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Geochemical-characteristics-of-some-crude-oils-from-Alif-Field-in-the-Marib-Shabowah-Basin-and

Geochemical-characteristics-of-some-crude-oils-from-Alif-Field-in-the-Marib-Shabowah-Basin-and
Geochemical-characteristics-of-some-crude-oils-from-Alif-Field-in-the-Marib-Shabowah-Basin-and

Geochemical characteristics of some crude oils from Alif Field in the Marib-Shabowah Basin,and source-related types

Mohammed Hail Hakimi a ,*,Wan Hasiah Abdullah b

a Geology Department,Faculty of Applied Science,Taiz University,6803Taiz,Yemen b

Department of Geology,University of Malaya,50603Kuala Lumpur,Malaysia

a r t i c l e i n f o

Article history:

Received 12December 2012Received in revised form 29April 2013

Accepted 14May 2013

Available online 29May 2013Keywords:Oil families Biomarker

Depositional environment Source inputs

Marib-Shabowah Basin Yemen

a b s t r a c t

The Marib-Shabowah Basin is an important hydrocarbon province in western Yemen,but the origin of hydrocarbons is not fully understood.In this regard,geochemical characteristics are used to provide information on source organic matter input,depositional environment and the correlation between crude oils from different pay zones.Two oil families are present within the study area and classi ?ed based on biomarker and non-biomarker parameters.The family I oils are characterized by low API gravity,high sulfur and trace metal (Ni,V)contents and low Ph/Ph ratio <1.0.These oils were derived from an alga organic matter that was deposited in a highly anoxic,hypersaline marine depositional environment and generated at low maturity.

Family II oils have medium to high API gravity,low sulfur and trace metal contents and relatively high Pr/Ph ratios (1.09e 1.59).The family II oils were derived from mixed marine and terrigenous organic matter and deposited under sub-oxic conditions.These oils were generated from source rocks with a wide range of thermal maturity ranging from early to peak oil window.The oil characteristics suggest that family I oils may be derived from the Tithonian age Safer calcareous shales and family II oils from the deeper Kimmeridgian Madbi shales.

ó2013Elsevier Ltd.All rights reserved.

1.Introduction

Sedimentary organic matter and crude oils contain complex assemblages of biological marker compounds (biomarkers)that preserve the molecular structure of various compounds that constitute the organisms.Biomarkers are widely used in the pe-troleum industry to identify groups of genetically related oils,to correlate oils with source rocks and to describe the probable source rock depositional environments for migrated oil of uncertain origin and the degree of biodegradation (Moldowan et al.,1985;Peters and Moldowan,1993;Peters et al.,2005).

Many oil ?elds have been discovered in the Marib-Shabowah Basin,an important hydrocarbon province in the western part of Yemen (Fig.1),since oil was ?rst discovered in the late 1980s.The Alif Field,located in the central portion of the Marib-Shabowah Basin (Fig.1),is one of the most proli ?c oil ?elds.The Marib-Shabowah Basin has attracted the interest of numerous re-searchers,authors and oil companies for the exploration of hy-drocarbons.The Marib-Shabowah Basin developed during the

Jurassic and is related to rifting of the Arabian plate from the Gondwana supercontinent (Redfern and Jones,1995;Beydoun et al.,1996).The stratigraphic section in the Marib-Shabowah Ba-sin is dominated by a thick Mesozoic succession and ranges in age from Jurassic to Cretaceous (Fig.2).The organic-rich shales of Madbi Formation (Kimmeridgian)and Safer Member (Tithonian)are the proli ?c oil prone source rocks in the Marib-Shabowah Basin (Brannin et al.,1999;Csato et al.,2001;Hakimi and Abdullah,2013).The Alif Member is considered the main reservoir in the Marib-Shabowah Basin (Fig.2)and comprises over 90%of recoverable oil in the basin (JNOC,2000“personal communication ”).Previous geochemical studies on the Marib-Shabowah Basin oils are un-published.Within this perspective,we report the results of an organic geochemical investigation on crude oils from the Alif Field.The objective is to use biomarker distributions together with the bulk geochemical parameters to characterize the oil types and to assess the respective depositional environment and thermal maturity of their potential source rocks.2.Samples and methods

The materials used in this study include 10crude oil samples representing different petroleum reservoirs in the Alif Field,Marib-

*Corresponding author.

E-mail address:ibnalhakimi@https://www.wendangku.net/doc/462651154.html, (M.H.

Hakimi).

Contents lists available at SciVerse ScienceDirect

Marine and Petroleum Geology

journal ho mep age:www.elsevier.co m/lo cate/marp

etgeo

0264-8172/$e see front matter ó2013Elsevier Ltd.All rights reserved.https://www.wendangku.net/doc/462651154.html,/10.1016/j.marpetgeo.2013.05.008

Marine and Petroleum Geology 45(2013)304e 314

Shabowah Basin(Table1).The geographic locations of the wells chosen are shown in Figure1.

The ratios of transition metals(vanadium and nickel)in crude oil are useful in the determination of source rock type,depositional environment and maturation because they remain unchanged irrespective of diagenetic and in-reservoir alteration effects (Barwise,1990;Udo et al.,1992).Absolute concentrations of va-nadium and nickel can be used to classify and correlate oils.These metals are the major metals in petroleum(Boduszynski,1987).The metals analysis was conducted at Geochem Laboratories Limited (USA).

Asphaltenes were precipitated from the crude oils by adding a 40fold excess of n-hexane.The precipitated asphaltenes were ?ltered.The fractions of the hexane soluble organic matter were separated into saturated hydrocarbons,aromatic hydrocarbons and NSO compounds using liquid column chromatography.A chro-matographic column(30?0.72cm)was packed with equal vol-umes of alumina and silica(both activated for2h at200 C).

The saturated hydrocarbon fractions were then analyzed by gas chromatography(GC)and gas chromatography e mass spectrom-etry(GC e MS).A FID GC with HP-5MS column and helium carrier gas was used.A temperature program from40to300 C at a rate of 4 C/min and then held for30min at300 C was used for GC analysis.GC e MS experiments were performed on a V5975B inert MSD mass spectrometer with a GC attached directly to the ion source(70eV ionization voltages,100mA?lament emission cur-rent,230 C interface temperature with full scan).

3.Results and discussion

Biomarker distributions and bulk oil parameters were used to assess the genetic relationship between hydrocarbon generation and their source rock depositional environments.Based on bulk geochemical properties and?ngerprints(GC and GC e MS),the investigated oils were classi?ed into two genetic families.A description of the geochemical characteristics of the oil families follows.

3.1.Non-biomarker characteristics

3.1.1.Bulk properties of crude oils

The bulk crude oil properties and compositions for the studied oils are presented in Table1.The crude oils from the Alif Field have a variety of API gravity values in the range of15.0e58.7 (Table1). Low API gravity is generally associated with either biodegraded oils or with immature sulfur-rich oils(Baskin and Peters,1992).

Biodegradation may occur in an oil reservoir,and the process dramatically affects the?uid properties of the hydrocarbons(e.g., Miiller et al.,1987).The early stages of oil biodegradation are characterized by the loss of n-alkanes or normal alkanes followed by loss of acyclic isoprenoids(e.g.,pristane and phytane). Compared with those compound groups,other compound classes (e.g.,highly branched and cyclic saturated hydrocarbons as well as aromatic compounds)are more resistant to biodegradation(Larter et al.,2005).In this respect,the analyzed oil samples contain a complete suite of n-alkanes in the low-molecular weight region and acyclic isoprenoids(e.g.,pristane and phytane;Fig.3).There-fore,there is no sign of biodegradation among the oil samples.This is also indicated by the oil samples generally containing more saturated hydrocarbons than aromatic hydrocarbons with saturate/ aromatic hydrocarbons ratios>1(Table1).On the other hand,the relationship between API gravity and sulfur content re?ects that the low API gravity is associated with sulfur-rich oils(Fig.4).A wide range of bulk property values of the crude oils analyzed indicates that two oil families are represented(Table1).Family I represent four crude oils,which have low API gravities,corresponding to high sulfur content of3.03e6.00wt%(Fig.4),suggesting that these oils were generated from clay-poor marine source rocks deposited under highly reducing conditions(Gransch and Posthuma,1973; Moldowan et al.,1985).In contrast,family II represents six crude

oil Figure1.Location map of the?elds in the Marib-Shabowah Basin including Alif Field and studied wells.

M.H.Hakimi,W.H.Abdullah/Marine and Petroleum Geology45(2013)304e314305

Figure2.Regional stratigraphic nomenclature in the Marib-Shabowah Basin,Republic of Yemen.

Table1

Bulk organic geochemical properties of crude oil samples from Alif Field,Marib-Shabowah Basin.

Wells Crude

oils Oil

family

Depths

(ft)

Reservoir rocks Chemical properties Metals Hydrocarbons Non-hydrocarbons Saturate/

aromatic

Waxiness

degree

S(n-C21e n-C31)/

S(n-C15e n-C20) API gravity

( )

Sulfur

(wt%)

Ni

(ppm)

V

(ppm)

VtNi

(ppm)

Saturate Aromatic Resinstasphaltenes

Alif-9SFCU-2I4367Safer-sandstone14.0 3.03 3.8036.340.133.424.142.5 1.390.55 SFCU-3I5893Safer-sandstone19.4 5.86 5.5020.826.328.712.059.3 2.390.54 Alif-16SFCU-4I4193Safer-sandstone15.0 6.00 6.1042.548.633.521.345.2 1.570.30 Alif-2SFCU-1I5370Safer-sandstone16.3 5.90 4.2039.043.233.020.846.2 1.590.53 SECU-1II6390Seen-sandstone39.2 1.130.13 1.16 1.2947.311.441.3 4.15 1.13 SECU-2II6540Seen-sandstone39.00.110.14 1.38 1.5241.515.842.7 2.630.98 Alif-1AFCU-1II5270Alif-sandstone58.70.170.17 1.10 1.2757.814.527.7 3.990.64 AFCU-2II5700Alif-sandstone40.10.310.110.440.5568.323.97.8 2.860.67 MECU-1II8080Meem-sandstone35.80.170.11 1.60 1.7134.027.938.1 1.270.82 MECU-2II8510Meem-sandstone38.80.800.14 1.05 1.1935.630.533.9 1.170.95

samples,which exhibit medium to high oil API gravities between 35.8 and 58.7 .These oils have a variety of sulfur contents,ranging from 0.11to 1.13wt%(Fig.4),suggesting they have been generated from clay-rich source rocks (Hedberg,1968;Gransch and Posthuma,1973;Moldowan et al.,1985).

The degree of waxiness S (n -C 21e n -C 31)/S (n -C 15e n -C 20)is used to categorize the amount of land derived organic material in oil,assuming that terrigenous material contributes a high molecular weight normal paraf ?n component to the oil (Connan and Cassou,1980;Johns,1986).The calculated ratio of S (n -C 21e n -C 31)/S (n -C 15e n -C 20)generally indicates a low degree of waxiness <1(Table 1),suggesting that these oils have been derived from algal and/or bacterial organic matter (Brooks et al.,1969;Tissot and Welte,

1984).The correlation between the degree of waxiness and sulfur content also re ?ects two different oil families (Fig.5).The family I oil samples have low waxiness values (<0.6)and high sulfur con-tent (>3wt.%)suggesting that they have been derived from

mainly

Figure 3.Gas chromatography traces of whole crude oil for representative two oil families in this

study.

Figure 4.Plot of the API gravity versus the sulfur content (wt%)for crude oils from various reservoir rocks in the Alif Field,Marib-Shabowah

Basin.

Figure 5.Relationship between sulfur content (wt%)and degree of the waxiness for the investigated crude oils in the Alif Field,Marib-Shabowah

Basin.

Figure 6.Relationship between total concentration of (V tNi)and degree of waxiness S (n -C 21e n -C 31)/S (n -C 15e n -C 20)for investigated crude oils from Alif Field,Marib-Shabowah Basin.

M.H.Hakimi,W.H.Abdullah /Marine and Petroleum Geology 45(2013)304e 314307

Figure 7.Gas chromatography traces of saturated hydrocarbons for representative oil samples in this study,showing two oil families.

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308

marine algal origin.On the other hand,family II oils have a rela-tively high waxiness values (>0.6)and low sulfur content,sug-gesting a relatively higher marine algal organic matter and lower terrigenous organic matter contribution.

3.1.2.Nickel and vanadium contents

Nickel and vanadium can be successfully used to distinguish between oils from different geographical areas (Hedberg,1968).The concentrations of the V and Ni can be also used to classify and correlate petroleum.In general,oils from marine carbonates or siliciclastics show low wax content,moderate to high sulfur and high concentrations of Ni and V elements (Barwise,1990),whereas land plant-derived oils contain high wax,low sulfur,and very low metal contents (Wenger et al.,2002).The investigated oils have a wide range of Ni and V content values,ranging from 0.44to 42.5ppm and 0.11to 6.10ppm,respectively.These values with sulfur content and degree of waxiness S (n -C 21e n -C 31)/S (n -C 15e n -C 20)values (Table 1)indicate a marine or perhaps slightly restricted marine environment.

The correlation of the total concentration of (V tNi)vs.degree of waxiness S (n -C 21e n -C 31)/S (n -C 15e n -C 20)are shown in Figure 6.The results indicate that trace metals are sensitive to changes in the

source input and re ?ects two different oil families.However,the latter ?gure shows that the family II oils considered to be derived from source rock contain a higher terrigenous organic matter contribution compared to family I oil samples.3.2.Biomarker characteristics

3.2.1.Normal alkanes and isoprenoids

The gas chromatograms of saturated hydrocarbon fractions from representative oil samples are shown in Figure 7and derived pa-rameters are listed in Table 2.The saturated gas chromatograms of the oil samples display a full suite of saturated hydrocarbons be-tween C 13e C 35n -alkanes and isoprenoids pristane (Pr)and phytane (Ph)(Fig.7).The differences in the distribution patterns of n -al-kanes and acyclic isoprenoids suggest that the investigated oils are derived from two different sources.

The n -alkane distribution of family I oils shows a predominance of low to medium molecular weight compounds (n -C 14e n -C 20),suggesting a signi ?cant contribution of algal derived organic

Table 2

Selected biomarker parameters of the crude oil samples illustrating source and maturity differences between the two oil families.Crude oils

Oil family

n -alkane and isoprenoids Triterpanes and terpanes (m /z 191)

Steranes and diasteranes (m /z 217)

Pr/Ph Pr/C 17Ph/C 18CPI

C 3222S/(22S t22R)C 29/C 30Ts/Tm MC 30/HC 30H index G/C 30C 2920S/(20S t20R)C 29bb /(bb taa )C 29/C 27Regular steranes (%)Diasterane/sterane

C 27C 28C 29SFCU-2I 0.420.43 1.470.910.59

0.630.290.060.12 1.130.350.350.267111180.31SFCU-3I 0.500.71 2.680.940.580.230.300.100.170.990.430.390.675116330.40SFCU-4I 0.270.23 1.100.740.600.700.180.070.22 1.050.420.420.446112270.44SFCU-1I 0.300.82 3.240.810.560.440.500.160.160.230.430.380.845014360.23SECU-1II 1.090.640.66 1.060.560.680.910.200.08e 0.500.540.92431641 1.09SECU-2II 1.530.630.46 1.060.620.43 2.000.110.05e 0.500.410.794518360.69AFCU-1II 1.240.520.430.990.630.62 1.060.110.06e 0.510.450.883721410.68AFCU-2II 1.520.590.44 1.020.590.36 1.500.100.07e 0.480.38 1.144222370.54MECU-1II 1.590.400.29 1.070.630.30 4.000.100.06e 0.520.55 1.004020400.71MECU-2II 1.360.400.28 1.04

0.62

0.46

5.00

0.12

0.08

e

0.51

0.55

1.06

38

22

40

0.77

Pr:pristane.Ph:phytane.

CPI:carbon preference index (2[C 23tC 25tC 27tC 29]/[C 22t2{C 24tC 26tC 28}tC 30]).Ts:(C 2718a (H)-22,29,30-trisnorneohopane).Tm:(C 2717a (H)-22,29,30-trisnorhopane).C 29/C 30:C 29norhopane/C 30hopane.MC 30/HC 30:C 30moretane/C 30hopane.H Index:(C 35/(C 31àC 35))homohopane.G/C 30:Gammacerane/C 30

hopane.

Figure 8.Phytane to n -C 18alkane (Ph/n -C 18)versus pristane to n -C 17alkane (Pr/n -C 17

).

Figure 9.Cross plot of dibenzothiophene/phenanthrene (DBT/Phe)versus pristane/phytane (Pr/Ph)ratios provides a powerful way to infer crude oil source rock depo-sitional environments and lithologies (Hughes et al.,1995).

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309

matter from a marine environment,whereas family II oils also show a predominance of low to medium molecular weight compounds (n -C 14e n -C 20)with the presence of signi ?cant waxy alkanes (tn -C 23)thus gave moderate CPI values (Table 2),suggesting a higher contribution of marine organic matter with minor terrigenous organic matter contribution (Brooks et al.,1969;Powell and McKirdy,1973;Tissot et al.,1978;Ebukanson and Kinghorn,1986;Murray and Boreham,1992).

Acyclic isoprenoids occur in a signi ?cant amount in all studied oil samples (Fig.7)and diagnostic biomarker ratios are listed in Table 2.The phytane being the most dominant peak in the satu-rated gas chromatograms of the family I oil samples studied (Fig.7);phytane concentration is always higher than n -C 18,thus giving distinctively high phytane/n -C 18ratios of 3.24e https://www.wendangku.net/doc/462651154.html,paratively lower values for these ratios (0.29e 0.66)were displayed by family II oil samples,which generally possess relatively,lower amounts of acyclic isoprenoids (compared to n -alkanes)than the family I oil samples (Fig.8).The pristane/phytane (Pr/Ph)ratio is also one of the most commonly used geochemical parameters and has been widely invoked as an indicator of the redox conditions in the depositional environment and source of organic matter (Didyk et al.,1978;Powell,1988;Chandra et al.,1994;Large and Gize,1996).Organic matter originating predominantly from land plants would be expected to contain high Pr/Ph >3.0(oxidizing condi-tions),low values of (Pr/Ph)ratio (<1.0)indicate anoxic conditions and values between 1.0and 3.0suggest intermediate conditions (sub-oxic conditions)(Philp,1985;Amane and Hideki,1997).The Pr/Ph ratios of the investigated oil samples range from 0.27to 1.59(Table 2),suggesting two oil types and derived from different source rocks.The family I oils have Pr/Ph ratio values <1.0,whereas family II oils have moderately Pr/Ph ratios in the range of 1.09e 1.59.The Pr/Ph ratios indicate that the family I oils considered to

be

Figure 10.The distributions of triterpanes m /z 191mass fragmentograms of saturated hydrocarbons representative of the two oil families in the Alif Field,Marib-Shabowah Basin,showing two oil families.

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310

derived from source rocks containing mainly marine algal-derived organic matter which was deposited in a more reducing environ-ment compared to family II oil samples (sub-oxic).This is consistent with the observed of high phytane/n -C 18ratios of family I oil samples compared to family II oil samples (Fig.8).Furthermore,the ratios of dibenzothiophene/phenanthrene and pristane/phytane can be also used to infer crude oil source rock depositional envi-ronments and lithologies (Hughes et al.,1995).The cross plot of dibenzothiophene/phenanthrene versus pristane/phytane in-dicates that Alif oils have been derived from two different source rock (Fig.9).The family I oils were derived from marine carbonate and marl sediments whereas the family II oils were derived from marine shales (Fig.9).

3.2.2.Triterpanes

The distributions of terpanes are commonly studied using GC e MS by monitoring the ions m /z 191(Brooks et al.,1969;Peters et al.,2005)as a legend to Figure 10.For peak assignments see Table A1in Appendix 1.Individual components were identi ?ed by comparison of their retention times and mass spectra with published literature (Philp,1985;Peters and Moldowan,1993).

The differences in the distribution patterns of m /z 191mass fragmentograms suggest that the investigated oils are classi ?ed into two oil families (Fig.10).The m /z 191mass fragmentograms of the saturated hydrocarbon fractions of all the oil samples analyzed show high proportions of hopanes relative to tricyclic terpanes as shown in Figure 10.The relative abundance of C 29norhopane is generally half or less than that of C 30hopane in most of the studied samples (Fig.10),with C 29/C 3017a (H)hopane ratios in the range of 0.23e 0.70(Table 2).The predominance of C 30hopane is frequently associated with clay-rich source rocks (Gürgey,1999).

The investigated oils possess a wide range of Ts/Tm ratio values and ranging from 0.18to 5.00(Table 2).Values of Tm (C 2717a (H)-22,29,30-trisnorhopane)and Ts (C 2718a (H)-22,29,30-trisnorneohopane)are well known to be in ?uenced by matura-tion,type of organic matter,and lithology (Moldowan et al.,1985).In the present study,the main difference is controlled by organic facies and lithology,with a maturation overprint within each oil family.Furthermore,the ratio of diasterane/sterane is plotted against Ts/Tm ratio,suggesting that family I oils have been associ-ated with more carbonate lithology compared to family II oil samples (Fig.11)as indicated by dibenzothiophene/phenanthrene and pristane/phytane ratios (Fig.9).Extended hopanes are

dominated by the C 31homohopane and generally decreasing to-ward the C 35homohopane (Fig.10).The ab hopanes are more prominent than the ba hopanes while the S isomers are more dominant than the R isomers among the homohopane (C 31e C 35).The distribution of the extended hopanes or homohopanes (C 31e C 35)has been used to evaluate redox conditions based on homo-hopanes index (Peters et al.,2005).This,in turn,suggests that the family I oils were derived from source rock deposited in a more reducing environment than the family II oil samples source rock.In support,relatively higher homohopanes index were obtained for family I oils compared to the family II oil samples (Table 2).High C 35/C 34hopanes ratios have been reported in highly reducing ma-rine oils (Moldowan et al.,1985;Peters and Moldowan,1991).This is consistent with the observed of high C 35/C 34hopanes ratios of family I oil samples (Fig.10).

In addition,gammacerane has been recorded in family I oil samples (Fig.10),is a strong indicator of high-salinity conditions and water column strati ?cation during deposition of the source rocks (Moldowan et al.,1985;ten Haven et al.,1989;Sinninghe-Damstéet al.,1995;Peters et al.,2005).The occurrence of gam-macerane in the family I oils is also consistent with Safer shales association with interbedded evaporites (refer to stratigraphic section in Fig.2)(Rohrback,1981;Mello et al.,1988).

3.2.3.Steranes

The distributions of diasteranes and the steranes (C 27,C 28and C 29)are characterized by the m /z 217ion chromatograms (Fig.12).Peaks labels are listed on Table A1in Appendix 1and the derived parameters are listed in Table 2.The relative amounts of C 27e C 29steranes can be used to give indication of source differences (Seifert and Moldowan,1979).The relative distribution of C 27,C 28and C 29steranes is graphically represented in the form shown for a regular steranes in a ternary diagram (Fig.13,Huang and Meinschein,1979).The original classi ?cation of Huang and Meinschein (1979)related C 27steranes to strong algal in ?uence and C 29steranes to strong higher plant in ?uence.The differences in the distribution of regular steranes (C 27e C 29)suggest that the oils are derived from different types of organic matter (Fig.13).The family I oil samples display a strong predominance of C 27steranes (Table 2),which suggest a dominance of marine algal organic matter (Fig.11),while the family II oils that composed of C 27e C 29steranes which is an indicator of the mixed marine/terrigenous origin for the oil as indicated by Pr/n -C 17and Ph/n -C 18ratios (Fig.8).This is consistent with the observed of low C 29/C 27sterane ratios of family I oil samples compared to family II oil samples (Table 2).

The diasterane/regular sterane ratios and two different sterane thermal maturity parameters,C 2920S/(20S t20R)and the C 29abb /(abb taaa ),are calculated and listed in Table 2.The higher dia-sterane/sterane ratios in the family II oil samples compared to family I oil samples correspond to the higher clay contents in the former (Gürgey,1999).3.3.Maturity of crude oils

The components in oil,NSO compounds,asphaltenes and saturated and aromatic hydrocarbons undergo increased cracking during thermal maturation.A variety of oil characteristics has been used to evaluate the level of thermal maturity of the investigated oils;these include biomarker and non-biomarker parameters.The biomarker and non-biomarker parameters are listed in Tables 1and 2,and are discussed in more detail below.In gas chromatography e mass spectrometry (GC e MS),biomarker maturation parameters such as C 3222S/(22S t22R)homohopane,moretane/hopane and 20S/(20S t20R)and bb /(bb taa )C 29sterane ratios,was used

as

Figure 11.Relationship between Ts/Tm ratio and Diasterane/sterane ratio for the investigated crude oils in the Alif Field,Marib-Shabowah Basin.

M.H.Hakimi,W.H.Abdullah /Marine and Petroleum Geology 45(2013)304e 314311

maturity indicators (Mackenzie et al.,1980;Waples and Machihara,1991).The ratios of 22S/(22R t22S)for C 3217a (H),21b (H)-hopanes are between 0.56and 0.63(Table 2)suggesting that they have reached equilibrium.The 20S/(20S t20R)and bb /(bb taa )C 29sterane ratios of the oils are between 0.35and 0.52,and 0.35e 0.55,respectively (Table 2).These biomarker maturation parame-ters are indicating that the oils are expelled from source rocks that were exposed to thermal maturity level equivalent to the early to peak oil window stage of petroleum generation.The correlation between two biomarker maturity parameters is shown in Figure 14(Peters and Moldowan,1993).This correlation re ?ects that the family I oils are early mature,whereas the family II oils are early mature to peak oil window (Fig.14).The relationship between isoprenoids Pr/n -C 17and Ph/n -C 18ratios (Fig.8)re ?ects the same interpretation as do the moretane/hopane ratios (Waples and Machihara,1991).

Non-biomarker parameters such as API gravity,sulfur and metal contents have also been used to evaluate the level of thermal maturity of the investigated oils (El-Gayar et al.,2002).The concentrations of Ni and V varied strongly with the maturity of oils and high maturity crude oils contained only small amounts of Ni and V elements (Barwise,1990).This is consistent the observed of low Ni and V content of family II oil samples compared to family I oil samples (Table 1).The correlation between API gravity and sulfur content (Fig.4),and between sulfur content and concentrations of (V tNi)values (Table 1)are indicated that the levels of metals and sulfur in crude oil decrease with increasing maturity,whereas the API gravity increase.This is consistent with previous biomarker

observations.

Figure 12.The distributions of steranes m /z 217mass fragmentograms of saturated hydrocarbons for representative two oil families in the Alif Field,Marib-Shabowah Basin.

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4.Conclusions

Geochemical characterization based upon biomarker compo-nents coupled with the bulk geochemical parameters was used to arrive at a clear characterization and classi ?cation of the Marib-Shabowah Basin crude oils.The ?ngerprints have been derived from the acyclic isoprenoids,triterpane and sterane biomarkers.Two oil families are observed and represented in the suite of investigated oil samples according to their sources.

Family I oils are characterized by low API gravity,high sulfur and metal contents and low Pr/Ph ratios (<1.0)indicating a strongly reducing marine conditions.This is supported by high C 35homohopane index and C 35/C 34hopane.These oils were derived from marine alga inputs,consistent which thus display a strong predominance of C 27regular steranes and supported by low C 29/C 27sterane ratio.The presence of gammacerane in these oils is a very good indicator of high-salinity conditions and water column strati ?cation during deposition of the source rocks.Previous work by Hakimi and Abdullah (2013)on the Safer shales

in the basin shows similar characteristics to these oils,suggesting that the family I oils are derived the interbedded Safer calcareous shales.

Family II oils have medium to high API gravity and low sulfur and metal contents.Oils from the family II display relatively high Pr/Ph ratios (1.09e 1.59),relatively low C 35homohopane index and high diasteranes relative steranes,indicating a marine clay source rock deposited in sub-oxic conditions.These oils type are composed of C 27e C 29regular steranes suggest that these oils were generated from source facies contain a mixture of marine with land plant organic matter deposited in a marine or perhaps slightly restricted marine environment.This is consistent the observed of low trace metal (Ni,V)content and relatively high waxiness values.The characteristics of these oils are consistent with their sourcing from the Madbi shales as described by Hakimi et al.(2010).

On the basis of the biomarker maturity and non-biomarker parameters,the investigated oils in the Alif Field are thermally mature and ranging from early mature to peak oil window.The family II oil samples were generated from source rocks with a wide range of thermal maturity and have entered early mature to peak oil window whereas the family I oil samples are early mature oils.

Acknowledgments

The authors thank the Petroleum Exploration and Production Authority (PEPA)and Safer Oil Company,Yemen for supplying the data and samples for this study.The authors are more grateful to the Department of Geology,University Malaya for providing facil-ities to complete this research.Special thanks are offered to Dr.Lloyd R.Snowdon for his helpful comments and corrections on an earlier version of the manuscript.

Appendix

1

Figure 13.Ternary diagram of regular steranes (C 27e C 29)showing the relationship between sterane compositions,source input,and depositional environment for the analyzed crude oils (modi ?ed after Huang and Meinschein,1979

).

Figure 14.Cross plot of two biomarker parameters sensitive to thermal maturity of the studied oil samples (modi ?ed after Peters and Moldowan,1993).

Table A1

Peak assignments for alkane hydrocarbons in the gas chromatograms of aliphatic fractions in the m /z 191(I)and 217(II)mass fragmentograms compound abbreviation.(I)Peak no.Ts 18a (H),22,29,30-trisnorneohopane Ts Tm 17a (H),22,29,30-trisnorhopane Tm

2917a ,21b (H)-nor-hopane C 29hop 3017a ,21b (H)-hopane Hopane 3M 17b ,21a (H)-Moretane

C 30Mor 31S 17a ,21b (H)-homohopane (22S)C 31(22S)31R 17a ,21b (H)-homohopane (22R)C 31(22R)32S 17a ,21b (H)-homohopane (22S)C 32(22S)32R 17a ,21b (H)-homohopane (22R)C 32(22R)33S 17a ,21b (H)-homohopane (22S)C 33(22S)33R 17a ,21b (H)-homohopane (22R)C 33(22R)34S 17a ,21b (H)-homohopane (22S)C 34(22S)34R 17a ,21b (H)-homohopane (22R)C 34(22R)35S 17a ,21b (H)-homohopane (22S)C 35(22S)35R

17a ,21b (H)-homohopane (22R)C 35(22R)(II)Peak no.a 13b ,17a (H)-diasteranes 20S Diasteranes b 13b ,17a (H)-diasteranes 20R Diasteranes c 13a ,17b (H)-diasteranes 20S Diasteranes d 13a ,17b (H)-diasteranes 20R Diasteranes e 5a ,14a (H),17a (H)-steranes 20S aaa 20S f 5a ,14b (H),17b (H)-steranes 20R abb 20R g 5a ,14b (H),17b (H)-steranes 20S abb 20S h

5a ,14a (H),17a (H)-steranes 20R

aaa 20R

M.H.Hakimi,W.H.Abdullah /Marine and Petroleum Geology 45(2013)304e 314313

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