Gas isotope reversals in fractured gas reservoirs of the western Canadian Foothills: Mature shale gases in disguise (Record no. 185590)

MARC details
000 -LEADER
fixed length control field 02623nab a2200205 4500
008 - CÓDIGOS DE INFORMACIÓN DE LONGITUD FIJA - INFORMACIÓN GENERAL
Campo de control de longitud fija 260224s2011 xxu
245 00 - TITULO
Título Gas isotope reversals in fractured gas reservoirs of the western Canadian Foothills: Mature shale gases in disguise
260 ## - PUBLICACION, DISTRIBUCION, ETC
Lugar de publicación, distribución, etc.
Nombre de publicador, distribuidor, etc.
Fecha de publicación, distribución, etc. ago. 2011
270 ## - FECHA DE CARGA
Fecha de carga 19/09/2011 ; 19/09/2011
300 ## - DESCRIPCION FISICA
Otra extensión 24 p. ; 1399-1422
520 ## - RESUMEN, ETC
Resumen Transcripción del resumen del autor. Isotopically reversed gases (13C methane > 13C ethane > 13C propane) occur in fractured mixed clastic-carbonate reservoirs of the Permian and the Triassic in the foothills at the western edge of the Western Canada sedimentary basin (WCSB). The 13C methane values (–42 to –24), gas dryness, and organic maturity (Ro > 2.2) are indicative of mature gases, and gas maturity generally increases with reservoir age and from the southeast to the northwest. The 13C ethane values range from –44 to –25, with the less negative values in isotopically normal gases to the northeast of the gas fields we studied. To explain the gas isotope reversals observed in the WCSB foothills, we adopt the concept of a closed-system shale, in which simultaneous cooking of kerogen, oil, and gas yields gas with light 13C ethane and heavy 13C methane. This gas was released from shales and trapped in fractured folds of brittle clastic-carbonate rocks during deformation and thrust faulting of the Laramide orogeny, creating some of the most prolific gas pools. These gases are actually mature shale gases. Local high abundances of H2S and CO2 are most likely the products of thermochemical sulfate reduction (TSR) reactions in anhydrite-rich interbeds and underbeds that admixed to the released shale gas during the tectonic event. No evidence exists that TSR is responsible for the isotope reversals. Variations in 13C ethane are likely caused by local differences in thermal history, the timing of gas release from shale, and the timing of the fault and fold development. Less negative 13C ethane values (resulting in isotopically normal gases) to the northeast of the fields and in the underlying Devonian carbonates likely reflect a more open shale system where the earliest generated gas was lost. We suggest that isotopic reversals are restricted to closed-system maturation, and that their magnitude may be related to the relative volume of gas retained in shales.
581 ## - ESTADO DE COLECCIÓN
Estado de colección 8
773 0# - CORRECCIÓN
Título AAPG Bulletin
Partes relacionadas 95
942 ## - DESC. DE MATERIAL
Tipo de item KOHA Artículo de Revista
100 1# - RESPONSABLE PERSONAL
Apellido, Nombre Tilley, Barbara
9 (RLIN) 51584
100 1# - RESPONSABLE PERSONAL
Apellido, Nombre McLellan, Scott
9 (RLIN) 51585
100 1# - RESPONSABLE PERSONAL
Apellido, Nombre Hiebert, Stephen
9 (RLIN) 51586
Holdings
Biblioteca propietaria Biblioteca actual Fecha de adquisición Inventario Total de préstamos Inventario Fecha de carga Tipo de item KOHA
Biblioteca Alejandro Angel Bulgheroni Biblioteca Alejandro Angel Bulgheroni 06/03/2026 200057679   200057679 06/03/2026 Artículo de Revista


Instituto Argentino del Petróleo y del Gas
Maipú 639 (C1006ACG) – Buenos Aires – Argentina
Tel: (54 11) 5277 IAPG (4274)
Lu - Vie 11 a 17 hs
Mail: biblio@iapg.org.ar


Copyright © 2026, Instituto Argentino del Petróleo y del Gas, todos los derechos reservados.

Protección de datos personales