Abstract
A number of episyenite occurrences within the Neoproterozoic Bohus granite, southwestern Sweden, were investigated in order to elucidate their genesis and past associated fluid regimes. Fluid inclusion microthermometry and O–H isotope systematics integrated with information from detailed mineralogy reveal a paragenetic succession within individual episyenites, including: (1) albitization of plagioclase, accompanied by dissolution of quartz, with a vuggy feldspathic reservoir rock as a result; (2) resumed infilling and replacement of igneous Fe–Ti-phases by various phyllosilicates (muscovite, chlorite and/or illite)±hematite assemblages and quartz, due to rift-related reactivation and (3) sporadic argillitic alteration and precipitation of fracture calcite. Although sparse owing to later overprinting, there are a few remnants that provide arguments for the involvement of meteoric water, shifted to a more 18O-rich composition, during the initial stage of dissolution and albitization. The main vug-filling phase is proposed to be associated with the ingress of surface-derived fluids with negative δ18O values, during the regional thermal anomaly accompanying the development of the nearby Permo-Carboniferous Oslo Rift at ~250Ma. The fluids involved during this event show consistently a marked, but variable 18O-depletion and resemble the modern-day shield brines, with modal salinities of 11–24 wt.% NaCl eq., low NaCl/(NaCl+CaCl2) weight ratios and no discernible CO2. Even though no P–T path can be defined for this phase, the fluid pressure can be restricted to 0.3–0.8kbar and temperature to 160–280°C, assuming a sedimentary overburden of ~3km. An overall variability in the δ18O and δD data can mainly be ascribed to (1) precipitation from fluids affected by isotopic exchange with the host rock and/or sedimentary overburden under highly variable water/rock ratios, and to some extent with (2) varying degrees of partial re-equilibration during subsequent hydrothermal interaction at lower temperatures, as emphasized by the presence of fluid inclusions of suspected secondary origin in quartz.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.