The conditions and timing of quartz cementation in the Brent sandstones in the Hild Field, Norwegian North Sea, were constrained on the basis of oxygen isotope microanalysis and fluid inclusion microthermometry combined with optical and cathodoluminescence (CL) microscopy studies. Samples of the Tarbert and the Ness Formations were investigated in three different wells, presently lying at 3.8–4.3 km subsea and at 140–155°C. Quartz cement is present in all wells. Abundance varies from 3% to 26%, and tends to increase with depth of burial. Two distinct, separate episodes of quartz cementation, referred to as Q1 and Q2, are readily distinguished by CL microscopy. The two episodes are also recognized in the bimodal distribution of fluid inclusion temperatures and oxygen isotope microanalyses. The data indicate that Q1 quartz formed in the Early Tertiary (65–35 Ma) at 95–110°C and 2.3–3.0 km burial depth, and that Q2 mainly precipitated in the Oligocene–Miocene (40–10 Ma) at 125–135°C and 3.1–3.7 km. Q1 quartz precipitation follows the onset of overpressuring in the reservoir, while precipitation of Q2 seems to slightly precede and accompany the main phase of oil filling (35–10 Ma). Secondary ion mass spectrometry (SIMS) oxygen isotope microanalyses yield δ 18O values ranging from 17‰ to 25‰, averaging 23±2‰ for Q1 and 19.5±1.5‰ for Q2. Calculated δ 18O values of quartz-forming waters are similar for Q1 and Q2, ranging from 1‰ to 3‰, and are similar to the δ 18O value (≈2‰) of present-day formation water in the reservoir. Quartz cementation in the Brent reservoir of the Hild Field occurred during deep burial, at high temperature, from evolved 18O-rich basinal water most likely derived from the Viking Graben. Two episodes of enhanced quartz precipitation are recorded around 100°C and 130°C. No evidence was found for any significant contribution of 18O-depleted Jurassic meteoric water and/or low temperature precipitation of quartz cement.
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