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25th International Meeting on Organic Geochemistry IMOG 2011

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P-310<br />

Implicati<strong>on</strong>s of source rock and oil geochemistry to the<br />

understanding of the petroleum systems of the Northern Red<br />

Sea<br />

Jennifer Scott 1 , John Guthrie 2 , Steve Crews 2 , Graeme Gord<strong>on</strong> 1 , Niall McCormack 1 , Dean<br />

Griffin 1 , Laura Lawt<strong>on</strong> 1 , Andy Pepper 2<br />

1 Hess, L<strong>on</strong>d<strong>on</strong>, United Kingdom, 2 Hess Corporati<strong>on</strong>, Houst<strong>on</strong>, United States of America<br />

The integrati<strong>on</strong> of data from <strong>on</strong>shore samples, basin<br />

modelling, and oil and source rock geochemistry, has<br />

resulted in a better understanding of the petroleum<br />

systems of the Northern Red Sea (NRS), Egypt.<br />

The primary source rock in the NRS is thought to be<br />

the pre-rift Dakhla Formati<strong>on</strong>. These Maastrichtian<br />

marls and calcareous shales outcrop <strong>on</strong>shore <strong>on</strong> the<br />

western rift shoulders of the NRS. They were<br />

probably deposited as part of the southerly marine<br />

transgressi<strong>on</strong> of the Neo-Tethys during the mid-late<br />

Cretaceous. There is also a lesser c<strong>on</strong>tributi<strong>on</strong> from<br />

the syn-rift source rocks of the Miocene Rudeis<br />

Formati<strong>on</strong>. Onshore pre-rift samples were analysed to<br />

quantify organic carb<strong>on</strong> c<strong>on</strong>tent, hydrogen index, and<br />

geochemical characteristics. From these results, it<br />

appears that the Maastrichtian Dakhla Formati<strong>on</strong> is a<br />

rich oil-pr<strong>on</strong>e source rock, analogous and genetically<br />

related to the prolific late Campanian - early<br />

Maastrichtian Brown Limest<strong>on</strong>e in the Gulf of Suez.<br />

Saturate biomarkers from oil shows in offshore<br />

cuttings from NRS were used to identify the relative<br />

c<strong>on</strong>tributi<strong>on</strong>s from pre-rift and syn-rift source rocks.<br />

Figure 1 shows that oils sourced from the pre-rift<br />

Dakhla/Brown Limest<strong>on</strong>e are characterised by low<br />

oleanane and high C29 (hopane) indices, and<br />

isotopically light δ13C values (depleted in 13C),<br />

indicating a more carb<strong>on</strong>ate-rich source rock.<br />

Meanwhile syn-rift sourced oils have higher oleanane<br />

and are isotopically heavier (enriched in 13C).<br />

Offshore NRS oil shows can be typed to both syn-rift<br />

and pre-rift source rocks, indicating that the Dakhla is<br />

both present and mature in the offshore NRS.<br />

By comparing the geochemical characteristics of the<br />

pre-rift from the NRS to a large number of oil and<br />

source rock samples from the Gulf of Suez, source<br />

rock facies and thermal maturity variati<strong>on</strong>s within the<br />

pre-rift can be identified. Regi<strong>on</strong>al thermal maturity<br />

modelling calibrated to well temperature data and<br />

biomarker thermal maturity parameters (Figure 2) of<br />

reservoir oils has improved the evaluati<strong>on</strong> of thermal<br />

maturity variati<strong>on</strong>s. Biomarkers and carb<strong>on</strong> isotopes<br />

have been used to distinguish facies variati<strong>on</strong>s within<br />

the pre-rift, and a potential proximal-distal marine<br />

facies trend within the Brown Limest<strong>on</strong>e/Dakhla has<br />

been identified. This work has allowed for a better<br />

understanding of the envir<strong>on</strong>ment of depositi<strong>on</strong> of<br />

these world-class source rocks.<br />

Figure 1: Carb<strong>on</strong> isotope parameters of oils and<br />

source rocks (SR) from the Gulf of Suez and Northern<br />

Red Sea.<br />

Figure 2: Sterane maturity parameters used to<br />

assess the relative thermal maturity of oils and source<br />

rocks from the Gulf of Suez and Northern Red Sea.<br />

Thank you to Hess and Premier for permissi<strong>on</strong> to<br />

publish this work.<br />

443

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