Poorly crystalline carbonaceous matter in high grade metasediments: implications for graphitisation and metamorphic fluid compositions

Poorly crystalline carbonaceous matter was observed in chlorite to sillimanite grade metasediments from the Trois Seigneurs Massif, in contrast to other studies of carbon crystallinity which observed well crystallised graphite under upper greenschist facies conditions. Using transmission electron microscopy four types of carbon particle were identified; globular carbon, composite flakes, homogeneous flakes and crystalline graphite. Globular carbon and composite flakes are poorly crystalline microporous carbon. Homogeneous flakes decompose in the electron beam and are probably composed of heavy volatile hydrocarbons. Graphite is confined to samples from retrograde shear zones and often occurs with globular carbon. The lack of graphitisation in metasediments is probably a consequence of the microporous structure of the carbonaceous matter combined with low f _{O 2}. The preservation of carbonaceous matter in the Trois Seigneurs metasediments is not compatible with the metasediments having been externally buffered by a high X _H2_O fluid syn-metamorphism. An alternative hypothesis of internal buffering is preferred to explain the carbonaceous matter in the Trois Seigneurs metasediments.     

A Gill twin propeller-vane anemometer for flux measurements during moderate and strong winds

A wind velocity measuring system based on the Gill propeller anemometer is described. A method of calculating the vertical component, which allows for the non-cosine response and avoids the region of stall and nonlinear operation, is presented. A summary of the possible errors in Reynolds stress and drag coefficient estimates is given. A method of establishing the distance constant using field observations is presented. Finally, some preliminary results and some intercomparisons with other anemometers are described briefly.Now at the Institute of Ocean Sciences, Patricia Bay, B.C., Canada.     

Zn–Pb–Cu volcanic-hosted massive sulphide deposits: criteria for distinguishing brine pool-type from black smoker-type sulphide deposition

Eight Zn–Pb–Cu massive sulphide deposits that appear to have formed on the sea floor (seven in Spain, one in Tasmania) are believed to have been precipitated in brine pools, based on the salinities and temperatures of fluid inclusions in underlying stockworks. Comparing the geological features of these deposits with those of the Zn–Pb–Cu massive sulphide ores of the Hokuroku Basin, Japan, which have formed as mounds from buoyant fluids of low salinity, shows that brine pool deposits have: (1) potentially very large size and tonnage, and high aspect ratio, (2) higher Zn/Cu and Fe/Cu values, (3) no evidence of chimneys, (4) relatively abundant framboidal pyrite and primary mineral banding, (5) reduced mineral assemblages (pyrite-arsenopyrite/pyrrhotite), and minor or rare barite in the massive sulphide, (6) associated stratiform and/or vein carbonates, (7) relatively unimportant zone refining, (8) lack of vertical variation in sphalerite and sulphur isotopic compositions, and (9) evidence of local bacterial sulphate reduction. Application of these criteria to the Rosebery deposit in Tasmania, for which there are no fluid inclusion data, leads to the conclusion that the southern section was deposited as separate lenses in a brine-filled basin or basins. Other potential candidates include Brunswick no. 12 and Heath Steele (Canada), Woodlawn and Captains Flat (New South Wales), Hercules and Que River (Tasmania), and Tharsis and the orebodies at Aljustrel (Spain and Portugal). Recently published fluid inclusion data for Gacun (China) and Mount Chalmers (Queensland) suggest that not all ores deposited from highly saline fluids have reduced mineral assemblages.     

Petrology and geochemistry of sphalerite from the Cambrian VHMS deposits in the Rosebery-Hercules district,western Tasmania: Implications for gold mineralisation and Devonian metamorphic-metasomatic processes

Summary Sphalerite is the major ore mineral in the Zn-rich, volcanic-hosted massive sulphide deposits of western Tasmania. These deposits have been affected by regional metamorphism to upper greenschist facies, and associated tectonic deformation related to the Devonian Tabberabberan Orogeny. The southern end of the Rosebery deposit has undergone metasomatic replacement related to a post-orogenic Devonian granite intrusion.Sphalerite from VHMS deposits in the Rosebery district varies widely in colour, grain size and texture. Compositional variation of the sphalerites was studied for three purposes (1) to investigate effects of the Devonian overprinting, (2) to provide pressure (depth) estimates at the time of Fe-S-O replacement during the Devonian, and (3) to deduce the effect ofa _FeS(a _{S 2}) on gold deposition and subsequent remobilisation.Sphalerite from the Rosebery deposit shows an FeS range from 2.0 to 20.0 mole%, with a bimodal distribution; a mode of 16.0 mole% FeS was noted for the F(_J) lens where Devonian metasomatism prevailed, whereas a mode of 2.4–4.0 mol% FeS was found for the other lenses. Sphalerite from the Hercules deposit has a range of 2.0–10.0 mole% FeS, whereas sphalerite from the South Hercules deposit ranges from 4.0-12.0 mole% FeS. VHMS sphalerites also contain minor copper, manganese and cadmium.The bimodal distribution of FeS content in Rosebery sphalerite suggests that the primary VHMS mineralisation underwent at least two periods of post-depositional re-equilibration. The FeS content in sphalerite in equilibrium with hexagonal pyrrhotite and pyrite indicates that the Devonian replacement occurred at a pressure off 3.0 ± 0.5 kb, corresponding to 8.0 ± 0.1 km depth.The relationship between FeS content in sphalerite and gold grades at Rosebery, Hercules and South Hercules displays complex patterns that reflect either variations in the initial depositional conditions an the seafloor (pH, temperature anda _{S 2}), or later Devonian metamorphic and metasomatic recrystallisation.Zusammenfassung Zinkblende ist das dominierende Erzmineral in den Zn-reichen, in vulkanischen Gesteinen beheimateten, massiven Sulfidlagerstätten West-Tasmaniens. Diese Lagerstätten sind von einer Regionalmetamorphose der oberen Grünschieferfazies und einer assoziierten Deformation, die der devonischen Tabberabberan Orogenese zuzuschreiben ist, überprägt worden. Das Südende der Rosebery Lagerstätte ist von einer metasomatischen Verdrängung, die mit einer post-orogenen, devonischen Granitintrusion im Zusammenhang steht, erfaßt worden.Die Zinkblende von VHMS Lagerstätten des Rosebery Distriktes variiert weitgehend in ihrer Farbe, Korngröße und Textur. Die Variation der chemischen Zusammensetzung der Zinkblende wurde aus drei Gründen untersucht: (1) um die Effekte der devonischen Überprägung zu studieren, (2) um zu Abschätzungen des Druckes (Tiefe) zur Zeit der Fe-S-O Verdrängung während des Devons zu gelangen, und (3) um die Auswirkung von^aFeS (^aS2) auf die Goldablagerung und folgende Remobilisation abzuleiten.Der FeS Gehalt der Zinkblende der Rosebery Lagerstätte reicht von 2.0 bis 20.0 Mol%, mit einer bimodalen Verteilung; ein Maximum bei 16.0 Mol% FeS ist für die F(_J) Linse charakteristisch, wo devonische Metasomatose vorherrscht, während ein zweites Maximum bei 2.0–4.0 Mol% FeS bei den anderen Linsen festgestellt wurde. Der FeS Gehalt der Zinkblende der Süd-Hercules Lagerstätte reicht von 4.0 bis 12.0 Mol%. Die VHMS Zinkblenden führen auch untergeordnet Kupfer, Mangan und Cadmium.Die bimodale Verteilung des FeS Gehaltes in der Rosebery Zinkblende läßt vermuten, daß die VHMS Mineralisation, nach ihrer Bildung, von mindestens zwei Perioden der Reequilibrierung erfaßt worden ist. Der FeS Gehalt in der Zinkblende im Gleichgewicht mit hexagonalem Pyrrhotin und Pyrit weist darauf hin, daß die devonische Verdrängung bei einem Druck von 3.0 ± 0.5 kb, vergleichbar mit 8.0 ± 0.1 km Tiefe, stattgefunden hat.Der Zusammenhang des FeS Gehalt in der Zinkblende mit den Goldgehalten in Rosebery, Hercules und Süd-Hercules ist komplex und spiegelt entweder unterschiedliche, primäre Bildungsbedingungen am Meeresboden (pH, Temperatur und^aS₂), oder spätere, devonische metamorphe und metasomatische Rekristallisation wider.

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Petrologie und Geochemie der Zinkblende aus der kambrischen VHMS Lagerstätte im Roseberry-Hercules Distrikt, West-Tasmanien: Hinweise für Goldmineralisation und devonische, metamorphe-metasomatische Prozesse

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With 14 Figures     

Climatic forcing before,during, and after the 8.2 Kyr B.P. global cooling event

This paper attempts at full characterization of the unique global 8.2 Kyr B.P. cooling event. Significant atmospheric cooling started during 9.5–8.5 Kyr B.P. when the Sun was extremely quiet during three periods of ∼ 50–100 years. The flood of melt water in the N. Atlantic from glacial lakes during the demise of the Laurentide ice sheet, starting at ∼ 8.5 Kyr B.P., adds to the atmospheric cooling. Climatic forcing events occurred at 8.5 Kyr B.P., at 8.2 Kyr B.P. and finally at 8.06 Kyr B.P., leading to concurrent increases or decreases in the atmospheric Δ¹⁴C levels, completely consistent with the climatic forcing proposed here.     

Lewis Ponds, a hybrid carbonate and volcanic-hosted polymetallic massive sulphide deposit, New South Wales, Australia

The Lewis Ponds Zn–Pb–Cu–Ag–Au deposit, located in the eastern Lachlan Fold Belt, central western New South Wales, exhibits the characteristics of both volcanic-hosted massive sulphide and carbonate-hosted replacement deposits. Two stratabound massive to disseminated sulphide zones, Main and Toms, occur in a tightly folded Upper Silurian sequence of marine felsic volcanic and sedimentary rocks. They have a combined indicated resource of 5.7 Mt grading 3.5% Zn, 2.0% Pb, 0.19% Cu, 97 g/t Ag and 1.9 g/t Au. Main Zone is hosted by a thick unit of poorly sorted mixed provenance breccia, limestone-clast breccia and quartz crystal-rich sandstone, whereas Toms Zone occurs in the overlying siltstone. Pretectonic carbonate–chalcopyrite–pyrite and quartz–pyrite stringer veins occur in the footwall porphyritic dacite, south of Toms Zone. Strongly sheared dolomite–chalcopyrite–pyrrhotite veins directly underlie the Toms massive sulphide lens. The mineralized zones consist predominantly of pyrite, sphalerite and galena. Paragenetically early framboidal, dendritic and botryoidal pyrite aggregates and tabular pyrrhotite pseudomorphs of sulphate occur throughout the breccia and sandstone beds that host Main Zone, but are rarely preserved in the annealed massive sulphide in Toms Zone. Main and Toms zones are associated with a semi-conformable hydrothermal alteration envelope, characterized by texturally destructive chlorite-, dolomite- and quartz-rich assemblages. Dolomite, chlorite, quartz, calcite and sulphides have selectively replaced breccia and sandstone beds in the Main Zone host sequence, whereas the underlying porphyritic dacite is weakly sericite altered. Vuggy and botryoidal textures resulted from partial dissolution of the dolomite-altered sedimentary rocks and unimpeded growth of base metal sulphides, carbonate and quartz into open cavities. The intense chlorite-rich alteration assemblage, underlying Toms Zone, grades outward into a weak pervasive sericite–quartz assemblage with distance from the massive sulphide lens. Limestone clasts and hydrothermal dolomite at Lewis Ponds are enriched in light carbon and oxygen isotopes. The dolomite yielded ¹³C_VPDB values of –11 to +1 and ¹⁸O_VSMOW values of 6 to 16. Liquid–vapour fluid inclusions in the dolomite have low salinities (1.4–7.7 equiv. wt% NaCl) and homogenization temperatures (166–232°C for 1,000 m water depth). Dolomitization probably involved fluid mixing or fluid–rock interactions between evolved heated seawater and the limestone-bearing facies, prior to and during mineralization. ³⁴S_VCDT values range from 2.0 to 5.0 in the massive sulphide and 3.9 to 7.4 in the footwall carbonate–chalcopyrite–pyrite stringer veins, indicating that the hydrothermal fluid may have contained mamgatic sulphur and a component of partially reduced seawater. The sulphide mineral assemblages at Lewis Ponds are consistent with moderate to strongly reduced conditions during diagenesis and mineralization. Low temperature dolomitization of limestone-bearing facies in the Main Zone host sequence created secondary porosity and provided a reactive host for fluid-rock interactions. Main Zone formed by lateral fluid flow and sub-seafloor replacement of the poorly sorted breccia and sandstone beds. Base metal sulphide deposition probably resulted from dissolution of dolomite, fluid mixing and increased fluid pH. Pyrite, sphalerite and galena precipitated from a relatively low temperature, 150–250°C hydrothermal fluid. In contrast, Toms Zone was emplaced into fine-grained sediment at or near the seafloor, above a zone of focused up-flowing hydrothermal fluids. Copper-rich assemblages were deposited in the Toms Zone footwall and massive sulphide lenses in Main and Toms zones as the hydrothermal system intensified. During the D₁ deformation, fracture-controlled fluids within the Lewis Ponds fault zone and adjacent footwall volcanic succession remobilized sulphides into syntectonic quartz veins. Lewis Ponds is a rare example of a synvolcanic sub-seafloor hydrothermal system developed within fossiliferous limestone-bearing facies. The close spatial association between limestone, hydrothermal dolomite, massive sulphide and dacite provides a basis for new exploration targets elsewhere in New South Wales.Editorial handling: D. Lentz     

Radio emission from the Sun at 843 MHz

The Molonglo Observatory Synthesis Telescope (MOST) has recently been modified to permit observations of the Sun. With a collecting area of 18000 m², MOST makes high-sensitivity measurements in right-hand circular polarisation over a 3 MHz bandwidth at 843 MHz. The maximum baseline of the multi-element interferometer is 1600 m, so that one-dimensional spatial resolution as fine as 32 arc sec is available. A resistor array produces simultaneously a set of 64 beams separated by 22 arc sec, which may be offset electronically to cover the entire Sun in a few seconds. Observations may be made with a beam shape corresponding to either a multiplying or an adding interferometer. By exploiting the technique of Earth-rotation synthesis the telescope may be used to make two-dimensional maps of the Sun at the time of the austral solstice with a synthesized beamwidth of 43 × 110 arc sec. This paper describes the instrument and the procedures used to make various types of solar observations, and exhibits some of the first data collected.