Isotopic age determinations of crystalline rocks of the Upper Harz Mountains,Germany     

Dr. Albrecht Baumann  Prof. Dr. Borwin Grauert  Dr. Sabine Mecklenburg  Dr. Roland Vinx 《International Journal of Earth Sciences》1991,80(3):669-690

Dating of crystalline rocks occurring in the Upper Harz Mountains was carried out by means of U-Pb isotope investigations on zircons and sphene as well as by Rb-Sr isotope measurements on whole-rock samples and biotites.U-Pb data of euhedral and rounded, detrital zircons of the allochthonous block of the Ecker gneiss point to an age (upper intercept) of the source area of the predominantly metasedimentary rocks of about 1.6 Ga or older. The lower intercept indicates a possible metamorphic event at ca. 560 Ma in the Ecker gneiss or in the source rock of the zircons of this complex. The concordant data point of a sphene fraction from a metavolcanic sample documents contact metamorphic influence on the Ecker gneiss by the Variscan intrusions of the Upper Harz Mountains.Emplacement of the intrusions of the Harzburg gabbronorite and the Brocken and Oker granites occurred contemporaneously 293–297 Ma ago within the analytical error limits. This points to a common geotectonic cause of the ascent of the magmas. Uplift of the Ecker gneiss block, now squeezed in between Harzburg gabbronorite and Brocken granite, was connected to these processes.The mineral ages of the plutonites are close to the intrusion ages indicating fast cooling processes in shallow crustal levels.

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Zusammenfassung Eine altersmäßige Einstufung der im Oberharz vorkommenden kristallinen Gesteine wurde durch U-Pb-Isotopenuntersuchungen an Zirkonen und Titanit sowie Rb-Sr-Isotopenmessungen an Gesamtgesteinsproben und Biotiten durchgeführt.U-Pb-Daten von idiomorphen und runden, detritischen Zirkonen der allochthonen Eckergneis-Scholle deuten auf ein Alter des Ursprungsgebietes der weitgehend metasedimentären Gesteine von etwa 1. 6 Ga oder älter hin und sie weisen ferner auf ein mögliches Metamorphose-Ereignis vor rund 560 Ma im Eckergneis oder im Liefergestein der Zirkone des Eckergneises hin. Der konkordante Datenpunkt bei ca. 295 Ma einer Titanit-Fraktion aus einer Metavulkanit-Probe dokumentiert die kontaktmetamorphe Beeinflussung des Eckergneises durch die variskischen Intrusionen des Oberharzes.Die Platznahme der Intrusionen der Gesteine des Harzburger Gabbronorit-Massivs sowie des Brokken- und Oker-Granits erfolgten innerhalb der analytischen Fehlergrenzen zeitgleich vor 293–295 Ma. Dies deutet auf eine gemeinsame geotektonische Ursache des Aufdringens der Magmen. Damit verbunden war der Aufstieg der Eckergneis-Scholle, die jetzt zwischen Harzburger Gabbronorit und Brockengranit »eingeklemmt« ist.Mineralalter der Plutonite liegen nahe bei den Intrusionsaltern und weisen auf rasche Abkühlungsvorgänge in seichtem Krustenniveau hin.

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Résumé Des mesures d'âge ont été effectuées sur des roches cristallines de l'Oberharz par les méthodes de l'U-Pb sur zircon et sphène et du Rb-Sr sur roches totales et sur biotites. La méthode U-Pb, appliquée aux zircons idiomorphes et détritiques arrondis de l'écaille allochtone des gneiss d'Ecker, fournit un âge (intersection supérieure) d'environ 1,6 Ga au moins pour la source des matériaux surtout métasédimentaires. L'intersection inférieure indique la possibilité d'un événement métamorphique à ± 560 Ma soit dans les gneiss d'Ecker, soit dans les roches-sources de leurs zircons. Un résultat concordant à ± 295 Ma fourni par le sphène d'une métavolcanite enregistre l'action du métamorphisme de contact engendré dans les gneiss d'Ecker par les intrusions varisques.La mise en place des intrusions du massif gabbronoritique du Harzburg et celle des granite de Brocken et d'Ocker ont été contemporaines: âges de 293 à 297 Ma, compris dans l'intervalle d'approximation des mesures. Ce résultat est en faveur d'une même cause géotectonique pour l'ascension de ces magmas. C'est en relation avec ce processus que s'est produit le soulèvement de l'écaillé des gneiss d'Ecker, actuellement coincée entre le gabbro du Harzburg et le granite de Brocken.Les âges minéraux des plutons sont voisins des âges d'intrusion, ce qui indique un refroidissement rapide dans un niveau crustal peu profond.

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Surface studies of asteroids with the Faint Object Camera of the Space Telescope     

Hans Josef Schober  Rudolf Albrecht 《Earth, Moon, and Planets》1980,22(2):175-175

Minor planets have been observed in the last few years for physical properties using photometry, polarimetry and IR-radiometry. Using the Faint Object Camera (FOC) of the Space Telescope (ST) it will be possible for the first time to observe a large number of asteroids with direct imaging systems.We propose to use the FOC with high resolution mode to examine minor planets with respect to (a) diameters and shapes, (b) surface and detail studies, (c) densities and (d) possible binary nature of selected asteroids.Paper presented at the European Workshop on Planetary Sciences, organised by the Laboratorio di Astrofisica Spaziale di Frascati, and held between April 23–27, 1979, at the Accademia Nazionale del Lincei in Rome, Italy.  相似文献   

Molecular characterization of organic matter in sediments from the Keg River formation (Elk Point group), western Canada sedimentary basin     

A. Behrens  H. Wilkes  P. Schaeffer  H. Clegg  P. Albrecht   《Organic Geochemistry》1998,29(8):1905-1920

Distributions of free and sulfur-bound biomarkers in organic-rich sediments from the lower and upper Keg River formation (Elk Point group, western Canada) reveal deposition of these sediments under reducing conditions, in agreement with the geological data. The predominance of aryl isoprenoids of Chlorobiaceae origin indicates that photic zone anoxia occurred during time of deposition. A series of novel aryl isoprenoids with a carboxylic acid function was identified by GC–MS and the structure of the predominant 3-methyl-5-(2′,3′,6′-trimethylphenyl)pentanoate was proven by synthesis of an authentic standard. The occurrence of these acids gives evidence that oxidative breakdown at least partially accounts for the diagenetic fate of aromatic carotenoids. Li/EtNH₂ desulfurization of two kerogen concentrates yielded only low amounts of sulfur-bound hydrocarbons, and suggests that either sulfur sequestration was not a predominant process or, more probably, that a major part of the hydrocarbons, initially sulfurized, were released upon maturation, giving further evidence that (poly)sulfide bonds are cleaved at relatively low levels of thermal stress.  相似文献   

Evolution and composition of the lithospheric mantle underneath the western Arabian peninsula: constraints from Sr−Nd isotope systematics of mantle xenoliths     

Friedhelm Henjes-Kunst  Rainer Altherr  Albrecht Baumann 《Contributions to Mineralogy and Petrology》1990,105(4):460-472

On the basis of their textures and mineral compositions spinel-peridotite xenoliths of the Cr-diopside group (group I) from Cenozoic volcanic fields of Arabia can be classified into different subtypes. Type IA is of lherzolitic to harzburgitic composition; mineral compositions are similar to those of group I mantle xenoliths from worldwide occurrences. Type IB xenoliths have lherzolitic to wehrlitic compositions; Mg/(Mg+Fe) ratios of the clinopyroxenes (0.862–0.916) and olivines (0.872–0.914) are similar too or slightly lower than those of typical IA minerals. Texturally, type IB xenoliths are distinguished from type IA rocks by the presence of intragranular spinel, intragranular relict Cr-pargasite, and subordinate intergranular Ba-phlogopite (11.1% BaO). The hydrous minerals in type IB xenoliths are interpreted to document an earlier metasomatism 1 which did not affect type IA lithospheric mantle. Subsequent recrystallization caused the partial replacement of Cr-pargasite in type IB materials and resulted in the formation of less hydrous mineral assemblages. Some of the type IA xenoliths are characterized by secondary intergranular amphibole which must have formed recently. The absence or presence of this intergranular amphibole is used to distinguish an anhydrous subtype IA1 from a hydrous subtype IA2. Type IB xenoliths may also contain secondary intergranular amphibole (similar to the one in subtype IA2) or they contain abundant formermelt patches now consisting of glass and phenocrysts of olivine, clinopyroxene, amphibole, and spinel. The secondary intergranular amphiboles and the former melt patches, both are interpreted as results of a second metasomatism (metasomatism 2). In their trace element and isotopic characteristics, type IA1 and type IA2 clinopyroxenes do not exhibit any systematic differences. Furthermore, type IA2 clinopyroxenes are in Sr isotopic disequilibrium with intergranular amphiboles. This suggests that type IA2 clinopyroxenes were not modified during the second metasomatism 2. All type IA clinopyroxenes have low Sr contents (100 ppm); most of them show Sm/Nd ratios higher than inferred for bulk earth. In their ⁸⁷Sr/⁸⁶Sr and ¹⁴³Nd/¹⁴⁴Nd ratios, type IA clinopyroxenes exhibit a large spread from 0.70226–0.70376 and from 0.51375–0.51251, respectively. Highly variable Sr/Nd ratios (5.0–79.3) and variable T_UR and T_CHUR model age relationships require different evolutions of the respective mantle portions. Nevertheless, all but two type IA clinopyroxenes form a linear array in a Sm–Nd isochron diagram which probably can not be explained by mixing. If taken as an isochron the slope of the array corresponds to an age of around 700 Ma. The mean initial _Nd of 5.8±1.7 (1) is similar to values for juvenile Pan-African (i.e. 850–650 Ma old) crust of the Arabian-Nubian shield. It is suggested that type IA lithospheric mantle and the juvenile Pan-African crust are two counterparts fractionated from a common source during the earlier stages of the Pan-African. Type IB clinopyroxenes have high Sr contents (200 ppm), variable Sr/Nd ratios (9–111) and Sm/Nd ratios generally below that inferred for bulk earth, and show a small spread in their Sr and Nd isotopic compositions (0.70299–0.70318 and 0.51285–0.51278, respectively). In a Sm–Nd isochron diagram the data points form a linear, horizontal array indicating a close-to-zero age for the earlier metasomatism 1 and suggesting a close genetic relationship to mantle processes related to the formation of the Red Sea.  相似文献   

In Memoriam     

Albrecht Unsöld 《Solar physics》1971,17(1):3-5

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Environmental heterogeneity predicts species richness of freshwater mollusks in sub-Saharan Africa     

T. Hauffe  R. Schultheiß  B. Van Bocxlaer  K. Prömmel  C. Albrecht 《International Journal of Earth Sciences》2016,105(6):1795-1810

Species diversity and how it is structured on a continental scale is influenced by stochastic, ecological, and evolutionary driving forces, but hypotheses on determining factors have been mainly examined for terrestrial and marine organisms. The extant diversity of African freshwater mollusks is in general well assessed to facilitate conservation strategies and because of the medical importance of several taxa as intermediate hosts for tropical parasites. This historical accumulation of knowledge has, however, not resulted in substantial macroecological studies on the spatial distribution of freshwater mollusks. Here, we use continental distribution data and a recently developed method of random and cohesive allocation of species distribution ranges to test the relative importance of various factors in shaping species richness of Bivalvia and Gastropoda. We show that the mid-domain effect, that is, a hump-shaped richness gradient in a geographically bounded system despite the absence of environmental gradients, plays a minor role in determining species richness of freshwater mollusks in sub-Saharan Africa. The western branch of the East African Rift System was included as dispersal barrier in richness models, but these simulation results did not fit observed diversity patterns significantly better than models where this effect was not included, which suggests that the rift has played a more complex role in generating diversity patterns. Present-day precipitation and temperature explain richness patterns better than Eemian climatic condition. Therefore, the availability of water and energy for primary productivity during the past does not influence current species richness patterns much, and observed diversity patterns appear to be in equilibrium with contemporary climate. The availability of surface waters was the best predictor of bivalve and gastropod richness. Our data indicate that habitat diversity causes the observed species–area relationship, and hence, that environmental heterogeneity is a principal driver of freshwater mollusk richness on a continental scale.  相似文献   

Hospital Laundry Wastewater Disinfection with Catalytic Photoozonation     

Lourdes Teresinha Kist  Caroline Albrecht  Ênio Leandro Machado 《洁净——土壤、空气、水》2008,36(9):775-780

Wastewater production in a hospital laundry and the treatment of the most critical wastewater stream, are assessed. Hospital laundry wastewaters are hazardous to the environment due to their high pollutant concentrations and the chemicals added during the clothes washing process. Heterogeneous photocatalysis with UV, O₃ and TiO₂ and their possible combinations were used for disinfection purposes. A ramp‐type reactor was used for TiO₂ (P25 Degussa) fixation and for photochemical diffusion of the ozonized air. After assessing 5‐day biological oxygen demand, chemical oxygen demand, pH, turbidity, and surfactant content, and checking for the presence of thermotolerant coliforms and Escherichia coli, it was concluded that UV/O₃/TiO₂ was the best process/combination, yielding a 100% disinfection rate and a microbiological inactivation of 0.5070 min^–1 for E. coli and of 0.5505 min^–1 for thermotolerant coliforms.  相似文献   

New Observing Opportunities in the Far‐Infrared and Submillimeter Range     

Albrecht Poglitsch  Eckard Sturm  Jürgen Stutzki 《Astronomische Nachrichten》2005,326(7):575-588

F01 CONDOR – 1.4 THz Hetrodyne Receiver for APEX and for GREAT on SOFIA F02 FLASH – a First Light APEX Submillimeter Heterodyne instrument F03 GREAT – The German first light heterodyne instrument for SOFIA F04 CHAMP+ – A powerfull submillimeter array for the APEX telescope F05 The JamesWebb Space Telescope (JWST) and its Mid Infrared Instrument (MIRI) F06 CHARM – a Compact Heterodyne Array Receiver Module for KOSMA with Scalable Fully Reflective Focal Plane Array Optics F07 Science with Herschel‐PACS F08 CI/CO Mapping of IC 348 & Cepheus B using SMART on KOSMA F09 The warm and dense interstellar medium observed with Herschel F10 Intelligent Detectors – On‐Board Data Reduction for Future Missions F11 The Herschel Photodetector Array Camera & Spectrometer PACS F12 Why Astromineralogy Should Care about the Far‐infrared Range F13 ESI: A European Imaging Far‐Infrared Spectrometer for the Japanese SPICA space observatory F14 STAR – A 16 Pixel Terahertz Array Receiver for SOFIA F15 FIFI LS, a Field‐Imaging Far‐Infrared Line‐Spectrometer for SOFIA F16 Characterization of high‐ and low‐stressed Ge:Ga array cameras for Herschel's PACS instrument F17 Herschel / PACS Guaranteed Time Programs at MPIA F18 NANTEN2: CI and mid‐J CO surveys of clouds and galaxies of the southern sky  相似文献   

The Far‐Infrared Emission of Galaxies     

Carsten Kramer  Albrecht Poglitsch  Jürgen Stutzki  Andreas Eckart 《Astronomische Nachrichten》2005,326(7):523-534

C01 Study of local infrared bright galaxies with HERSHCEL‐PACS C02 PDR modeling of the COBE Far‐Infrared data of the Milky Way C03 MAMBO observations of BzK‐selected vigorous starburst galaxies at z ∼ 2 C04 Starburst galaxies in the far‐infrared. Modelling the line, PAH and dust continuum emission C05 The SED from isothermal clouds C06 PDRs in M83 and M51: The road to HIFI/Herschel and SOFIA C07 Large Scale Mapping of Molecular Gas in the Vicinity of 30 Doradus in the Large Magellanic Cloud C08 Modelling far‐infrared emission from dust in gas‐rich galaxies C09 [CII]/CO(1‐0) Line Ratio at low Metallicities C10 Gas, Stars and Dust in the Spiral Arms of M51 C11 The ISOPHOT 170 micron Serendipity Survey (ISOSS) catalog of optically identified galaxies C12 Spitzer Images of M33: A Probe to Radio‐FIR Correlation C13 Observations of far‐infrared emission from dust in gas‐rich galaxies C14 Dust and Gas in Nearby Galaxies: First Results from SINGS and THINGS C15 Sequential Starburst in Arp220?  相似文献   

The impact of diagenetic fluid–rock reactions on Rotliegend sandstone composition and petrophysical properties (Altmark area, central Germany)     

Dieter Pudlo  Viktor Reitenbach  Daniel Albrecht  Leonhard Ganzer  Ulrich Gernert  Joachim Wienand  Bernd Kohlhepp  Reinhard Gaupp 《Environmental Earth Sciences》2012,67(2):369-384

In the framework of the German R&D joint project CLEAN (CO₂ large-scale enhanced gas recovery in the Altmark natural gas field), Rotliegend reservoir sandstones of the Altensalzwedel block in the Altmark area (Saxony-Anhalt, central Germany) have been studied to characterise litho- and diagenetic facies, mineral content, geochemical composition, and petrophysical properties. These sands have been deposited in a playa environment dominated by aeolian dunes, dry to wet sand flats and fluvial channel fills. The sediments exhibit distinct mineralogical, geochemical, and petrophysical features related to litho- and diagenetic facies types. In sandstones of the damp to wet sandflats, their pristine red colours are preserved and porosity and permeability are only low. Rocks of the aeolian environment and most of the channel fill deposits are preferentially bleached and exhibit moderate to high porosity and permeability. Although geochemical element whole rock content in these rocks is very similar, element correlations are different. Variations in porosity and permeability are mainly due to calcite and anhydrite dissolution and differences in clay coatings with Fe-bearing illitic-chloritic composition exposed to the pore space. Moreover, mineral dissolution patterns as well as compositions (of clays and carbonate) and morphotypes of authigenic minerals (chlorite, illite) are different in red and bleached rocks. Comparison of the geochemical composition and mineralogical features of diagenetically altered sandstones and samples exposed to CO₂-bearing fluids in laboratory batch experiments exhibit similar character. Experiments prove an increase in wettability and water binding capacity during CO₂ impact.  相似文献