TY - JOUR
T1 - Tracing the sources and evolution processes of shale gas by coupling stable (C,H) and noble gas isotopic compositions: Cases from Weiyuan and Changning in Sichuan Basin, China.
AU - Cao, Chunhui
AU - Zhang, Mingje
AU - Li, Liwu
AU - Wang, Yuhui
AU - Li, Zhongping
AU - Du, Li
AU - Holland, Greg
AU - Zhou, Zheng
PY - 2020/4/9
Y1 - 2020/4/9
N2 - The source and thermal evolution history of organic matter for the Longmaxi shale are still debated. This study analyzed the molecular and stable carbon isotopic compositions of hydrocarbons (CH
4, C
2H
6, and C
3H
8) and CO
2 as well as the stable hydrogen isotopic compositions of methane, ethane, and noble gases (He, Ne, Ar, Kr, and Xe). Shale gases in the WY and CN areas show an extremely-low-wetness with CH
4 concentrations range from 93.41% to 99.01%. Non-hydrocarbon gases are mainly N
2 (0.22%–2.81%) and CO
2 (0.03%–1.35%). H
2S have not been detected. Different δ
13C
1 and δ
13C
2 values in WY and CN shale gases (WY: −37.3‰ to −35.0‰ and −40.3‰ to −38.3‰, CN: −29.8‰ to −26.3‰ and −35.3‰ to −32.7‰) and various carbon isotope-composition distribution patterns (δ
13C
1>δ
13C
2<δ
13C
3 and δ
13C
1>δ
13C
2>δ
13C
3) of hydrocarbons indicate a complex evolution process. WY shale gases include more oil-cracking gas than CN shale gases, suggesting WY shale gases more like come from Type I-II organic matter. In shale gas systems, methane content and δ
13C
1 ratios vary with the degree of thermal evolution, so the origin of shale gas cannot be determined using carbon isotope data alone. The wide range of δ
13C
CO2 values (−8.9‰ to −0.8‰) and N
2/
40Ar ratios (20.8–165.1) suggests multiple origins of the gases. Emeishan mantle plume provides the source of heat for some thermo-genic gas. Noble gas isotopic compositions (
3He/
4He: 0.001Ra to 0.019Ra) indicate air and crustal origins with no significant contribution from the mantle.
40Ar/
36Ar ratios (1194.3–4604.5) are consistent with the age of Longmaxi strata calculated by accumulative effect of Ar isotope. The shale gas humidity, carbon isotope ratios, and the carbon isotope-composition distribution patterns may contain information indicating the shale gas sweet spot.
AB - The source and thermal evolution history of organic matter for the Longmaxi shale are still debated. This study analyzed the molecular and stable carbon isotopic compositions of hydrocarbons (CH
4, C
2H
6, and C
3H
8) and CO
2 as well as the stable hydrogen isotopic compositions of methane, ethane, and noble gases (He, Ne, Ar, Kr, and Xe). Shale gases in the WY and CN areas show an extremely-low-wetness with CH
4 concentrations range from 93.41% to 99.01%. Non-hydrocarbon gases are mainly N
2 (0.22%–2.81%) and CO
2 (0.03%–1.35%). H
2S have not been detected. Different δ
13C
1 and δ
13C
2 values in WY and CN shale gases (WY: −37.3‰ to −35.0‰ and −40.3‰ to −38.3‰, CN: −29.8‰ to −26.3‰ and −35.3‰ to −32.7‰) and various carbon isotope-composition distribution patterns (δ
13C
1>δ
13C
2<δ
13C
3 and δ
13C
1>δ
13C
2>δ
13C
3) of hydrocarbons indicate a complex evolution process. WY shale gases include more oil-cracking gas than CN shale gases, suggesting WY shale gases more like come from Type I-II organic matter. In shale gas systems, methane content and δ
13C
1 ratios vary with the degree of thermal evolution, so the origin of shale gas cannot be determined using carbon isotope data alone. The wide range of δ
13C
CO2 values (−8.9‰ to −0.8‰) and N
2/
40Ar ratios (20.8–165.1) suggests multiple origins of the gases. Emeishan mantle plume provides the source of heat for some thermo-genic gas. Noble gas isotopic compositions (
3He/
4He: 0.001Ra to 0.019Ra) indicate air and crustal origins with no significant contribution from the mantle.
40Ar/
36Ar ratios (1194.3–4604.5) are consistent with the age of Longmaxi strata calculated by accumulative effect of Ar isotope. The shale gas humidity, carbon isotope ratios, and the carbon isotope-composition distribution patterns may contain information indicating the shale gas sweet spot.
U2 - 10.1016/j.jngse.2020.103304
DO - 10.1016/j.jngse.2020.103304
M3 - Article
VL - 78
JO - Journal of Natural Gas Science and Engineering
JF - Journal of Natural Gas Science and Engineering
SN - 1875-5100
M1 - 103304
ER -