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25th International Meeting on Organic Geochemistry IMOG 2011

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P-088<br />

Crude oil in the Alpine Foreland Basin of Austria: a known<br />

petroleum system revisited<br />

Achim Bechtel 1 , Reinhard Gratzer 1 , Reinhard F. Sachsenhofer 1 , Hans-Gert Linzer 2 ,<br />

Doris Reischenbacher 1 , Hans-Martin Schulz 3<br />

1 M<strong>on</strong>tanuniversitaet, Leoben, Austria, 2 Rohoel-Aufsuchungs AG, Vienna, Austria, 3 GFZ German Research<br />

Centre for Geosciences, Potsdam, Germany (corresp<strong>on</strong>ding author:Achim.Bechtel@mu-leoben.at)<br />

The Alpine Foreland Basin is a minor oil and<br />

moderate gas province in central Europe. The<br />

majority of the fields is located in southeastern<br />

Germany and Austria. In the Austrian part of the<br />

Alpine Foreland Basin, oil and minor thermal gas are<br />

thought to be predominantly sourced from lower<br />

Oligocene horiz<strong>on</strong>s (i.e. the Schöneck, Dynow, and<br />

Eggerding formati<strong>on</strong>s). The source rocks are<br />

immature where the oil fields are located and enters<br />

the oil window at ca. 4 km depth beneath the Alpine<br />

nappes indicating l<strong>on</strong>g-distance lateral migrati<strong>on</strong>.<br />

Most important reservoirs are Upper Cretaceous and<br />

Eocene basal sandst<strong>on</strong>es.<br />

Stable carb<strong>on</strong> isotope and biomarker ratios of oils<br />

from different reservoirs indicate compositi<strong>on</strong>al trends<br />

in W-E directi<strong>on</strong> which reflect differences in source,<br />

depositi<strong>on</strong>al envir<strong>on</strong>ment (facies), and maturity of<br />

potential source rocks (Fig. 1). Thermal maturity<br />

parameters from oils of different fields are <strong>on</strong>ly in the<br />

western part c<strong>on</strong>sistent with northward displacement<br />

of immature oils by subsequently generated oils. In<br />

the eastern part of the basin different migrati<strong>on</strong><br />

pathways must be assumed (Fig. 1c). The trend in<br />

S/(S+R) isomerisati<strong>on</strong> of ��� C29 steranes versus the<br />

��� (20R)/��� (20R) C29 steranes ratio from oil<br />

samples can be explained by differences in thermal<br />

maturati<strong>on</strong> without invovling l<strong>on</strong>g-distance migrati<strong>on</strong>.<br />

The results argues for hydrocarb<strong>on</strong> migrati<strong>on</strong> through<br />

highly permeable carrier beds or open faults rather<br />

than relatively short migrati<strong>on</strong> distances from the<br />

source. The lateral distance of oil fields to the positi<strong>on</strong><br />

of mature source rocks beneath the Alpine nappes in<br />

the south suggests migrati<strong>on</strong> distances between less<br />

than 20 km and more than 50 km.<br />

Biomarker compositi<strong>on</strong>s of the oils suggest Oligocene<br />

shaly to marly succcesi<strong>on</strong>s (i.e. Schoeneck, Dynow,<br />

and Eggerding formati<strong>on</strong>s) as potential source rocks,<br />

taking into account their immature character. Best<br />

matches are obtained between the oils and units a/b<br />

(marly shale) and c (black shale) of the ―normal‖<br />

Schöneck Formati<strong>on</strong>, as well as with the so-called<br />

―Oberhofen facies‖. Results from open system<br />

pyrolysis-gas chromtography of potential source rocks<br />

indicate sligthly higher sulfur c<strong>on</strong>tent of the resulting<br />

pyrolysate from unit b. The enhanced dibenzo–<br />

thiophene/phenanthrene ratios of oils from the<br />

western part of the basin would be c<strong>on</strong>sistent with a<br />

higher c<strong>on</strong>tributi<strong>on</strong> of unit b to hydrocarb<strong>on</strong> expulsi<strong>on</strong><br />

in this area. Differences in the relative c<strong>on</strong>tributi<strong>on</strong> of<br />

sedimentary units to oil generati<strong>on</strong> are inherited from<br />

thickness variati<strong>on</strong>s of respective units in the<br />

overthrusted sediments. The observed trend toward<br />

lighter � 13 C values of hydrocarb<strong>on</strong> fracti<strong>on</strong>s from oil<br />

fields in a W-E directi<strong>on</strong> are c<strong>on</strong>sistent with lower<br />

� 13 C values of organic matter in unit c.<br />

231

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