids and soritids (suborder Miliolina) and rotaliines (suborder Rotaliina) are most abundant at depths <300 m, reflecting downslope bottom transport in proximity to bank-margin reefs. Small miliolines, rosalinids, and discorbids are abundant in periplatform ooze at depths <300 m and are winnowed from the carbonate platform. Increased variation in assemblage diversity below 900 m reflects mixing of shallow- and deep-water species by sediment gravity flows.



Author(s):  
D.E. Brownlee ◽  
A.L. Albee

Comets are primitive, kilometer-sized bodies that formed in the outer regions of the solar system. Composed of ice and dust, comets are generally believed to be relic building blocks of the outer solar system that have been preserved at cryogenic temperatures since the formation of the Sun and planets. The analysis of cometary material is particularly important because the properties of cometary material provide direct information on the processes and environments that formed and influenced solid matter both in the early solar system and in the interstellar environments that preceded it.The first direct analyses of proven comet dust were made during the Soviet and European spacecraft encounters with Comet Halley in 1986. These missions carried time-of-flight mass spectrometers that measured mass spectra of individual micron and smaller particles. The Halley measurements were semi-quantitative but they showed that comet dust is a complex fine-grained mixture of silicates and organic material. A full understanding of comet dust will require detailed morphological, mineralogical, elemental and isotopic analysis at the finest possible scale. Electron microscopy and related microbeam techniques will play key roles in the analysis. The present and future of electron microscopy of comet samples involves laboratory study of micrometeorites collected in the stratosphere, in-situ SEM analysis of particles collected at a comet and laboratory study of samples collected from a comet and returned to the Earth for detailed study.



Nature ◽  
2017 ◽  
Author(s):  
Laura Castells
Keyword(s):  


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