In the upper greenschist to granulite grade rocks of the Willyama Supergroup at Broken Hill, Australia, earlier recognition of metamorphosed graded bedding in siliciclastic metasedimentary rocks led to interpretations of these rocks as deep-water turbidites. However, graded beds can also be deposited in shelfal environments below storm wave base. This study identified other tempestite features including wave oscillation ripples, hummocky cross-stratification and swaley cross-stratification indicating that deposition took place above the wave base of the larger storms.
Albitised metasedimentary rocks of the upper Thackaringa Group show structures such as swaley cross-stratification typical of shallow-water conditions above fair-weather wave base. Deposition of the Broken Hill Group commenced with muddy Allendale Metasediments conformable on the Thackaringa Group. The Ettlewood Calc-Silicate Member, originally a dolomitic, siliceous sediment, is interpreted as coastal sabkha indicating onset of a marine transgression. The Parnell Gneiss represents a volcanic or volcaniclastic interruption, heralding gradually increasing input of sand in the Freyers Metasediments reaching a maximum in middle Freyers Metasediments, followed by an abrupt reversion to mud, still influenced by wave action. An open marine shelf is interpreted, possibly 30 m deep (no more than 100 m) in the final stage of a developing rift. The Broken Hill Group terminated with the massive Hores Gneiss volcanic unit.
Sedimentation of the siliciclastic Sundown Group took place in similar conditions, commencing with a muddy interval overlying the Hores Gneiss. The shallowing produced by ~90 m thickness of volcanic/volcaniclastic Hores Gneiss was compensated by subsidence.
Paragon Group deposition commenced with substantial black mud, resulting from isolation from the sand supply and probably isolation from the sea. A fresh connection to the sea led first to the deposition of dolomitic carbonate (King Gunnia Calc-Silicate Member), then to deposition of parallel-laminated fine sand below wave base (upper Cartwrights Creek Metasediments), followed by ripple cross-laminated sand above wave base (Bijerkerno Metasediments). The Dalnit Bore Metasediments show abundant very thin graded silt–mud units possibly deposited below storm wave base, and thicker units of stacked wave oscillation ripples deposited above the wave base of larger storms.
The Broken Hill orebody is hosted by altered Broken Hill Group metasedimentary rocks deposited at water depths of ~30 m. Unless the ore fluid temperature was less than 150°C, it is likely that the orebody formed below the seafloor: at such shallow-water depths, the confining pressure would be inadequate to suppress boiling of hotter rising hydrothermal fluids. 相似文献
The Sorkhe-Dizaj orebody is located 32 km southeast of Zanjan within the Tarom subzone of the Alborz-Azarbaijan structural zone. It is hosted mainly in quartz monzonite-monzodiorite and, to a lesser extent, in volcanoclastic rocks. Mineralization occurs in the form of stockwork and veins, comprising predominantly magnetite and actinolite, with minor pyrite and chalcopyrite. Two generations of magnetite and apatite are inferred: the first as disseminations in the host rock and the second mainly as an alteration product of actinolite, secondary K-feldspar, silica, sericite, chlorite and epidote. Fluid inclusion studies were carried out on second-generation apatite, and late-stage quartz to understand the geochemical evolution of the ore-bearing fluids. Fluid inclusions are of three types, i.e. primary, secondary, and pseudo-secondary. These inclusions are liquid or vapour single-phase, two-phase rich in liquid or vapour, and three-phase. Homogenization temperatures of second-generation apatite are inferred to be between 209°C and 520°C (mostly between 290°C and 320°C), indicating salinities of 9.08–21.61 wt.% NaCl equiv. At 342°C, the δ18O values range from 9‰ to 11.32‰ for the second-generation magnetite associated with coeval apatite. Fluid inclusions in the late-stage quartz veins are inferred to have homogenized between 186°C and 263°C, with δ18O values ranging between 2.5‰ and 7.4‰ at 220°C. Oxygen isotopes in the late-stage carbonate veins have values of 3.28–6.14‰ at 100°C. These data in the late-stage veins imply introduction of a cooler, less saline, isotopically depleted fluid, probably meteoric water. Field observations, mineral parageneses, and fluid inclusion?+?oxygen isotope data suggest that the magnetite-apatite veins formed from a predominantly magmatic-derived fluid. Introduction of cooler meteoric water in the final stage of mineralization reduced δ18O values, facilitating precipitation of sulphides, quartz, and carbonate veins. 相似文献