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32. ORGANIC GEOCHEMICAL COMPARISON OF CRETACEOUS GREEN AND BLACK CLAYSTONES FROM HOLE 530A IN THE ANGOLA BASIN 1 Philip A. Meyers, Oceanography Program, Department of Atmospheric and Oceanic Science, Thomas W. Trull, 2 Senior Honors Project, Department of Chemistry and Orest E. Kawka, 3 Oceanography Program, Department of Atmospheric and Oceanic Science, The University of Michigan, Ann Arbor, Michigan ABSTRACT Three pairs of Upper Cretaceous black shales and adjacent green claystones from Hole 53OA were analyzed to com- pare types and amounts of organic matter and lipids and to seek information about their environments of deposition. The organic-carbon-rich black shales have C/N ratios nearly seven times those of the organic-carbon-lean green clay- stones. The lipid content of organic matter in the black shales is about ten times less than in adjacent green layers. Or- ganic matter in both types of rocks is thermally immature, and distributions of alkanoic acids, alkanols, sterols, and al- kanes contain large amounts of terrigenous components. Pristane/phytane ratios of less than one suggest that younger Turonian sediments were laid down under anoxic conditions, but ratios greater than one suggest that older Turonian Cenomanian deposits accumulated in a more oxic environment. Closely bedded green and black layers have very similar types of lipid distributions and differ primarily in concentrations, although black shales contain somewhat larger amounts of terrigenous lipid components. Geochemical and stratigraphic evidence suggests much of the organic matter in these samples originated on the African continental margin and was transported to the Angola Basin by turbidity flow. Rapid reburial of organic-carbon-rich sediments led to formation of the black shales. INTRODUCTION Black shales containing high amounts of organic matter were deposited in deep waters of the South At- lantic during the Cretaceous period. Occurrences of black shale formation are found in the Barremian-Ap- tian at Deep Sea Drilling Project (DSDP) Site 361 in the Cape Basin and at Sites 327 and 330 on the Falkland Plateau, in the Albian at Site 363 on the northern flank of Walvis Ridge, in the Turonian-Santonian at Site 356 on the Sao Paulo Plateau, and in the Aptian-Albian and Turonian-Santonian at Site 364 in the Angola Basin (Bolli, Ryan et al., 1978). Concentrations of organic carbon reach as high as 24% dry weight of Aptian sedi- ment at Site 364 (Foresman, 1978). The conditions which led to the formation of these organic-carbon-rich layers are not understood, although some combination of low availability of oxygen and abundant supply of organic matter seems likely. Primary among the scientific goals of DSDP Leg 75 was to investigate the Cretaceous paleoceanographic conditions in which black shales were formed. Hay et al. (1982) summarize information obtained from Site 530 in the Angola Basin where black shale layers were found in the Albian to early Coniacian. They conclude that or- ganic-carbon-rich sediments accumulated in an oxygen minimum zone of varying intensity on the African con- tinental slope and were redeposited in deep waters by 1 Hay, W. W., Sibuet, J.-C, et al., Init. Repts. DSDP, 75: Washington (U.S. Govt. Printing Office). 2 Present address: Woods Hole Oceanographic Institution, Woods Hole, Massachusetts. 3 Present address: School of Oceanography, Oregon State University, Corvallis, Oregon. turbidity flows and slumping. Preservation of organic matter in the deep-water environment was enhanced by rapid burial in the bottom. Organic geochemistry can provide information which will help answer some of the questions about black shales. Evidence of biological sources and of deposi- tional environments is often preserved in the elemental and molecular composition of organic matter in rocks and sediments. In the case of the Aptian to Coniacian rocks at Site 530, relatively thin layers of black shales are interbedded with thicker layers of organic-carbon- lean green and red claystones (Site 530 summary, this volume). The differences in bulk organic contents and in color indicate changes in depositional conditions and possibly variations in supply of organic matter. Analy- ses of total organic carbon, C/N atomic ratios in organ- ic matter, and lipid composition of samples from closely bedded green and black layers were done to compare the organic matter character of these different rocks. METHODS Six samples were collected on board D/V Glomar Challenger from freshly opened core sections from Hole 530A for the purpose of this comparative study. Two younger Turonian samples, one green clay- stone and one black shale, were selected from Section 530A-95-5. These samples were halved longitudinally and shared between this study and the kerogen study described by Deroo et al. (this volume). Four older Turonian samples from Section 530A-97-1 consist of a green claystone overlying a black shale layer, the top of the black shale layer, the bottom of the black shale layer, and the underlying green claystone. The samples were immediately frozen in heat-sealed Kapak bags and kept frozen until analyzed. Samples were first freeze-dried, and then their total carbon content was measured with a Hewlett-Packard 185B CHN analyzer. Residual carbon was measured after HC1 dissolution of carbonates and was considered to represent the total organic carbon content. Percent cal- 1009
Transcript
  • 32. ORGANIC GEOCHEMICAL COMPARISON OF CRETACEOUS GREEN AND BLACKCLAYSTONES FROM HOLE 530A IN THE ANGOLA BASIN1

    Philip A. Meyers, Oceanography Program, Department of Atmospheric and Oceanic Science,Thomas W. Trull,2 Senior Honors Project, Department of Chemistry

    andOrest E. Kawka,3 Oceanography Program, Department of Atmospheric and Oceanic Science, The University of

    Michigan, Ann Arbor, Michigan

    ABSTRACT

    Three pairs of Upper Cretaceous black shales and adjacent green claystones from Hole 53OA were analyzed to com-pare types and amounts of organic matter and lipids and to seek information about their environments of deposition.The organic-carbon-rich black shales have C/N ratios nearly seven times those of the organic-carbon-lean green clay-stones. The lipid content of organic matter in the black shales is about ten times less than in adjacent green layers. Or-ganic matter in both types of rocks is thermally immature, and distributions of alkanoic acids, alkanols, sterols, and al-kanes contain large amounts of terrigenous components. Pristane/phytane ratios of less than one suggest that youngerTuronian sediments were laid down under anoxic conditions, but ratios greater than one suggest that older TuronianCenomanian deposits accumulated in a more oxic environment. Closely bedded green and black layers have very similartypes of lipid distributions and differ primarily in concentrations, although black shales contain somewhat largeramounts of terrigenous lipid components. Geochemical and stratigraphic evidence suggests much of the organic matterin these samples originated on the African continental margin and was transported to the Angola Basin by turbidityflow. Rapid reburial of organic-carbon-rich sediments led to formation of the black shales.

    INTRODUCTION

    Black shales containing high amounts of organicmatter were deposited in deep waters of the South At-lantic during the Cretaceous period. Occurrences ofblack shale formation are found in the Barremian-Ap-tian at Deep Sea Drilling Project (DSDP) Site 361 in theCape Basin and at Sites 327 and 330 on the FalklandPlateau, in the Albian at Site 363 on the northern flankof Walvis Ridge, in the Turonian-Santonian at Site 356on the Sao Paulo Plateau, and in the Aptian-Albian andTuronian-Santonian at Site 364 in the Angola Basin(Bolli, Ryan et al., 1978). Concentrations of organiccarbon reach as high as 24% dry weight of Aptian sedi-ment at Site 364 (Foresman, 1978). The conditionswhich led to the formation of these organic-carbon-richlayers are not understood, although some combinationof low availability of oxygen and abundant supply oforganic matter seems likely.

    Primary among the scientific goals of DSDP Leg 75was to investigate the Cretaceous paleoceanographicconditions in which black shales were formed. Hay et al.(1982) summarize information obtained from Site 530 inthe Angola Basin where black shale layers were found inthe Albian to early Coniacian. They conclude that or-ganic-carbon-rich sediments accumulated in an oxygenminimum zone of varying intensity on the African con-tinental slope and were redeposited in deep waters by

    1 Hay, W. W., Sibuet, J . -C, et al., Init. Repts. DSDP, 75: Washington (U.S. Govt.Printing Office).

    2 Present address: Woods Hole Oceanographic Institution, Woods Hole, Massachusetts.3 Present address: School of Oceanography, Oregon State University, Corvallis,

    Oregon.

    turbidity flows and slumping. Preservation of organicmatter in the deep-water environment was enhanced byrapid burial in the bottom.

    Organic geochemistry can provide information whichwill help answer some of the questions about blackshales. Evidence of biological sources and of deposi-tional environments is often preserved in the elementaland molecular composition of organic matter in rocksand sediments. In the case of the Aptian to Coniacianrocks at Site 530, relatively thin layers of black shalesare interbedded with thicker layers of organic-carbon-lean green and red claystones (Site 530 summary, thisvolume). The differences in bulk organic contents andin color indicate changes in depositional conditions andpossibly variations in supply of organic matter. Analy-ses of total organic carbon, C/N atomic ratios in organ-ic matter, and lipid composition of samples from closelybedded green and black layers were done to compare theorganic matter character of these different rocks.

    METHODS

    Six samples were collected on board D/V Glomar Challenger fromfreshly opened core sections from Hole 530A for the purpose of thiscomparative study. Two younger Turonian samples, one green clay-stone and one black shale, were selected from Section 530A-95-5.These samples were halved longitudinally and shared between thisstudy and the kerogen study described by Deroo et al. (this volume).Four older Turonian samples from Section 530A-97-1 consist of agreen claystone overlying a black shale layer, the top of the black shalelayer, the bottom of the black shale layer, and the underlying greenclaystone. The samples were immediately frozen in heat-sealed Kapakbags and kept frozen until analyzed.

    Samples were first freeze-dried, and then their total carbon contentwas measured with a Hewlett-Packard 185B CHN analyzer. Residualcarbon was measured after HC1 dissolution of carbonates and wasconsidered to represent the total organic carbon content. Percent cal-

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  • P. A. MEYERS, T. W. TRULL, O. E. KAWKA

    cium carbonate was calculated from the difference between initial andresidual carbon contents. Atomic C/N ratios of organic matter weredetermined from residual carbon CHN values. Percent organic carboncontents of the samples were calculated on a dry-weight basis for theoriginal carbonate-containing sediment.

    A two-stage procedure was used to extract lipids from the freeze-dried samples. Soxhlet extraction with toluene/methanol yielded theeasily extracted materials. A second extraction with 0.5N KOH inmethanol/toluene provided the hydrolyzable fraction of components.These are called the free and bound fractions, respectively, in thischapter and are comparable to the free and bound fractions of Bras-sell et al. (1980). Both fractions were treated with methanolic borontrifluoride to convert fatty acids to their methyl esters, and then lipidsubfractions were separated by column chromatography on silica gel.The classes so obtained contained aliphatic hydrocarbons, fatty acidmethyl esters, and hydroxy lipids, including sterols and alkanols.Hydroxy compounds were silylated with BSTFA prior to gas chroma-tography (GC).

    Splitless injection gas-liquid chromatography was employed to de-termine the types and amounts of compounds comprising the üpid sub-fractions. A Hewlett-Packard 5830 FID gas chromatograph equipped-with a 20 m SE54 glass capillary column was used with hydrogen ascarrier gas. Quantification was accomplished through the use of knownamounts of internal standards added to each sample before columnchromatography and includes corrections for GC response differencesand laboratory contaminants. Individual compounds were tentativelyidentified by GC retention times in this preliminary survey of the lipidcharacter of these rocks.

    RESULTS AND DISCUSSION

    Organic Carbon and C/N Values

    Black shale samples have much higher concentrationsof organic carbon and much higher C/N ratios than dothe green shales (see Table 1). These differences in theamount of organic matter and in its elemental composi-tion are consistent with those found in a large assort-ment of samples from layers of black shales and red andgreen claystones in Cretaceous rocks from Hole 53OA(Site 530 summary; Meyers et al., this volume).

    Concentrations of organic carbon of the green clay-stones average 0.53 % and are only slightly higher thanthe averages of 0.2% found in modern, deep-ocean sedi-ments (Degens and Mopper, 1976) and of 0.3% com-piled by Mclver (1975) from analyses of older marinedeposits from DSDP Legs 1 through 31. The organicmatter in these layers probably was buried in sedimentsdeposited under oxygenated bottom waters, a situationwhich does not favor organic matter preservation (Hin-ga et al., 1979; Cobler and Dymond, 1980; Demaisonand Moore, 1980). This material may have experiencedfurther postdepositional destruction as documented byWaples and Sloan (1980) in samples from DSDP Leg 58.In contrast to the green claystones, the black shalesamples contain concentrations of organic carbon which

    Table 1. General descriptions of samples selected for organic geochem-ical comparison of green and black layers, Hole 53OA.

    Core-Section(interval in cm)

    95-5, 0-2195-5, 38-5097-1, 87-9197-1, 91-9597-1, 99-10597-1, 105-110

    Sub-bottomdepth

    (m)

    101410141027102710271027

    Age

    Younger Turon.Younger Turon.Older Turon.Older Turon.Older Turon.Older Turon.

    Lithology

    Green claystoneBlack shaleGreen claystoneBlack shaleBlack shaleGreen claystone

    CaCO3(%)

    < l< l< l< l< l< l

    Corg

    w0.20

    12.950.584.89

    10.010.80

    C/N

    4.536.06.8

    38.140.3

    5.7

    are unusually high for most marine sediments. Suchhigh values have been reported for only a few modernlocations, generally under anoxic or poorly oxygenatedbottom waters as summarized in Demaison and Moore(1980). An uncommon combination of abundant supplyof organic matter and of exceptional preservation insediments is required for these organic-carbon-rich de-posits to accumulate.

    The contrast in C/N ratios between the green clay-stones and black shales may reflect different amounts ofdiagenesis of organic matter, different sources of organ-ic matter, or some combination of these two possibil-ities. Atomic C/N ratios of the green claystones average5.7 (Table 1), a value similar to those found in DSDPLeg 58 sediments (Waples and Sloan, 1980). Such lowratios reflect greater diagenetic loss of organic carbonthan of nitrogen, because surficial marine sedimentscommonly have C/N ratios in the range of 9 to 18(Stevenson and Cheng, 1972; Muller, 1977). In organic-carbon-lean samples like the green claystones, C/N ra-tios can be affected by the presence of inorganic am-monium and by organic nitrogen compounds sorbed toclay minerals (Muller, 1977), and thus they may not bereliable indicators of sources of organic matter. In thecase of the organic-carbon-rich black shales, however,the high concentrations of organic matter override theeffects of these minor nitrogen contributions. The atom-ic C/N ratios average 38.1 in the black shales and mayindicate an important land-plant contribution to thesediment organic matter (cf. Muller, 1977). Carbon iso-topic analyses of DSDP Leg 40 samples also suggest thepossibility of terrigenous material in black shales depos-ited during Cretaceous times in the Angola Basin (Fores-man, 1978; Simoneit, 1978a). However, Hinga et al.(1979) report elemental analyses of diatom debris fromsediment traps in the North Atlantic Ocean which yieldatomic C/N ratios of 28 to 54, and Dean et al. (1981)show a correlation between high organic-carbon contentand greater depletion in 13C in mid-Cretaceous marinelimestones samples from the Hess Rise during DSDPLeg 62. Evidently, much remains to be learned aboutthe effects of diagenesis upon elemental and isotopiccompositions of organic matter, and C/N ratios andcarbon isotopic data must be interpreted with caution.

    Free and Bound Lipid Components—General

    Representative chromatograms of lipid fractions arepresented in Figure 1. Identification and quantificationof individual lipid components are based upon inte-grated peak areas from such chromatograms with cor-rections for mass discrimination over the fairly broadmolecular weight range surveyed. Identifications mustbe considered tentative until verified by combined gaschromatography-mass spectrometry analyses now under-way. Laboratory contamination of samples was minor,and corrections have been made for it in our data. Noobvious evidence of shipboard contamination was ob-served (cf. Doran and Johnson, 1979).

    Lipid contents of the green claystones and blackshales analyzed in this chapter are summarized in Table2. In general, free lipids are at higher concentrations

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  • CRETACEOUS CLAYSTONES

    Table 2. Summary of geolipid contents of samples of green claystones and black shales, Hole 53OA.

    Geolipid component

    Hydrocarbons

    Total, µg/g sedimentTotal, mg/g C o r gn-alkanes, µg/g sediment/i-alkanes, mg/g C o r gPristane/phytanePristane/n-Ci7

    «-C29/π-c17CPI (16-32)

    Fatty acids

    Total, µg/g sedimentTotal, mg/g C o r gn-alkanoics, µg/g sedimentn-alkanoics, mg/g C o r g«-C26/«-Ci6CPI (16-32)

    Alkanols and sterols

    Total, µg/g sedimentTotal, mg/g C o r gn-alkanols, µg/g sedimentn-alkanols, mg/g C o r gn-C28/n-Ci6CPI (16-32)Sterols, µg/g sedimentSterols, mg/g C o r g

    95-5,

    Green

    Free

    0.86

    3.41.72.11.00.274.2

    0.400.200.0660.0330.19

    310.0260.013

    0-21

    claystone

    Bound

    1.8

    2.81.41.71.30.127.1

    0.760.380.100.0511.37.30.0690.035

    95-5.

    Black

    Free

    0.83

    6.70.0524.80.0370.632.1

    5.10.039

    38-50

    shale

    Bound

    3.80.0292.70.0210.332.0

    2.00.0150.120.0011.33.10.200.001

    97-1,

    Green

    Free

    6.91.21.80.311.62.16.50.94

    2.30.401.50.260.374.6

    1.60.280.120.0211.3

    a0.160.028

    Sample(interval in cm)

    87-91

    claystone

    Bound

    0.840.140.280.0480.750.507.80.95

    1.40.240.690.120.0836.2

    1.50.260.130.0224.0

    170.0430.007

    97-1,

    Black

    Free

    450.928.40.171.73.24.01.6

    6.50.134.00.0821.082.6

    4.60.0940.200.0041.7

    160.610.013

    91-95

    shale

    Bound

    1.70.0350.220.0043.19.40.0720.001

    97-1,

    Black

    Free

    1801.8

    270.271.32.51.51.8

    11.00.115.10.0510.742.2

    8.60.0860.590.0067.72.71.40.014

    99-105

    shale

    Bound

    0.850.0080.350.0030.910.678.31.1

    2.90.0292.10.0210.242.4

    2.90.0290.230.0022.04.30.210.002

    97-1,

    Green

    Free

    354.45.70.711.22.40.560.66

    3.50.442.30.290.4103.7

    3.00.380.460.0585.9

    160.320.040

    105-110

    claystone

    Bound

    0.880.110.320.400.900.770.690.73

    1.70.211.00.130.0744.5

    1.00.130.0630.0080.666.20.0170.002

    Note: Blank space = not determined.a No odd-chain n-alkanols were detected.

    than are bound lipids. This is especially true for thehydrocarbon fraction of total, or free plus bound,lipids. Free-to-bound ratios of concentrations range be-tween 0.5 to 3.8 for fatty acids and alcohols and be-tween 8 and over 200 for hydrocarbons. No consistentdifference in this ratio exists between green and blacklayers. Concentrations of each lipid fraction per weightof dry rock are generally greater in black shales than ininterbedded green claystones. However, the converse isfound when concentrations are expressed in milligramslipid per gram organic carbon, showing that the organ-ic-carbon-rich black shales are lean in lipid componentsrelative to other forms of organic matter. Degradationof nonlipid materials is the probable cause for greenclaystones to have higher proportions of lipid compo-nents. Among the lipid components, hydrocarbons havethe greatest concentration, fatty acids are intermediate,and alcohols have the smallest concentration. Withinthe alcohol fractions, sterols and n-alkanols generallyhave roughly similar total concentrations.

    Aliphatic Hydrocarbons

    Ratios of biomarker hydrocarbons extracted fromsediments and sedimentary rocks are commonly used toprovide information about sources of organic matter,paleoenvironmental conditions of sedimentation, anddiagenesis of organic matter. Pristane-to-phytane ratiosless than one suggest anoxic depositional environments

    whereas ratios greater than one indicate oxic conditions(Didyk et al., 1978). The values in Table 2 from Section530A-95-5 are about 0.85 for free hydrocarbons and 1.8for bound hydrocarbons, and those from Section 53OA-97-1 are between 1.2 and 1.7 in the free hydrocarbon ex-tracts and 0.75 to 0.91 in the bound extracts. Adjacentgreen and black samples have essentially the same pris-tane/phytane ratios. Because free hydrocarbons havehigher concentrations than do the bound fractions, theirmarker compounds are probably more representative ofthe total extractable organic matter in these samples.

    The low pristane/phytane ratios in the free hydrocar-bon fractions of Samples 53OA-95-5,0-21 cm, and 53OA-95-5, 38-50 cm suggest that the organic matter in boththese Turonian samples was buried under anoxic condi-tions. However, the green layer (Sample 53OA-95-5, 0-21 cm) was bioturbated, and so lack of oxygen musthave been confined to the sediments. Other investiga-tors have reported low pristane/phytane ratios in Creta-ceous rocks from the Atlantic. For example, ratios of0.6 and 0.3 have been measured in an Aptian blackmudstone from DSDP Site 364 in the Angola Basin (Si-moneit, 1978a) and for a Cenomanian black shale fromDSDP Site 367 (Didyk et al., 1978), respectively, and in-dicate anoxic conditions accompanying deposition ofthese other organic-carbon-rich samples.

    In contrast to Section 53OA-95-5, the free hydrocar-bon pristane/phytane ratios suggest at least mildly oxy-

    1011

  • P. A. MEYERS, T. W. TRULL, O. E. KAWKA

    14

    14

    Sample 530A-97-1,105-110 cmFree hydrocarbons

    29 31

    Sample 530A-97-1,105-110 cmFree acids

    16 17I.S. 18I

    22 24 26

    20

    Sample 530A-97-1, 105-110 cmFree alcohols

    II I.S.

    28

    1/

    30

    Figure 1. Representative chromatograms of hydrocarbon, fatty acid (as methyl esters), and fatty alcohol plus sterol (as BSTFA ethers)fractions of free and bound extracts. (GC conditions: 20m SE54 glass capillary column, hydrogen carrier gas at 2 ml/min., 70 to270°C at 4°C/min. Major straight-chain components are identified by carbon numbers.)

    1012

  • CRETACEOUS CLAYSTONES

    17 19 21

    PR PH

    23

    25

    Sample 530A-97-1,105-110 cmBound hydrocarbons

    SQ

    27

    29

    31

    33

    14 16 17I.S. 18

    18:1

    22

    20

    ^-üW-'v^>~A~

    Sample 530A-97-1,105-110 cmBound acids

    30

    14

    16

    Figure 1. (Continued).

    18

    VA/—Λ/

    22

    I.S.(5αCholestane)

    Sample 530A-97-1,105-110 cmBound alcohols

    Cholesterol

    1013

  • P. A. MEYERS, T. W. TRULL, O. E. KAWKA

    genated depositional environments during Cenomaniantimes for both the green claystones and the black shalesin Section 530A-97-1. However, this interpretation con-flicts with the abundance of sulfur present as pyrite inthe black shales (Hay et al., 1982; Site 530 summary,this volume), the presence of porphyrins indicated bystrongly colored red bands observed in column chroma-tography of the extracts from black shales, and the highconcentrations of organic carbon in the black shales, allof which suggest anoxic conditions within the sediments(Didyk et al., 1978). The discrepancy between the pris-tane/phytane ratios and other anoxic/oxic indicators inSection 530A-97-1 may result from thermal enhance-ment of this ratio similar to that observed by Simoneit etal. (1981) in Cretaceous black shale samples from near adiabase intrusion at DSDP Site 368. However no intru-sions are known at DSDP Site 530, and other organicmatter parameters remain to be examined to test thispossibility.

    A high proportion of land-derived organic mattermay dilute lipid input from marine algae and result inhigher values of the pristane/w-heptadecane ratio inocean sediments (Didyk et al., 1978). The high values inthe free hydrocarbon fractions in rocks from Section530A-97-1 (Table 2) suggest large contributions of ter-rigenous organic matter to both green claystones andblack shales. Bound hydrocarbon fractions have ratiosbelow one and evidently contain proportionately morealgal and microbial organic matter.

    Another measure of terrigenous vs. aquatic hydrocar-bon origin is the ratio of C2 9/C1 7 w-alkanes. Land plantscommonly have w-alkane distributions dominated byC2 7, C29, and C3i hydrocarbons, whereas algae containmostly shorter-chain w-alkanes (Simoneit, 1978b); there-fore, high C29/Q7 ratios may indicate large terrigenouscontributions of organic matter. In Samples 530A-97-1,87-91 cm and 530A-97-1, 91-95 cm, this ratio suggestsmajor amounts of land-derived components in the hy-drocarbon contents of the green claystone and underly-ing black shale. Sample 530-97-1, 99-105 cm is from thebase of a black shale layer 14-cm thick and may containabout equal portions of terrigenous and aquatic hydro-carbons. The underlying green claystone sample, Sam-ple 530A-97-1, 105-110 cm, has a C2 9/C1 7 ratio whichindicates predominance of algal hydrocarbons. How-ever, preferential losses of n-C17 relative to longer-chainrt-alkanes (cf. Giger et al., 1980) may result in the C29/C1 7 ratio presenting an exaggerated indication of theoriginal proportion of land-derived material.

    Evidence of alteration of w-alkanes can be given bycarbon preference indices (CPI) of hydrocarbon ex-tracts from rocks (Bray and Evans, 1961). In general,hydrocarbons in young marine sediments have relativelyhigh CPI values and those in thermally mature rockshave values close to one. Hunt (1979) notes that in situa-tions where essentially no land-derived organic matter ispresent the CPI value of young sediment can be as lowas one, but this is rarely found and does not seem to bethe case at Site 530. The CPI's of the green claystonesfrom Section 530A-97-1 are quite low and may reflectconsiderable hydrocarbon diagenesis in these samples.The black shales from this section have somewhat high-

    er CPI values, indicating less hydrocarbon maturationor alteration. This difference is consistent with the dif-ference in overall preservation of organic matter in thetwo types of rocks as evidenced by their organic carbonconcentrations.

    Distributions of free n-alkanes of samples from Sec-tion 530A-97-1 are bimodal (Fig. 2), showing both algal(C17 to C19) and land plant (C27 to C31) inputs. Boundn-alkanes do not have strongly bimodal distributions. Inthe green claystones, the bound distributions have max-ima at shorter chain lengths than in the correspondingfree fraction. The distribution of bound H-alkanes inSample 530A-97-1, 99-105 cm, a black shale, is skewedtowards longer chain-length components, and in generalall of the n-alkane distributions of the black shale sam-ples seem to contain more land plant materials than dothe green claystones.

    Fatty Acids

    As indicated by low values of the C2 6/C1 6 n-alkanoicacid ratios (Table 2), the major constituents of fatty aciddistributions are shorter-chain /i-alkanoic acids. Themajor component in five of the six free acid fractionsand in all of the bound fractions is «-C16 acid (Fig. 3).Bimodal distributions containing algal (C16, C18) andterrigenous (C^ to C32) acids make up the free fractionsand resemble the fatty acid distribution of an Aptianblack mudstone from DSDP Site 364 in the Angola Ba-sin (Simoneit, 1978a). Bound fractions have smallercontributions of land-plant long-chain acids than do thefree fractions. A similar difference between distribu-tions of free and bound acids is reported by Brassell etal. (1980) in Pleistocene-to-Miocene samples fromDSDP Site 440 in the Japan Trench. This differencesuggests a more autochthonous origin for the boundfractions of lipids in DSDP samples. Peaks having re-tention times corresponding to those of unsaturated andbranched acids were present in most of the fatty acidchromatograms, but identification of these acids awaitsfurther analysis.

    Distributions of acids in the green claystones and inthe adjacent black shales are not the same. Black shalescontain relatively larger proportions of long-chain ter-rigenous π-alkanoic acids. Because postdepositionaldegradation would preferentially destroy shorter-chainacids (cf. Matsuda and Koyama, 1977), rocks in whichorganic matter is poorly preserved should retain fewerof these acids than would rocks in which degradationhas been retarded. If the original acid contents of thegreen and black layers had been similar, those of the or-ganic-carbon-lean green claystones should now have rel-atively small contributions of C1 6 and C1 8 components,and this is not the case. On this basis, the difference indistributions probably reflects the input of more land-plant acids to the black shales than to the green clay-stones rather than being a diagenetic result. These ter-rigenous materials may have been originally depositedon the African continental margin and become trans-ported to their present location by turbidity flow.

    CPI values of free acids average 4.2 for the greenclaystones and 2.3 for the black shales. In the boundfractions, the respective mean CPI values are 5.9 and

    1014

  • CRETACEOUS CLAYSTONES

    Sample97-1,87-91 cm

    15 17 19 21 23 25 27 29 31 33 35 15 17 19 21 23 25 27 29 31 33 35

    Sample97-1,105-110 cm

    15 17 19 21 23 25 27 29 31 33 35Alkane chain length

    15 17 19 21 23 25 27 29 31 33 35Alkane chain length

    Figure 2. «-Alkane distributions in free (open bars) and bound (hachured bars) extracts of hydrocarbons fromgreen claystones (left) and black shales (right).

    16 18 20 22 24 26 28 30 32 34

    16 18 20 22 24 26 28 30 32 34

    16 18 20 22 24 26 28 30 32 34Fatty acid chain length

    16 18 20 22 24 26 28 30 32 34

    16 18 20 22 24 26 28 30 32 34

    16 18 20 22 24 26 28 30 32 34Fatty acid chain length

    Figure 3. n-Alkanoic acid distributions in free (open bars) and bound (hachured bars) extracts of fatty acidsfrom green claystones (left) and black shales (right).

    1015

  • P. A. MEYERS, T. W. TRULL, O. E. KAWKA

    2.3. Although the higher CPI's of the green claystonesreflect the large contributions of n-C16 and «-C18 acids,more odd-chain alkanoic acids appear in the black shaledistributions than in those of the green claystones (Fig.3). These odd-chain components are especially evidentfrom «-C19 to Λ-C2 3 and may be diagenetically derivedfrom longer-chain acids.

    Alkanols

    Most distributions of «-alkanols contain large contri-butions of C1 6, C22, and C2 8 (Fig. 4). The ratio of n-C2$to «-C16 is used in Table 2 as an indicator of land plantversus aquatic alkanols. Although this ratio makes nodistinction between black shale and green claystone norbetween free and bound alkanols, it does show an im-portant contribution of terrigenous material in most ofthe samples. This conclusion is supported by the abun-dance of n-C26, n-C2$, and /2-C3O in these samples (Fig.4). The alkanol distributions of the black shales in par-ticular differ from those found in Pleistocene-to-Mio-cene samples from DSDP Site 362 (Boon et al., 1978)and from DSDP Site 440 (Brassell et al., 1980) in whichn-C22 and n-C^ dominate. As also seen in the fatty acid

    contents, the alkanols indicate more terrigenous mate-rial in the black shales than in the green claystones.

    Alkanol CPI values in Table 2 are higher than CPI'sof alkanes or alkanoic acids from the same samples.Green claystones have higher CPI's than do their adja-cent black shales, and free fractions usually have higherCPI's than found for bound alkanols. The lower valuesof the black shales is similar to the lower alkanoic acidCPI values and may also be the result of diagenetic pro-duction of odd-chain components from longer-chainprecursors. Because few reports of n-alkanol contentsof ancient rocks exist, it is difficult to interpret theseCPI values. However, the strong predominance of even-chain components in both the black shales and the greenclaystones seems remarkable. It may be that diagenesisof alkanols does not form shorter-chain homologs butinstead decreases the overall amount of alkanols whilenot greatly modifying the original biogenic character.

    Sterols

    Contributions of C2 7, C2 8, and C2 9 components to thetotal concentrations of sterols were compared by thescheme of Huang and Meinschein (1979). For this com-

    i π

    if1ül

    Sample95-5, 0-21 cm

    I p'P pp f

    Sample95-5, 38-50 cm

    16 18 20 22 24 26 28 30 32 16 18 20 22 24 26 28 30 32

    Sample97-1,87-91 cm

    ill k • f

    Sample97-1, 91-95 cm

    16 18 20 22 24 26 28 30 32 16 18 20 22 24 26 28 30 32

    [i.k

    Sample97-1, 105-110 cm

    16 18 20 22 24 26 28 30 32Alkanol chain length

    Sample97-1, 99-105 cm a

    16 18 20 22 24 26 28 30 32Alkanol chain length

    Figure 4. n -Alkanol distributions in free (open bars) and bound (hachured bars) extracts of alcohols fromgreen claystones (left) and black shales (right).

    1016

  • CRETACEOUS CLAYSTONES

    parison, all diene and monoene stenols and stanols hav-ing the same carbon number were tentatively identifiedby GC retention times and their contributions added to-gether. The comparison (Fig. 5) shows that C28 sterolsare not abundant in any of these Cretaceous samplesand that C27 and C28 sterols contribute about equally tothe totals. Except for the free sterol fractions of twogreen clay stones, most of the samples have similar com-positions in both the free and bound fractions. How-ever, these sterol compositions do not resemble thosereported by Huang and Meinschein in modern sedi-ments, indicating that the original sterol contents ofthese sedimentary rocks have been modified. It is possi-ble that sterane distributions, which remain to be de-termined, will provide better source information, asdid those found in the Cretaceous Viking Formation ofCanada (Huang and Meinschein, 1979).

    Ratios of C29/C27 stenols range from 0.07 to 2.3 inthe free fraction and from 0.08 to 1.1 in the bound.They show no relationship to green or black sample col-or, nor do the ratios of the free and bound fractions ofan individual sample appear to be related. Stenol/stanolratios are between 1.3 and 35 for C27 sterols and 0.09and 2.8 for C29 sterols. The large proportion of un-saturated sterols in many of these rocks is surprising inview of the rapid decrease in stenol/stanol ratios usuallyfound in young marine sediments (Huang and Mein-schein, 1978). Although it is tempting to conclude thatthe presence of these unsaturated molecules in the blackshales results from exceptional preservation of organic

    matter, their existence in the organic-carbon-lean greenclaystones is paradoxical. These preliminary sterol iden-tifications evidently require further investigation.

    CONCLUSIONS

    Upper Cretaceous black shales contain higher con-centrations of organic carbon and have higher organicmatter C/N ratios than do adjacent green clay stonelayers. Lipid contents of both types of rocks consist ofsimilar distributions of marine and terrigenous compo-nents, but black shales have somewhat larger propor-tions of terrigenous n-alkanes, /z-alkanoic acids, andw-alkanols than are found in green claystones. The lipidcontribution to total organic matter is less in the blackshales than in the organic-carbon-lean green claystones,indicating enhanced preservation of nonlipid matter inthe black shales and general thermal immaturity of thesesamples.

    The rocks in this study were deposited in the earlyAngola Basin as turbidites whose source is believed tobe on the African continental margin (Hay et al., 1982;Site 530 summary, this volume). The interbedding ofthin layers (1 to 15 cm) of black shales in thicker layersof green and red claystones and the presence of abun-dant bioturbation rules out the possibility of perma-nently anoxic bottom waters during Turonian time. Sed-iments rich in organic matter may have accumulatedwhere an extended and intensified oxygen minimumzone impinged on the ocean bottom in midwater depths(Demaison and Moore, 1980; Dean et al., 1981). Rede-

    Green Claystones1. Sample 530A-95-5, 0-21 cm3. Sample 530A-97-1, 87-91 cm6. Sample 530A-97-1, 105-110 cm

    Black Shales2. Sample 530A-95-5, 38-50 cm4. Sample 530A-97-1, 91-95 cm5. Sample 530A-97-1, 99-105 cm

    100 100

    Figure 5. Total C27, C28, and C29 sterol distributions in free and bound extracts from green claystones andblack shales.

    1017

  • P. A. MEYERS, T. W. TRULL, O. E. KAWKA

    position of these sediments in deeper waters could thenhave occurred by turbidity flow, and subsequent preser-vation of organic matter could have been achieved byrapid burial in a nominally oxic environment.

    Differences between the green and black layers sug-gest that variability existed in depositional conditions. Ifthese turbidites came from the same source, then theremust have been major fluctuations in the oxygen mini-mum zone in response to changes in the supply of ter-restrial and/or aquatic organic matter. If they had dif-ferent sources, then the organic-carbon-rich sedimentscame from a site which received more land-derived ma-terial. Organic geochemical data from this investigationsuggests that the black shales contain more terrestrialorganic matter than do the green claystones. Finally,younger Turonian sediments (Section 530A-95-5) mayhave been deposited under anoxic conditions on the ba-sis of pristane/phytane ratios, whereas older Turonian.sediments (Section 530A-97-1) were laid down undermildly oxic conditions. This difference points out thatthe conditions leading to black shale formation need nothave been the same at all times or at all locations in theoceans.

    ACKNOWLEDGMENTS

    We thank W. E. Dean, M. J. Leenheer, J. Rullkötter, and B. R. T.Simoneit for suggesting improvements to the manuscript. We aregrateful to the Deep Sea Drilling Project (International Phase ofOcean Drilling) for making possible the participation of P. A. Meyerson board D/V Glomar Challenger during Leg 75.

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    Bolli, H. M., Ryan, W. B. F., and the Shipboard Scientific Party, 1978.Angola continental margin: Sites 364 and 365. In Bolli, H. M.,Ryan, W. B. F., et al., Init. Repts. DSDP, 40: Washington (U.S.Govt. Printing Office), 357-455.

    Boon, J. J., van der Meer, F. W., Schuyl, P. J. W., de Leeuw, J. W.,Schenck, P. A., and Burlingame, A. L., 1978. Organic geochemi-cal analyses of core samples from Site 362, Walvis Ridge, DSDPLeg 40. In Bolli, H. M., Ryan, W. B. F., et al., Init. Repts. DSDP,Suppl. to Vols. 38, 39, 40, and 41: Washington (U.S. Govt. Print-ing Office), 627-637.

    Brassell, S. C , Comet, P. A., Eglinton, G., Isaacson, P. J., McEvoy,J., Maxwell, J. R., Thomson, I. D., Tibbetts, P. J. C , and Volk-man, J. K., 1980. Preliminary lipid analyses of Sections 440A-7-6,440B-3-5, 440B-8-4, 440B-68-2, and 436-11-4: Legs 56 and 57,Deep Sea Drilling Project. In Scientific Party, Init. Repts. DSDP,56, 57, Pt. 2,: Washington (U.S. Govt. Printing Office), 1367-1390.

    Bray, E. E., and Evans, E. D., 1961. Distribution of «-paraffins as aclue to recognition of source beds. Geochim. Cosmochim. Acta,22:2-15.

    Cobler, R., and Dymond, J., 1980. Sediment trap experiment on theGalapagos Spreading Center, equatorial Pacific. Science, 209:801-803.

    Dean, W. E., Claypool, G. E., and Thiede, J., 1981. Origin of organ-ic-carbon-rich mid-Cretaceous limestones, mid-Pacific mountainsand southern Hess Rise. In Thiede, J., Valuer, T. L., et al., In-

    it. Repts. DSDP, 62: Washington (U.S. Govt. Printing Office),877-890.

    Degens, E. T., and Mopper, K., 1976. Factors controlling the distri-bution and early diagenesis of organic material in marine sedi-ments. In Riley, J. P., and Chester, R. (Eds.), Chemical Oceanog-raphy (Vol. 6): New York (Academic Press), 59-113.

    Demaison, G. J., and Moore, G. T., 1980. Anoxic environments andoil source bed genesis. Org. Geochem., 2:9-31.

    Didyk, B. M., Simoneit, B. R. T., Brassell, S. C , and Eglinton, G.,1978. Organic geochemical indicators of palaeoenvironmentalconditions of sedimentation. Nature, 272:216-222.

    Doran, T., and Johnson, P. G., 1979. Examination of potential geo-chemical contaminants in Leg 48 material. In Montadert, L.,Roberts, D. G., et al., Init. Repts. DSDP, 48: Washington (U.S.Govt. Printing Office), 1157-1160.

    Foresman, J. B., 1978. Organic geochemistry DSDP Leg 40, con-tinental rise of southwest Africa. In Bolli, H. M., Ryan, W. B. F.et al., Init. Repts. DSDP, 40: Washington (U.S. Govt. PrintingOffice), 557-567.

    Giger, W., Schaffner, C , and Wakeham, S. G., 1980. Aliphatic andolefinic hydrocarbons in recent sediments of Greifensee, Switzer-land. Geochim. Cosmochim. Acta, 44: 119-129.

    Hay, W. W., Sibuet, J.-C, and the Shipboard Scientific Party, 1982.Sedimentation and accumulation of organic carbon in the AngolaBasin and on Walvis Ridge: Preliminary results of Deep Sea Drill-ing Project Leg 75. Geol. Soc. Am. Bull., 93:1038-1058.

    Hinga, K. R., Sieburth, J. McN., and Heath, G. R., 1979. The supplyand use of organic material at the deep-sea floor. / . Mar. Res., 37:557-579.

    Huang, W.-Y., and Meinschein, W. G., 1978. Sterols in sediments ofBaffin Bay, Texas. Geochim. Cosmochim. Acta, 42:1391-1396.

    , 1979. Sterols as ecological indicators. Geochim. Cosmoch-im. Acta, 43:739-745.

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    Mclver, R., 1975. Hydrocarbon occurrences from JOIDES Deep SeaDrilling Project. Proc. Ninth World Pet. Congr., pp. 269-280.

    Matsuda, H., and Koyama, T., 1977. Early diagenesis of fatty acidsin lacustrine sediments: I. Identification and distribution of fattyacids in recent sediment from a freshwater lake. Geochim.Cosmochim. Acta, 41:777-783.

    Muller, P. J., 1977. C/N ratios in Pacific deep-sea sediments: Ef-fect of inorganic ammonium and organic nitrogen compoundssorbed by clays. Geochim. Cosmochim. Acta, 41:765-776.

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    Simoneit, B. R. T., Brenner, S., Peters, K. E., and Kaplan, I. R.,1981. Thermal alteration of Cretaceous black shale by diabase in-trusions in the eastern Atlantic: II. Effects on bitumen and kero-gen. Geochim. Cosmochim. Acta, 45:1581-1602.

    Stevenson, F. J., and Cheng, C.-N., 1972. Organic geochemistry ofthe Argentine Basin sediments: Carbon-nitrogen relationships andQuaternary correlations. Geochim. Cosmochim. Acta, 36:653-671.

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    Date of Initial Receipt: June 22, 1982

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