Abstract
Six crude oil samples from six wells in Khabbaz Oil Field were analyzed using gas chromatography/mass spectroscopy. One of the samples was from Lower Qamchuqa reservoir. The rest were taken from the Upper Qamchuqa reservoir. Biomarker distribution and characteristics are used to provide information on source of organic matter input, depositional conditions, maturation level, and possible source rock. The n-alkanes, terpanes, steranes, and aromatic compounds have been monitored through using specified mass/charge ratios. The crude oils from Khabbaz Oil Field are not affected by biodegradation as it is revealed from the gas chromatogram shapes of the studied samples and the high ratio of saturated and aromatic hydrocarbons to the NSO components. All samples reveal the dominant of short chain n-alkanes between C15-C18, with isoprenoids pristane and phytane. The unimodal envelope chromatograms, maximum peak carbon n-C15-n-C20, and low CPI values (0.89–0.93) indicating a high contribution of aquatic algae organic matter and with minor input from terrestrial plants. The high presence of C27 regular steranes also support this conclusion. In the studied oil samples of Khabbaz Oil Field, phytane has relatively higher concentrations than pristane with low Pr/Ph ratios in range 0.60–0.73. This indicates that these oils were derived from organic matter deposited in a marine environment under reducing conditions. In most samples, the abundance of C32 homohopanes is moderate and the 22S/22R + 22S epimerization ratio is around 0.55 to 0.61. In addition, gammacerane is recorded in the analyzed samples and the gammacerane index (gammacerane/C30 hopane) are indicating that the oils were generated from carbonate source rocks in anoxic and high salinity conditions. The relative C30 hopane abundance is less than C29 norhopane in all samples with high C29/C30 17α (H) hopane ratios in the range 1.33–1.62 which indicates that such crude oils are derived from carbonate-rich source rock. 20S/(20S+20R) and ββ/(ββ+αα) C29 sterane ratios are relatively consistent for all the analyzed samples, ranging between 0.43–0.46 and 0.58–0.63, respectively. This ratio (DBT/Phe) is also used to draw with Pr/Ph ratio as cross-plot, which is clearly indicates that the oils were generated from marine carbonate source rock. The Khabbaz crude oils have a 20S/ (20S +20R) and ββ/(ββ+αα) C29 sterane ratios in the range 0.43 to 0.46 and 0.58–0.63, respectively, which indicate thermal maturity (equivalent to peak oil generation stage). The Lower Qamchuqa reservoir is higher in pressure and temperature than the Upper Qamchuqa, as a result the oil of Lower Qamchuqa has higher maturity and API gravity. The studied area is underlain by several rock units which could make potential source rocks for the Khabbaz oils. The biomarkers distribution, and the δ13Corg indicate that the to Chia Gara Formation considered as the main source rock of the oils within Khabbaz Oil Field.
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Acknowledgements
The authors would like to thank the North Oil Company in Kirkuk for giving the studied crude oil samples with information on each well. The support from TOTAL Oil Company in analyzing crude oils by GC-MS in their laboratory is highly appreciated.
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Appendix 1
Appendix 1
Identified peaks in the m/z 177, m/z 191, m/z 217, and m/z 198 mass fragmentograms of Figures 6, 9, 10, and 12.
Peaks on m/z177 | ||
---|---|---|
TNH | Trisnorhopane | TNH |
C28DH | C28 Demethylated hopane | C28DH |
C29DH | C29 Demethylated hopane | C29DH |
30-norhopane | 30-Norhopane | 30-norhopane |
Peaks on m/z191 | ||
C23/3 | C23 Tricyclic (Cheilanthane) | Tri C23 |
C24/3 | C24 Tricyclic (Cheilanthane) | Tri C24 |
C25/3 R-S | C25 Tetracyclic R and S | Tri C25 R-S |
C24/4 | C24 Tetracyclic | Tet C24 |
C26/3 -S | C26 Tricyclic (Cheilanthane) | Tri C26 |
C26/3 -R | C26 Tricyclic (Cheilanthane) | Tri C26 |
C28/3 -S | C28 Tricyclic (Cheilanthane) | Tri C28 |
C28/3 -R | C28 Tricyclic (Cheilanthane) | Tri C28 |
C29/3 -S | C29 Tricyclic (Cheilanthane) | Tri C29 |
C29/3 -R | C29 Tricyclic (Cheilanthane) | Tri C29 |
Ts | 18α(H),22,29,30-trisnorneohopane | Ts |
Tm | 17α(H),22,29,30-trisnorhopane | Tm |
BNH | Bisnorhopane 17a,21b(H)-Dinorhopane | BNH |
C29DH | C29 Demethylated hopane | C29DH |
C29 | 17α,21β(H)-nor-hopane | C29 hop |
OLN | 18α(H) and 18β(H)-oleanane | OLN |
C30H | 17α,21β(H)-hopane | Hopane |
C30M | 17 β,21α (H)-Moretane | C30βα |
C31S | 17α,21β(H)-homohopane (22S) | C31(22S) |
C31R | 17α,21β(H)-homohopane (22R) | C31(22R) |
GCRN | C30 Gammacerane | GCRN |
C32/6 | 17α,21β(H)-homohopane | C32/6 |
C32S | 17α,21β(H)-homohopane (22S) | C32(22S) |
C32R | 17α,21β(H)-homohopane (22R) | C32(22R) |
C33/6 | 17α,21β(H)-homohopane | C33/6 |
C33S | 17α,21β(H)-homohopane (22S) | C33(22S) |
C33R | 17α,21β(H)-homohopane (22R) | C33(22R) |
C34/6 | 17α,21β(H)-homohopane | C34/6 |
C34S | 17α,21β(H)-homohopane (22S) | C34(22S) |
C34R | 17α,21β(H)-homohopane (22R) | C34(22R) |
C35/6 | 17α,21β(H)-homohopane | C35/6 |
C35S | 17α,21β(H)-homohopane (22S) | C35(22S) |
C35R | 17α,21β(H)-homohopane (22R) | C35(22R) |
Peaks on m/z217 | ||
C27 Sdia | 13β,17α(H)-diasteranes 20S | Diasteranes |
C27 Rdia | 13β,17α(H)-diasteranes 20R | Diasteranes |
C27 ααS | 5α,14α(H), 17α(H)-steranes 20S | C27ααα20S |
C27 ββR | 5α,14β(H), 17β(H)-steranes 20R | C27αββ20R |
C27 ββS | 5α,14β(H), 17β(H)-steranes 20S | C27αββ20S |
C27 ααR | 5α,14α(H), 17α(H)-steranes 20R | C27ααα20R |
C28 ααS | 5α,14α(H), 17α(H)-steranes 20S | C28ααα20S |
C28 ββR | 5α,14β(H), 17β(H)-steranes 20R | C28αββ20R |
C28 ββS | 5α,14β(H), 17β(H)-steranes 20S | C28αββ20S |
C28 ααR | 5α,14α(H), 17α(H)-steranes 20R | C28ααα20R |
C29 ααS | 5α,14α(H), 17α(H)-steranes 20S | C29ααα20S |
C29 ββR | 5α,14β(H), 17β(H)-steranes 20R | C29αββ20R |
C29 ββS | 5α,14β(H), 17β(H)-steranes 20S | C29αββ20S |
C29 ααR | 5α,14α(H), 17α(H)-steranes 20R | C29ααα20R |
Peaks on m/z 198 | ||
DBT | Dibenzothiophene | DBT |
4MDBT | 4 methyldibenzothiophene | 4MDBT |
2+3 MDBT | 2+3 methyldibenzothiophene | 2+3 MDBT |
1MDBT | 1 methyldibenzothiophene | 1MDBT |
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Qader, F.M., Mohialdeen, I.M.J., Al-Qayim, B. et al. Organic geochemical characterization of crude oil from the Cretaceous reservoir rocks of the Khabbaz Oil Field, Kirkuk Area, Northern Iraq. Arab J Geosci 14, 2117 (2021). https://doi.org/10.1007/s12517-021-08467-4
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DOI: https://doi.org/10.1007/s12517-021-08467-4