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Abstract
DOI:10.1306/13371579St640398
Comparison of Oil
Generation
Kinetics Derived from Hydrous Pyrolysis and Rock-eval in Four-dimensional Models of the Western Canada Sedimentary Basin and Its Northern Alberta Oil Sands
Generation
Kinetics Derived from Hydrous Pyrolysis and Rock-eval in Four-dimensional Models of the Western Canada Sedimentary Basin and Its Northern Alberta Oil Sands
Debra K. Higley,1 Michael D. Lewan2
1U.S. Geological Survey, PO Box 25046 Denver, Colorado, 80225, U.S.A. (e-mail: [email protected])
2U.S. Geological Survey, PO Box 25046 Denver, Colorado, 80225, U.S.A. (e-mail: [email protected])
ACKNOWLEDGMENTS
This chapter benefited from reviews and comments by Lauri Burke, Nicholas Gianoutsos, and Margaret Ellis, all of the U.S. Geological Survey. The authors are indebted to Ben Grossberndt and staff at the Alberta Energy Resources Conservation Board Core Research Centre (Calgary, Alberta) and Steven G. Gloverand and staff at the Ministry of Energy, Mines and Petroleum Resources, Energy Data Centre (Victoria, British Columbia) for providing information and access to cores that were used in this study to compile composite samples of the major oil-prone source rocks.Any use of trade, product, or firm names is for descriptive purposes only and does not imply endorsement by the United States Government.
ABSTRACT
Four-dimensional petroleum system models within the Western Canada sedimentary basin were constructed using hydrous pyrolysis (HP) and Rock-Eval (RE) kinetic parameters for six of the major oil-prone source rocks in the basin. These source rocks include the Devonian Duvernay Member of the Woodbend Group; Devonian-Mississippian Exshaw Formation; Triassic Doig Formation; Gordondale Member; Poker Chip A shale, both of the Jurassic Fernie Group; and Ostracod Zone of the Lower Cretaceous Mannville Group. The Mannville Group coals also contributed oil to the oil sands (Higley et al., 2009) but are excluded herein because HP kinetics were used for both models with identical results.
The locations of oil migration flowpaths are identical for the HP and RE models, with the exception of an earlier onset of
generation
and migration shown with the HP
model
. Both models show that the oil sands are located at focal points of the petroleum migration pathways. The principal differences between the models are the onset and extent of oil
generation
from the Jurassic Fernie source rocks (Gordondale Member and Poker Chip A shale) at about 85 Ma with the HP
model
and 65 Ma with the RE
model
. Earlier oil
generation
in the HP
model
is caused by the high sulfur content of the type IIS kerogen in the Jurassic source rocks. The influence of organic sulfur is accounted for in the HP kinetic parameters, but not the RE kinetic parameters. The cumulative volume of oil generated from the source rocks is 678 billion m3 for the HP
model
and 444 billion m3 for the RE
model
, or 65% of the HP volume. This difference is attributed to early
generation
from type IIS kerogen that resulted in much larger volumes of thermally mature source rocks for the Jurassic Fernie Group and consequently larger volumes of generated oil. The Gordondale Member in the HP
model
generated more than 550 times the volume of oil generated by the Gordondale Member in the RE
model
. The timing and generated volumes are comparable in the RE and HP models for source rocks that contain normal levels of organic sulfur (type II kerogen). The Duvernay is an exception because of the very low sulfur content of its type II kerogen. The result is higher HP kinetic than RE kinetic parameters, with associated greater thermal maturities required for HP than for RE oil
generation
. Consequently, there is less mature Duvernay source rock in the HP
model
than the RE
model
.
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