Migration and Accumulation of Hydrocarbons in Cretaceous and Tertiary Reservoirs of Iraq: Implications of a 2D/3D Basin Modeling Study
By
Janet K. Pitman1, Douglas Steinshouer2, Michael Lewan3
(1) U.S. Geological Survey, Lakewood, CO (2) GeoLukas, Denver, CO (3) U. S. Geological Survey, Lakewood, CO
Multilayer, 2D/3D petroleum system modeling was undertaken to evaluate the
origin and extent of hydrocarbon (HC) generation, expulsion, and secondary
migration in the Upper Jurassic Sargelu/Naokelekan source rock system of Iraq.
Structural restorations of source rock surfaces, regional isopach and facies
maps, and thermal maturity data were used as input to the model. Petroleum
generation and potential migration pathways on the top of a (Lower Cretaceous)
composite reservoir unit immediately overlying the
principle
source rock unit
were modeled for three geologic
time
periods: 25, 8, and 0 Mybp. Petroleum
accumulations predicted by the model were compared with the location of known
fields that produce from the Cretaceous reservoir interval. Modeling results
show that in the early Miocene, at about 25 Mybp, the first major stage of HC
generation and expulsion was initiated in two depocenters. The petroleum that
migrated laterally from these areas began to fill most fields in northern Iraq
and the largest fields in southern Iraq. By 8 Mybp, in the late Miocene, the
area of main stage HC generation extended along the Zagros Mountain Front due to
extensive foreland basin deposition associated with the Zagros Orogeny, and
folding and faulting caused larger petroleum drainage basins to be segmented
into smaller subbasins. Related southwest tilting set up a northeast-southwest
HC flow pattern across the region. Modelling results demonstrate that Cretaceous
reservoired oil in northern Iraq remigrated vertically along faults and
fractures ultimately charging younger Tertiary reservoirs. At present day, most
subbasins containing hydrocarbon accumulations are underlain by active source
rock, and most fields lie on or close to migration pathways and have been
subject to filling and spilling. It follows that prospects closest to modeled
pathways are highly likely to be charged and thus have low exploration risk.