RESERVOIR COMPLEXITY REVEALED BY STABLE ISOTOPE COMPOSITION OF PRODUCED GASES FROM HORN RIVER BASIN SHALES
HRB gases are dry, mature and thermogenic in origin and the mole fraction of methane in shale gas samples ranged from ~80 to 90%. Gases from the Muskwa and Otter Park Fms. are indistinguishable based on chemical composition; however Evie gases contained higher fractions of CO2. δ13Cmethane values for the Muskwa and Otter Park mud gases averaged -34.9‰ and -35.0‰ respectively but varied along ~2 km of horizontal sections from -35.5‰ to -34.5‰ in the Muskwa compared to -36.9‰ to -31.9‰ in the Otter Park. Lateral δ13Cmethane profiles in these adjacent formations imply large differences in the scale of heterogeneity of permeability within these two shale units.
δ13C time series of methane, ethane and propane show isotopic variations during gas production. Methane produced at early stages was generally enriched in 12C compared to gases sampled later in production. δ13Cmethane values of gas from the Muskwa, Otter Park and Evie ranged between ~ -38‰ and -28‰. δ13C of gas did not vary monotonically with production. Examples of non-reversal, partial and full isotope reversal are all observed in HRB gases produced from a given well. In general enrichment in 13C of methane was observed in shale gases after periods of well ‘shut-in’. We conclude that shale reservoirs are far more complicated than heretofore realized.