Sulfur isotopic composition of gas-phase organic sulfur compounds provides insights into the thermal maturation of organic-rich rocks. (15th August 2019)

• Record Type: Journal Article
• Authors: Amrani, Alon; Rosenberg, Yoav Oved; Meshoulam, Alexander; Said-Ahmad, Ward; Turich, Courtney; Luu, Nathalie; Jacksier, Tracey; Stankiewicz, Artur; Feinstein, Shimon; Shurki, Avital
• Is Part Of: Geochimica et cosmochimica acta. Volume 259(2019)
• Page Start: 91
• Page End: 108
• Publication Date: 2019-08-15
• Subjects: Compound specific sulfur isotope -- Natural gas -- Sour -- Pyrolysis -- Ghareb Formation -- Thiols -- Misotope exchange; Geochemistry -- Periodicals; Meteorites -- Periodicals; Géochimie -- Périodiques; Météorites -- Périodiques; Geochemie; Astrochemie; Electronic journals; 551.905
• DOI: 10.1016/j.gca.2019.05.042
• Languages: English
• ISSNs: 0016-7037

Abstract

Abstract: Volatile and gas phase organic sulfur compounds (VOSCs) are important components in subsurface reservoir fluids and despite their relatively low concentrations, can provide important information about organic matter origin, diagenetic transformation, thermal maturation, and oil and gas generation, expulsion, and migration. We present an approach for the utilization of VOSC concentration and compound specific S isotopes ratio (δ 34 S) data as a new geochemical tool to study natural gas origin and formation. We studied the formation pathways of VOSCs, their δ 34 S values, and interaction with an organic-rich sedimentary rock (or 'source rock') from the Ghareb Formation (Type II-S kerogen) deposited in an upwelling marine environment. The immature source rock was subjected to laboratory controlled thermal maturation. We used a semi-open, non-isothermal pyrolysis system heated between 200 and 440 °C, and analyzed the molecular composition and compound specific δ 34 S values of the evolved gases at various thermal maturity stages. Formation of VOSCs commenced at 206 °C, a temperature generally associated with less thermally mature systems, and typically before the onset of oil generation for similar organic-rich source rocks, allowing study of low thermal maturity conditions (∼0.3 %Roeq ). Overall, the VOSCs obtained had δ 34 S values similar to the bulk kerogen values (mostly within 4‰). However, thiol (or mercaptan) δ 34 S values closely followed those of H2 S (Δ 34 Sthiols-H2S = −1 ± 1‰) throughout the experiment. Ab-initio calculations for the S isotopic exchange between H2 S and thiols were close to the experimental observations. This suggests that thiols rapidly attained equilibrium with H2 S despite their very short residence time in the system (minutes to hours). Furthermore, throughout the experiment, the concentrations of the six different thiols were found to be proportional to the coexisting, concentration ratio of [H2 ]/[H2 S]. The proportionality factors of the 6 different thiols strongly correlate with reported heats of formation (ΔHf °), further supporting the notion that the generation of thiols in the system rapidly reached equilibrium. At pyrolysis temperatures up to 350 °C, δ 34 S and concentration values of other VOSCs produced in the gas phase, including sulfides and thiophenes, probably represent generation from S-containing moieties in kerogen and bitumen with limited interaction with co-existing H2 S. The reaction of hydrocarbons and H2 S to produce VOSCs is inversely correlated with thermal stability, i.e. thiols > sulfides > thiophenes. Therefore, the δ 34 S values, concentrations and distributions of VOSCs can be utilized as a proxy for reaction extent and formation mechanism of petroleum and H2 S, including primary generation by thermal maturation, or potentially other processes such as migration and thermochemical sulfate reduction. This work demonstrates a novel and useful geochemical tool to study the source and fate of natural gas in the subsurface.