The Zn–Pb±Ag±Cu San Cristobal district is located 100 km east of Lima in the western cordillera of Peru. It is centred around the Chumpe intrusion and is composed of vein and carbonate replacement ore types. The main San Cristobal vein presents a paragenesis that can be divided into three stages: (a) an early wolframite–quartz–pyrite stage, (b) a quartz–base metal stage, and (c) a late quartz–carbonate–barite stage.
Fluid inclusions in quartz from the tungsten stage are biphase (LV) at room temperature and homogenise to the liquid phase between 146 and 257 °C. Their salinities range between 2.1 and 5.1 wt.% NaCl equiv. Rare inclusions contain an additional crystal of halite and have salinities of 46–54 wt.% NaCl equiv. Data of the first two stages show a decrease in homogenisation temperatures concomitant with a salinity decline. Fluid inclusions in quartz from the late stage homogenise at higher temperatures, between 252 and 323 °C, with salinities ranging between 4.6 and 6.7 wt.% NaCl equiv.
Hydrogen and oxygen isotope data indicate a two-stage evolution. Isotopic compositions of the fluid associated with the first two stages define a trend with constant δ18O values and decreasing δD values (δ18O=3.2‰ to 5.0‰ V-SMOW and δD=−60‰ to −112‰ V-SMOW), which is interpreted as mixing of a dominantly magmatic component with minor meteoric water that had equilibrated with the host rocks. This interpretation is supported by sulphur and lead isotopic data from previous studies. By contrast, the quartz–carbonate–barite stage bears isotopic characteristics defining a trend with a coupled decrease of δ18O and δD (δ18O=−8.1‰ to 2.5‰ V-SMOW and δD=−57‰ to −91‰ V-SMOW) and is explained by addition of meteoric water to the system and subsequent mixing with a less important magmatic component.
Different fluid origins are confirmed by laser ablation ICP-MS analyses of the triphase (LVH) and biphase (LV) primary inclusions. The concentrations of the major ore elements, i.e., W, Cu, Zn and Pb, decrease throughout the paragenesis; W, and to a lesser extent Cu, show significant variations, associated with a steep decrease in their concentration. The decreasing concentrations can be explained by mineral deposition and dilution by the meteoric fluid; differences in the rate of decrease indicate selective precipitation of W. Fluid inclusions of the quartz–carbonate stages show an abrupt increase in Ba and Sr concentrations. This is interpreted to reflect a higher volume of host rock silicate alteration, probably due to the increasing size of the fluid flow cell and is explained by the input of a third fluid of unknown origin. LA-ICP-MS analyses show that the fluids were already depleted in W and Cu before reaching the emplacement of carbonate replacement ore type, whereas Zn and Pb were still present in considerable amounts. This is again due to selective precipitation and is consistent with the interpretation that the economically interesting metals were dominantly introduced by magmatic fluids. 相似文献
A combined study using multi-radiometric dating and oxygen isotopic geothermometry was carried out for Mesozoic quartz syenite, alkali-feldspar granite and associated hydrothermal uranium mineralization at Dalongshan in the Middle-Lower Yangtze valley of east-central China. Radiometric dating of the quartz syenite yields a whole-rock Rb–Sr isochron age of 135.6±4.3 Ma, a zircon U–Pb isochron age of 132.9±2.2 Ma, and K–Ar ages of 126±2, 118±3 and 94±4 Ma for hornblende, biotite and orthoclase, respectively. The alkali-feldspar granite yields a whole-rock Rb–Sr isochron age of 117.3±3.3 Ma, a zircon U–Pb isochron age of 114.7±2.1 Ma, and K–Ar ages of 112±2, 109±3 and 88±4 Ma for hornblende, biotite and orthoclase, respectively. Oxygen isotope thermometry for both granites gives temperatures of 685 to 720, 555 to 580, 435 to 460 and 320 to 330 °C, for hornblende, magnetite, biotite and orthoclase respectively, when paired with quartz. The systematic differences among the ages by the different techniques on the different minerals are used to reconstruct the cooling history of the granite. The results yield rapid cooling rates of 27.4 to 58.6 °C/Ma from 800 to 300 °C in the early stage, but slow cooling rates of 6.3 to 7.2 °C/Ma from 300 to 150 °C in the late stage. The regular sequence of oxygen isotope temperatures for the different quartz–mineral pairs demonstrates that diffusion is a dominant factor controlling the closure of both radiometric and O isotopic systems during granite cooling. Pitchblende U–Pb isochron dating yields an uranium mineralization age of 106.4±2.9 Ma, which is younger than the age of the granite emplacement and thus considerably postdates the time of magma crystallization, but is close to the closure time of the K–Ar system in the biotite. This points to a close relationship between granite cooling and ore-forming process. It appears that hydrothermal mineralization took place in the stage of slow cooling of the granite, whereas the rapid cooling of the granite was concurrent with the migration of hydrothermal fluids along fault structures. Therefore, the activity of the ore-forming hydrothermal system is temporally dictated by the cooling rates of the granite and may lag about 25 to 30 Ma behind the crystallization timing of associated granite. 相似文献
Leveling surveys in 1923, 1976, and each year from 1983 to 1993 have shown that the east-central part of the Yellowstone caldera, near the base of the Sour Creek resurgent dome, rose at an average rate of 14±1 mm/year from 1923 to 1976 and 22±1 mm/year from 1976 to 1984. In contrast, no detectable movement occurred in the same area from 1984 to 1985 (-2±5 mm/year), and from 1985 to 1993 the area subsided at an average rate of 19±1 mm/year. We conclude that uplift from 1923 to 1984 was caused by: (1) pressurization of the deep hydrothermal system by fluids released from a crystallizing body of rhyolite magma beneath the caldera, then trapped beneath a self-sealed zone near the base of the hydrothermal system; and (2) aseismic intrusions of magma into the lower part of the sub-caldera magma body. Subsidence since 1985 is attributed to: (1) depressurization and fluid loss from the deep hydrothermal system, and (2) sagging of the caldera floor in response to regional crustal extension. Future intrusions might trigger renewed eruptive activity at Yellowstone, but most intrusions at large silicic calderas seem to be accommodated without eruptions. Overpressurization of the deep hydrothermal system could conceivably result in a phreatic or phreatomagmatic eruption, but this hazard is mitigated by episodic rupturing of the self-sealed zone during shallow earthquake swarms. Historical ground movements, although rapid by most geologic standards, seem to be typical of inter-eruption periods at large, mature, silicic magma systems like Yellowstone. The greatest short-term hazards posed by continuing unrest in the Yellowstone region are: (1) moderate to large earthquakes (magnitude 5.5–7.5), with a recurrence interval of a few decdes; and (2) small hydrothermal explosions, most of which affect only a small area (<0.01 km2), with a recurrence interval of a few years. 相似文献
