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The Effect of Provenance on Clay Mineral Diagenesis in Gulf of Mexico Shales Matthew W. Totten, Sr. 1 , Joniell Borges 2 , and Iris M. Totten 1 1 Department of Geology, Kansas State University, Manhattan, Kansas 66506 2 Department of Geological Sciences, Northwestern University, Evanston, Illinois 60208 ABSTRACT This study examines 43 samples from drill cuttings from an offshore well in the Ship Shoal area, Gulf of Mexico. The mudrock samples were taken from a depth interval of 4800-13,600 ft (1463-4146 m), with the deepest sample penetrating the upper Miocene series. Previously reported work on the same samples (Totten et al., 2002) confirmed diagenetic growth of illite at the expense of smectite with increasing depth. The amount of K 2 O varies between 2.5 to 3.6 weight % and also increases with depth. However, only 17% of the increase is depth related (R 2 = 0.17). In contrast, none of the other major elements correlate with depth. Provenance analyses of heavy-mineral suites suggest an increase in the amount of sediment derived from a felsic source in deeper parts of the well. This is also supported by the increase of incompatible trace elements when compared to compatible elements at greater depths. Because felsic rocks contain a higher percentage of potassium-bearing minerals, the K 2 O variation may therefore be directly related to changes in provenance. The K 2 O required to drive the smectite-illite transformation reaction in these rocks could be acquired from potassium-rich minerals that were originally present in the mud- rock. INTRODUCTION The transformation from smectite to illite during burial diagenesis in mudrocks has been well established since the pioneering work of Hower et al. (1976). Several mechanisms have been proposed for the conversion of smectite to illite. Most call upon the dissolution of K-feldspar to partially provide the necessary potassium and aluminum (e.g., Boles and Franks, 1979). The problem is that illitization is not complete even after all of the K- feldspar is gone. Pollastro (1985) suggested that mixed-layer clays dissolve to provide the additional elements. In a similar fashion, Totten and Blatt (1993) proposed cannibalization of existing illites to illitize any remaining smectite layers. This idea is supported by the observed decrease in total clay percentage with depth. Berger et al. (1999) and Cuadros and Altaner (1998) have suggested the discrete formation of illite and formation of illite from kaolinite. There are many additional articles on the subject, too many to cite, most addressing the source of re- quired elements (potassium and aluminum), or speculating on the sinks for released elements, mainly silicon (e.g., Totten and Blatt, 1996). Many studies report an increase in whole-rock K 2 O with increased depth, and suggest that the increased K 2 O reflects an external source of potassium introduced to the rock after burial (Berger et al., 1999; Gier, 1998; Land et al., 1997; Awwiller, 1993). These authors conclude that mudrocks behave as open systems during burial diagenesis. The elements involved in the conversion of smectite to illite are free to come and go as required. The Totten, M. W., Sr., J. Borges, and I. M. Totten, 2007, The effect of provenance on clay mineral diagenesis in Gulf of Mex- ico shales: Gulf Coast Association of Geological Societies Transactions, v. 57, p. 699-716. 699
Transcript

The Effect of Provenance on Clay Mineral Diagenesis in Gulf of Mexico Shales

Matthew W. Totten, Sr.1, Joniell Borges2, and Iris M. Totten1

1Department of Geology, Kansas State University, Manhattan, Kansas 66506

2Department of Geological Sciences, Northwestern University, Evanston, Illinois 60208

ABSTRACT This study examines 43 samples from drill cuttings from an offshore well in the Ship

Shoal area, Gulf of Mexico. The mudrock samples were taken from a depth interval of 4800-13,600 ft (1463-4146 m), with the deepest sample penetrating the upper Miocene series. Previously reported work on the same samples (Totten et al., 2002) confirmed diagenetic growth of illite at the expense of smectite with increasing depth. The amount of K2O varies between 2.5 to 3.6 weight % and also increases with depth. However, only 17% of the increase is depth related (R2 = 0.17). In contrast, none of the other major elements correlate with depth.

Provenance analyses of heavy-mineral suites suggest an increase in the amount of sediment derived from a felsic source in deeper parts of the well. This is also supported by the increase of incompatible trace elements when compared to compatible elements at greater depths. Because felsic rocks contain a higher percentage of potassium-bearing minerals, the K2O variation may therefore be directly related to changes in provenance. The K2O required to drive the smectite-illite transformation reaction in these rocks could be acquired from potassium-rich minerals that were originally present in the mud-rock.

INTRODUCTION

The transformation from smectite to illite during burial diagenesis in mudrocks has been well established

since the pioneering work of Hower et al. (1976). Several mechanisms have been proposed for the conversion of smectite to illite. Most call upon the dissolution of K-feldspar to partially provide the necessary potassium and aluminum (e.g., Boles and Franks, 1979). The problem is that illitization is not complete even after all of the K-feldspar is gone. Pollastro (1985) suggested that mixed-layer clays dissolve to provide the additional elements. In a similar fashion, Totten and Blatt (1993) proposed cannibalization of existing illites to illitize any remaining smectite layers. This idea is supported by the observed decrease in total clay percentage with depth. Berger et al. (1999) and Cuadros and Altaner (1998) have suggested the discrete formation of illite and formation of illite from kaolinite. There are many additional articles on the subject, too many to cite, most addressing the source of re-quired elements (potassium and aluminum), or speculating on the sinks for released elements, mainly silicon (e.g., Totten and Blatt, 1996).

Many studies report an increase in whole-rock K2O with increased depth, and suggest that the increased K2O reflects an external source of potassium introduced to the rock after burial (Berger et al., 1999; Gier, 1998; Land et al., 1997; Awwiller, 1993). These authors conclude that mudrocks behave as open systems during burial diagenesis. The elements involved in the conversion of smectite to illite are free to come and go as required. The

Totten, M. W., Sr., J. Borges, and I. M. Totten, 2007, The effect of provenance on clay mineral diagenesis in Gulf of Mex-ico shales: Gulf Coast Association of Geological Societies Transactions, v. 57, p. 699-716.

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assumption is that the provenance of deeper samples has not varied greatly from the shallower samples; therefore, any chemical differences are attributed to open system behavior.

Bloch et al. (1998) has questioned this assumption with respect to Gulf of Mexico shales. They suggest that increased orogenic activity during the Laramide orogeny in the early Cenozoic provided more potassium to the basin because of the increased felsic igneous production in the source area. Lynch et al. (1999) countered this idea and reaffirmed the original consensus that little provenance variation exists during much of the Tertiary in south Texas. Additional work regarding the control of provenance versus diagenesis on the reported varaiations in Gulf of Mexico mudrocks are needed to resolve this question.

Heavy mineral investigations have been used for nearly a century to determine the provenance of sandstones. Most studies concentrate on the non-opaque mineral fraction. Other studies reveal variations in the mineralogical and chemical characteristics of opaque heavy minerals and have established their usefulness for provenance dis-crimination (Schneiderman, 1995; Grigsby, 1990; Basu and Molinaroli, 1989; Hiscott, 1984). Examination of the heavy-mineral fraction from Paleozoic shales discloses a variety of heavy minerals, comparable to the heavy frac-tion in sandstones (Hanan and Totten, 1996). A recent study used heavy minerals as provenance indicators in shales from the Ouachita Mountains (Totten et al., 2000).

The whole-rock trace element geochemistry of shales has also been used to determine provenance. Most useful are ratios of compatible to incompatible elements (Taylor and McLennan, 1985). Compatible elements (e.g., Cr, V, Ni) are concentrated in mafic igneous rocks while incompatible elements (e.g., Th, La, Zr) are con-centrated in more evolved felsic igneous rocks. Changes in these ratios reflect changes in the provenance of the sediments. The documented open system behavior of sandstones limits the utility of provenance based on trace elements (Milliken et al., 1994); however, they are widely used in shales.

OBJECTIVES

The objectives of this study are to 1) determine the variation in provenance over time within a well in the

Gulf of Mexico, 2) assess the effect of this variation on reported diagenetic trends in mudrocks, and 3) based on these results, determine whether these mudstones behave as an open or closed system.

Provenance will be determined based on the suite of heavy minerals separated from the mudrocks, and also on the distribution of whole-rock trace elements. We hope to test the assumption that provenance varies with time (depth) in the Gulf of Mexico Basin.

GEOLOGIC SETTING The well cuttings used in this study belong to a vertical well in the Ship Shoal area, protraction block num-

ber 97, OCS-G 12936, offshore Louisiana, Gulf of Mexico (Fig. 1). The well is located approximately 10 mi offshore in a water depth < 250 ft (80 m). The well penetrated the upper Miocene as indicated by the presence of the benthic foraminifera, Bolovina thalamannii at a depth of 13,070 ft (3983 m). The total depth of the well was 13,670 ft (4146 m).

The major rivers that currently supply sediment to this area of the Gulf are the Mississippi, Atchafalaya, Red, Sabine, and the Pearl. Over time all have switched the locations of their deltas, spreading the sediment over particular areas during distinct time periods. Each river drains a different source area, so the specific mix of sedi-ment at any geographic location in the Gulf of Mexico is a function of where the rivers were unloading their sedi-ment. Since the position of each river varies over time, it is expected that the sediment should also vary with time. Because time varies with depth in a well, the provenance of the sediment should vary with depth. The more easterly rivers would be expected to have an Appalachian dominated provenance, rich in metamorphic sedi-ments. The Colorado Plateau sources the more westerly rivers, which is mostly a felsic volcanic and plutonic igneous source.

The subsurface stratigraphy of southern Louisiana is not formally divided into formations, but is based on biostratigraphic units. The rocks penetrated by this well are alternating mudrocks and sandstones as seen from the wire-line log. The upper Miocene rocks are mainly deltaic sequences of alternating quartzose sands and clay-rich mudrocks (Anderson, 1976). In the Early Pliocene (indicated by the presence of benthic foraminifera Textu-laria X at 8700 ft or 2650 m), the mudrocks are thinner and the amount of inter-bedded sandstone increases. At

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The Effect of Provenance on Clay Mineral Diagenesis in Gulf of Mexico Shales

Figure 1. Location of well used in this study (modified after Totten et al., 2002).

shallower depths, up to the Pliocene/Pleistocene boundary (Lenticulina at 5000 ft or 1540 m), mudrock and sand-stone are interbedded.

The conversion of smectite to illite has been documented within the same area as this study. Totten et al. (2005) reported an increase in illite-rich mixed layer clays and a corresponding decrease in smectite-rich mixed layers with increasing depth in the adjacent South Timbalier protraction block in a multi-well study. A previous clay mineral study (Totten et al., 2002) of the same Ship Shoal well samples reported an excellent correlation between the percentages of illite-rich layers with depth (Fig. 2).

METHODS The gamma ray and spontaneous potential well logs were used to identify mudrock-rich zones. Mudrock

cuttings were carefully picked using a binocular microscope from sample bags covering 10 meter intervals. Cut-tings were intentionally restricted to those that were angular and had a homogenous gray mudrock appearance. The more rounded mudrock cuttings were left out to avoid any suspected uphole cavings that may have come up with the drilling fluids. The shallowest sampled depth was at 4800 ft (1463 m.). The well was sampled at 200 ft (66 m) intervals, down to the final depth of 13,600 ft (4146 m). A minimum of 7 grams of mudrock was picked from each interval, weighed, and stored in plastic zippered bags.

The mudrock cuttings were crushed using mortar and pestle and stored in small glass vials. The samples were then washed with weak acetic acid solution (pH = 5.6) to remove any adsorbed cations from the surface of the mudrocks. The rinse solution was stored in plastic bottles for later analysis.

Elemental Analyses The major oxides K2O, Na2O, MgO, MnO, and TiO2 concentrations were determined using a Spectrascan®

V direct-coupled spectrometer (DCP). The major oxides SiO2, Al2O3, and CaO, as well as all trace-element con-

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centrations were determined using a Siemens SRS 200® x-ray fluorescence (XRF) spectrometer at the Tulane University CIF Inorganic Laboratory.

Mineral Determinations X-ray diffraction (XRD) techniques were used to study the relative amounts of quartz and K-feldspar. The

XRD analyses were performed on a Scintag XDS-2000® x-ray diffractometer. Peak areas were calculated for the diagnostic peaks of each mineral, and were assumed to approximate the relative proportions of these minerals within the sample.

Heavy mineral separations were accomplished using lithium metatungstate (LMT) after the method of Hanan and Totten (1996). Two grams of ground mudrock sample were weighed and placed in plastic centrifuge tubes that contained LMT adjusted to a specific gravity of 2.85. These tubes were centrifuged for one hour after which the lighter fraction (floating material) was decanted after freezing the material on the bottom of the tube (heavy minerals) with liquid nitrogen. A portion of the heavy minerals were washed, dried, and mounted on a circular glass slide in petropoxy (RI = 1.54) for petrographic microscope reconnaissance and scanning electron microscope analyses.

Heavy minerals were examined using an Amray 1820® digital scanning electron microscope (SEM) with an energy dispersive system (EDS). Heavy minerals were identified by comparing their EDS elemental spectra to EDS spectra obtained from known heavy minerals. The percentages of each heavy mineral species were obtained using the image analyses capabilities of the Iridium IXRF© software which operates the SEM.

Figure 2. Increase in illite-rich mixed layer clays within the mixed layer fraction with depth (modified after Totten et al., 2002).

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RESULTS Whole-rock chemical analyses are presented in Table 1. Major elements are reported in weight percent, and

trace elements in parts per million. The major cation concentrations of the solution washed from the remnant drilling mud are given in Table 2. The area of the characteristic XRD peak for quartz and K-spar is reported in Table 3. The heavy mineral recoveries, as well as the percentage of each mineral species present, are reported in Table 4.

Pyrite was the most abundant of the heavy minerals. Most of the pyrite was authigenic as evidenced by framboids, often present in clusters and distinguishable by their spherical morphology. Ilmenite and TiO2 (reported in Table 4 as rutile) were the next most abundant. Rutile was present in larger quantities than ilmenite. Iron oxides were less common. Opaque heavy minerals were present at all depths. Minerals that were altering (primarily into the formation of iron oxides) were grouped together and called alteration products. The term ‘composites’ was given to those grains that showed the presence of more than one mineral in their EDS spectrum.

Among the micas, biotite was common and was more abundant at deeper depths, whereas muscovite was present only in deeper samples. Chlorite was present at almost all depths. The micas and chlorite had a flaky appearance and were present as relatively coarse grains. The carbonate heavy minerals were mainly ankerite and dolomite. Both ankerite and dolomite decrease in abundance with depth.

DISCUSSION

Influence of Drilling Fluids on Mudrock Fragments

To control the problems encountered while drilling through swelling clays (smectite) most drilling muds

contain KCl solutions to stabilize these clays. We were interested whether these solutions influenced the chemis-try of the clays by increasing the adsorption of K+. Analyses of the rinse solutions did not reveal any significant contamination of K+ or Ca+2 from the drilling fluids (Fig. 3). The potassium concentration averages 100 ppm, not enough to affect the 1-2% increase in K2O down the well. The Na+ concentration of the rinse was present in ex-cess of 1000 ppm and shows a negative correlation with depth.

Mineral Trends with Depth Total areas of diagnostic XRD peaks of the major non-clay minerals were plotted with depth to determine

their relative change (Fig. 4). The intensity of the quartz peak (4.26 Å, angstroms) increases with depth suggest-ing that it becomes more abundant. A corresponding decrease in K-feldspar (3.2 Å) is observed. Our previous work on samples from the same well showed an increase in illite relative to smectite over the same interval (Totten et al., 2002). In addition to increasing in percentage, illite peaks also sharpened with depth, indicating increased crystallinity. We interpret the increase in quartz to be due to the release of silica during the smectite-illite transformation. In contrast, the gradual loss of K-feldspar provided the K2O and Al2O3 for the formation of illite. All of these trends are consistent with reported mineralogical trends during burial diagenesis in mudrocks from the Texas Gulf Coast.

The percentage of the total heavy-mineral fraction within the shale did not show any significant trend with depth. Variation in individual heavy-mineral species was observed, as discussed below.

Chemical Variation with Depth The formation of illite requires the addition of K+ and Al+3, and is accompanied by the release of Si+4, H2O

and other cations like Na+, Ca+2, Mg+2 and Fe+2. The increase in the amount of whole-rock K2O, which is some-times accompanied by the increase of Al2O3, is the most commonly reported chemical change during burial diagenesis (Lynch, 1997; Hower et al., 1976). Our mudrocks show that a weak correlation exists between K2O

The Effect of Provenance on Clay Mineral Diagenesis in Gulf of Mexico Shales

703

Samp # 1 2 3 4 5 6 7 8 9 11 12 13 14 15 16

Depth ft 4800 5000 5200 5400 5600 5800 6000 6200 6400 6800 7000 7200 7400 7600 7800

Depth m 1463 1524 1585 1646 1707 1768 1829 1890 1951 2073 2134 2195 2256 2317 2378 Wt. % Na2O* 1.50 2.41 1.99 1.75 2.08 2.27 2.61 2.12 1.97 1.96 2.13 2.04 2.30 1.77 2.31 MgO* 1.91 2.19 2.30 2.06 2.05 2.15 1.82 2.39 1.98 2.15 2.18 2.60 2.61 1.95 2.04 Al2O3 16.92 18.44 18.44 18.79 18.88 18.03 18.87 17.16 18.19 19.45 16.83 18.28 17.10 18.08 16.94 SiO2 59.74 63.59 62.67 63.58 62.43 65.94 64.95 64.18 63.09 65.15 63.31 62.95 61.64 62.46 61.86 P2O5 0.19 0.12 0.15 0.13 0.16 0.14 0.14 0.15 0.12 0.16 0.18 0.15 0.17 0.17 0.19 SO3 0.73 0.92 0.67 0.69 0.97 0.65 0.62 0.99 0.62 0.90 0.77 1.03 1.00 0.69 0.50 K2O* 2.49 3.07 3.39 2.71 2.80 2.52 2.75 2.70 2.74 3.01 2.81 2.94 2.95 3.08 2.93 CaO 1.87 1.17 1.08 1.13 1.05 0.94 0.91 0.91 1.08 0.97 1.11 1.13 1.00 0.94 1.06 TiO2* 0.59 0.56 0.92 0.83 0.73 0.66 0.59 0.76 0.79 0.64 0.61 0.56 0.62 0.68 0.77 MnO* 0.06 0.07 0.07 0.06 0.06 0.05 0.07 0.07 0.07 0.06 0.04 0.07 0.08 0.07 0.08 FeO* 5.96 6.37 6.26 5.86 5.92 5.34 4.90 5.86 6.56 5.56 5.35 5.44 5.83 5.86 5.67 Sum 91.95 98.90 97.94 97.59 97.13 98.69 98.24 97.29 97.22 100.01 95.33 97.18 95.31 95.75 94.35 ppm Ag nd nd nd nd nd nd nd 0.7 0.5 nd nd 0.5 nd nd nd As 11 9 8 10 11 7 8 7 9 10 8 8 9 10 7 Ba 505 500 465 456 465 618 505 548 452 552 629 550 563 514 479 Bi nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd Br 9 14 5 nd nd 1 nd 1 nd nd nd nd nd nd nd Cd nd nd nd nd 1 nd 1 nd nd nd nd nd nd nd nd Ce 80 85 82 84 82 84 89 93 86 82 82 81 83 91 85 Cl 245 266 320 222 238 217 232 229 264 272 345 259 276 276 247 Co nd nd nd 33 nd nd nd nd 31 37 40 nd nd nd nd Cr 85 76 71 72 79 62 60 68 80 79 82 74 80 87 77 Cs 7 10 7 9 8 10 7 9 8 7 8 8 8 9 9 Cu 24 26 22 24 23 43 25 22 24 24 33 24 22 28 23 Ga 21 21 19 21 22 18 21 20 21 21 20 19 21 22 21 Ge 5 3 3 6 3 0 4 4 6 4 4 4 3 3 3 Hg nd nd nd nd nd nd nd nd nd nd nd nd nd nd I nd nd nd nd nd 2 nd nd nd nd nd nd 2 nd nd In nd nd nd nd nd nd nd nd nd nd nd nd 0 nd nd Mo 5 5 4 5 5 4 3 4 6 4 5 4 6 5 4 La 46 48 47 48 45 48 46 53 50 44 47 46 48 46 50 Nb 17 17 18 19 18 19 21 23 19 19 20 18 20 20 19 Ni 31 24 29 27 29 24 26 27 28 25 31 29 27 30 24 Pb 26 20 27 18 20 39 21 23 19 21 19 18 18 20 19 Rb 139 134 141 139 145 127 141 146 142 147 139 137 142 148 143 Sb 2 2 2 2 2 1 1 2 nd 1 nd nd nd 1 1 Se nd 1 1 nd nd nd nd nd 1 nd nd nd nd nd nd Sn 3 3 3 3 4 3 3 4 4 2 3 3 3 3 3 Sr 152 176 137 133 128 142 139 136 131 142 150 148 126 127 128 Ta nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd Te nd 2 nd nd nd nd nd nd nd nd 2 2 nd nd nd Th 13 14 11 13 14 12 15 14 13 15 14 13 14 14 13 Tl 2 nd nd 2 nd nd nd nd nd nd nd nd nd 2 nd U 5 6 5 6 6 5 7 5 7 6 8 6 6 nd 5 V 123 104 111 116 110 93 101 98 118 116 115 102 109 118 121 W 56 12 11 91 11 14 8 nd 14 8 6 14 12 7 5 Y 31 31 32 31 31 33 35 40 32 34 33 32 32 33 32 Zn 114 100 100 100 105 281 96 96 97 102 96 95 99 96 93 Zr 180 191 190 187 184 213 219 211 181 196 200 190 186 191 195

Table 1. Whole-rock concentration. Asterisk indicates from DCP, and nd indicates not detectable.

Totten et al.

704

Samp # 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32

Depth ft 8200 8400 8600 8800 9000 9200 9400 9600 9800 10000 10200 10400 10600 10800 11000

Depth m 2500 2561 2622 2683 2744 2805 2866 2927 2988 3049 3110 3171 3232 3293 3354 Wt. % Na2O* 2.15 2.26 2.16 2.20 2.48 2.49 2.06 3.01 2.20 2.18 2.29 2.26 2.34 2.39 1.55 MgO* 2.15 1.85 1.85 1.82 1.85 2.10 1.91 1.91 2.36 2.16 2.15 1.79 1.97 2.78 1.62 Al2O3 17.55 18.21 17.10 16.99 16.95 16.64 18.34 17.62 18.45 19.12 17.13 18.37 15.97 17.46 18.18 SiO2 61.13 62.55 59.98 60.29 61.07 61.34 61.75 61.83 62.35 62.45 62.50 63.98 63.06 61.80 61.76 P2O5 0.18 0.17 0.18 0.20 0.18 0.20 0.18 0.17 0.18 0.16 0.18 0.16 0.16 0.18 0.16 SO3 0.32 0.68 0.56 0.49 0.58 0.78 0.49 0.55 0.55 0.51 0.55 1.18 0.80 0.91 1.23 K2O* 3.02 3.12 2.97 3.12 3.54 2.96 2.83 3.39 3.12 3.31 2.77 2.67 3.39 3.31 2.95 CaO 1.00 0.86 0.92 0.83 0.93 0.91 0.98 0.91 0.95 0.86 0.90 0.82 0.87 0.95 0.84 TiO2* 0.61 0.70 0.61 0.69 0.75 0.65 0.62 0.63 0.61 0.76 0.63 0.61 0.59 0.63 0.59 MnO* 0.07 0.07 0.08 0.06 0.07 0.08 0.08 0.07 0.06 0.06 0.06 0.06 0.05 0.05 0.04 FeO* 5.94 5.64 6.27 6.04 5.89 5.74 5.82 5.59 5.93 5.79 5.84 5.73 6.26 5.69 6.27 Sum 94.12 96.11 92.69 92.74 94.29 93.88 95.05 95.68 96.77 97.36 95.00 97.64 95.45 96.15 95.19 ppm Ag 0.5 nd nd nd nd nd nd nd 0.7 nd nd nd nd nd nd As 7 10 11 9 9 9 8 9 8 9 8 9 9 11 10 Ba 477 463 463 470 474 466 472 470 492 495 541 503 536 497 460 Bi nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd Br nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd Cd nd nd nd nd nd nd nd nd nd nd 1 nd nd nd nd Ce 82 86 88 95 99 97 90 85 94 94 89 94 98 91 91 Cl 254 204 288 249 258 291 251 235 256 243 310 247 276 248 253 Co nd nd nd nd nd nd nd nd nd 40 nd 37 nd 49 42 Cr 84 77 95 93 83 89 84 78 77 71 82 71 63 86 78 Cs 7 10 7 8 10 8 7 8 11 8 9 7 9 10 8 Cu 28 23 25 25 22 23 25 25 26 24 27 22 20 21 21 Ga 22 23 22 22 21 21 23 21 21 21 21 20 20 22 22 Ge 4 3 3 4 3 4 4 3 0 3 4 4 4 4 5 Hg nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd I nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd In nd nd 1 nd nd nd nd nd nd 1 nd nd nd nd nd Mo 4 nd 4 5 6 3 4 3 3 2 3 2 4 4 4 La 39 50 48 55 54 53 48 49 53 50 42 48 53 49 49 Nb 18 20 20 22 22 22 21 20 19 19 20 21 25 21 22 Ni 33 30 37 37 28 30 28 26 29 36 30 28 21 32 28 Pb 21 21 23 22 23 24 20 21 57 22 21 22 23 21 23 Rb 146 148 155 155 154 156 153 150 146 152 142 149 154 164 162 Sb 1 1 2 nd 1 2 nd 1 1 1 2 nd nd 1 2 Se nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd Sn 4 3 3 3 3 4 3 3 4 3 3 3 3 3 5 Sr 127 125 118 113 115 118 114 114 116 121 114 121 128 116 104 Ta nd nd nd nd 9 nd nd nd nd nd nd nd nd nd nd Te nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd Th 13 14 15 14 15 14 14 13 13 13 12 15 16 16 14 Tl nd nd nd nd nd nd nd nd nd nd nd nd nd nd nd U 6 7 6 5 7 6 6 7 7 7 6 7 7 7 7 V 125 109 143 140 125 130 136 119 118 109 118 105 105 121 120 W nd 5 9 nd 8 nd 5 6 7 5 5 5 10 5 6 Y 32 34 34 35 33 35 33 33 33 33 34 34 38 34 35 Zn 121 102 123 108 108 101 100 101 101 109 113 94 117 105 111 Zr 200 187 188 189 205 202 199 208 203 201 224 239 233 207 212

Table 1 (Cont’d). Whole-rock concentration. Asterisk indicates from DCP, and nd indicates not detectable.

The Effect of Provenance on Clay Mineral Diagenesis in Gulf of Mexico Shales

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Samp # 33 34 35 36 37 38 39 40 41 42 43 44 45

Depth ft 11200 11400 11600 11800 12000 12200 12400 12600 12800 13000 13200 13400 13600

Depth m 3415 3476 3537 3598 3659 3720 3780 3841 3902 3963 4024 4085 4146 Wt. % Na2O* 2.36 2.41 2.01 2.39 1.85 1.97 1.95 1.75 1.71 2.03 1.68 2.24 1.90 MgO* 1.90 2.08 2.09 2.35 1.58 2.09 2.22 0.97 2.53 2.18 1.89 2.38 2.39 Al2O3 17.49 17.87 17.57 17.72 18.94 18.97 19.33 18.71 19.62 18.72 19.78 18.58 19.05 SiO2 62.06 62.34 61.22 62.33 63.49 63.66 62.88 63.44 61.25 61.00 64.13 64.25 62.32 P2O5 0.16 0.15 0.17 0.15 0.15 0.15 0.11 0.19 0.15 0.15 0.15 0.16 0.18 SO3 0.72 0.80 0.44 0.86 0.32 0.57 0.51 0.32 0.84 0.78 0.32 0.32 0.38 K2O* 3.61 3.30 3.31 3.12 2.63 3.24 3.30 2.77 3.24 3.30 2.92 3.15 3.05 CaO 0.86 0.90 1.22 0.85 0.89 0.79 0.89 0.97 1.09 0.91 1.00 0.85 0.90 TiO2* 0.60 0.68 0.57 0.85 0.68 0.60 0.72 0.75 0.61 0.61 0.84 0.61 0.61 MnO* 0.05 0.04 0.05 0.09 0.04 0.05 0.04 0.06 0.05 0.03 0.05 0.04 0.04 FeO* 6.47 5.85 6.32 5.94 5.52 5.01 5.74 6.43 6.47 6.50 5.61 5.72 6.40 Sum 96.27 96.42 94.97 96.64 96.10 97.09 97.69 96.36 97.57 96.21 98.38 98.31 97.21 ppm Ag nd nd nd nd nd nd nd nd nd nd nd 0.5 nd As 7 8 10 9 8 8 10 8 8 8 6 10 8 Ba 468 508 477 476 461 458 470 490 464 486 11 610 546 Bi nd nd nd nd nd nd nd nd nd nd nd nd nd Br nd nd nd nd nd nd nd nd nd nd nd nd nd Cd nd nd nd nd nd nd nd nd nd nd nd nd nd Ce 97 84 95 91 94 88 92 92 88 92 83 81 92 Cl 230 213 260 229 243 228 250 231 224 218 263 221 233 Co nd nd nd nd nd nd nd nd nd 40 nd nd nd Cr 80 60 89 75 69 65 69 71 69 80 62 65 86 Cs 9 9 7 8 7 8 8 8 7 10 7 7 9 Cu 22 20 23 23 21 22 20 20 18 21 23 23 23 Ga 21 22 21 21 22 21 22 20 23 23 19 21 24 Ge 5 3 4 4 4 0 3 4 4 4 1 0 5 Hg nd nd nd nd nd nd nd nd nd nd nd nd nd I nd nd nd nd nd nd nd nd nd nd 3 nd nd In nd 1 0 1 nd nd nd nd nd nd nd nd nd Mo 2 4 4 2 2 nd 3 3 4 4 3 2 3 La 51 48 47 49 51 51 48 51 48 53 49 46 52 Nb 23 23 22 22 24 22 23 22 22 22 24 24 25 Ni 29 23 31 28 28 27 29 28 28 27 21 26 29 Pb 22 22 21 21 20 26 21 20 21 21 34 33 21 Rb 167 151 151 154 150 154 161 149 157 170 151 154 171 Sb nd nd 1 nd nd 2 2 nd 2 1 2 2 nd Se 1 nd nd 1 nd nd 1 nd nd nd nd nd 1 Sn 4 3 4 4 4 3 3 3 4 4 3 5 4 Sr 104 111 113 106 108 105 105 108 117 119 124 124 126 Ta nd nd nd nd nd nd nd nd nd nd nd nd nd Te nd nd nd nd nd nd nd nd nd nd nd nd nd Th 16 17 15 14 16 13 14 14 15 15 15 17 16 Tl nd nd nd nd nd nd nd nd nd nd nd nd nd U 7 5 6 6 6 5 6 7 7 7 7 7 8 V 108 101 113 108 100 101 105 96 110 117 95 98 124 W nd 4 nd nd 6 8 8 6 5 nd 7 9 5 Y 36 35 34 35 36 34 35 36 35 34 38 37 35 Zn 100 87 88 176 92 437 80 79 74 80 236 730 86 Zr 218 229 218 231 247 249 231 235 226 209 254 260 215

Table 1 (Cont’d). Whole-rock concentration. Asterisk indicates from DCP, and nd indicates not detectable.

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Samp # Depth Depth Total K+ Total Na+ Total Ca+2

Feet Meters ppm ppm ppm 1 4800 1463 107 1303 21 2 5000 1524 87 1092 6 3 5200 1585 92 1101 17 4 5400 1646 243 1013 39 5 5600 1707 110 1356 12 6 5800 1768 95 1322 13 7 6000 1829 93 1006 12 8 6200 1890 102 1110 23 9 6400 1951 159 1170 21

10 6600 2012 130 1380 38 11 6800 2073 47 1005 13 12 7000 2134 77 1282 13 13 7200 2195 131 1029 25 14 7400 2256 58 984 4 15 7600 2317 78 793 15 16 7800 2378 119 1009 25 18 8200 2500 105 778 14 19 8400 2561 102 816 19 20 8600 2622 193 1081 22 21 8800 2683 106 816 12 22 9000 2744 226 1015 28 23 9200 2805 148 1031 24 24 9400 2866 114 1153 22 25 9600 2927 145 1001 22 26 9800 2988 129 725 20 27 10000 3049 108 652 12 28 10200 3110 118 687 20 29 10400 3171 79 651 15 30 10600 3232 79 816 14 31 10800 3293 235 909 35 32 11000 3354 105 800 19 33 11200 3415 87 699 16 34 11400 3476 65 844 16 35 11600 3537 58 941 16 36 11800 3598 83 736 18 37 12000 3659 41 598 16 38 12200 3720 44 684 20 39 12400 3780 125 847 23 40 12600 3841 96 828 14 41 12800 3902 126 635 20 42 13000 3963 195 872 19 43 13200 4024 106 885 27 44 13400 4085 245 754 20 45 13600 4146 222 745 26

Table 2. Concentration of cations rinsed from the drilling mud.

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Samp Depth Depth Quartz K-feldspar No. feet meters 4.26 A 3.2 A 1 4800 1463 165.2 130.3 3 5200 1585 163.4 112.1 5 5600 1707 170.1 134.4 7 6000 1829 140.7 196.5 9 6400 1951 203 134.6 11 6800 2073 195.7 155.6 13 7200 2195 197.3 140.3 15 7600 2317 212.8 124.2 18 8200 2500 207.3 120 20 8600 2622 216.3 114.6 22 9000 2744 268.6 109.5 24 9400 2866 247.5 100 26 9800 2988 249.6 90.7 28 10200 3110 274.5 110.1 30 10600 3232 290.4 96 32 11000 3354 283.5 96.6 34 11400 3476 359.3 92.4 36 11800 3598 322.9 155.6 38 12200 3720 408.5 110.1 40 12600 3841 419.3 105.2 42 13000 3963 319.2 71.5 44 13400 4085 476.3 88.7 45 13600 4146 353.5 80

Table 3. XRD peak area variation of quartz and feldspar with depth.

and depth (r = 0.41); however, considerable variation is observed (Fig. 5). The coefficient of causation (R2 = 0.17) suggests that only 17% of the variation of K2O is depth related. Clearly other factors, such as provenance variation, are controlling the variation in whole-rock potassium content. Whole-rock oxides have also been nor-malized to TiO2 because of its immobile nature during weathering and diagenesis (Gunter, 1991). K2O / TiO2 ratios do not show any significant correlation with depth. Other oxides such as Al2O3 and SiO2 that are involved in the smectite-illite transformation also show a random variation without a significant correlation with depth.

The variation in major element chemistry may indicate that there was a considerable amount of chemical variation in the source at the time of deposition of the sediment. This may explain the variation with depth in the chemistry of the mudrock. Therefore an attempt was made to assess the variation in provenance of these mud-rocks.

Provenance Some trace-elements ratios provide an index of chemical differentiation (Taylor and McLennan, 1985);

therefore, their ratios in sediments can be used in the estimation of dominant mafic or felsic source. Cr-Th plots

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Samp No. 3 5 11 15 22 26 30 36 42 45 Depth ft. 5200 5600 6800 7600 9000 9800 10600 11800 13000 13600 Depth m. 1585 1707 2073 2317 2744 2988 3232 3598 3963 4146

Alteration Product 4.9 3.8 6.9 5.2 16.0 8.5 4.0 3.3 3.6 4.9 Amphibole 0.1 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.0 0.2 Ankerite 8.4 8.6 4.3 3.4 3.4 3.1 1.6 0.7 5.6 0.4 Apatite 4.2 4.3 0.6 3.7 0.9 6.6 5.0 1.1 4.5 0.1 Barite 0.0 0.0 1.0 0.0 0.0 1.5 0.0 0.0 3.4 2.0 Biotite 0.1 1.1 3.0 3.4 0.2 2.4 11.1 10.9 3.0 4.5 Chlorite 1.6 0.6 2.4 2.3 0.5 0.0 2.7 1.1 0.0 6.9 Composite 2.6 0.8 1.3 12.5 8.3 4.1 5.9 4.2 17.9 9.2 Dolomite 15.4 7.8 0.6 3.6 1.1 2.5 0.3 6.5 0.6 4.1 Iron oxide 0.7 1.8 1.0 0.5 0.4 4.3 6.4 4.5 2.5 0.2 Garnet 10.9 0.1 1.3 3.6 1.3 2.7 3.0 1.5 4.0 2.6 ilmenite 6.1 5.6 0.9 1.8 1.0 6.1 11.9 1.0 0.0 6.1 K/S/A* 1.0 0.0 0.0 0.2 0.3 0.0 0.7 0.9 1.1 0.8 Monazite 0.0 0.0 0.5 1.4 0.7 0.0 0.0 1.7 3.0 0.0 Muscovite 0.0 0.0 0.0 0.7 0.0 0.0 0.0 1.0 3.2 3.5 Pyrite 34.9 55.6 55.6 45.2 39.4 38.2 30.9 45.5 31.1 26.0 Rutile 5.2 7.4 4.2 9.0 18.4 8.8 10.3 2.7 8.9 23.8 Sphene 2.2 0.9 3.6 0.1 1.2 0.0 3.2 0.0 0.0 0.0 Staurolite 0.0 0.0 0.0 0.0 0.7 0.0 0.0 0.0 1.4 0.0 Tourmaline 1.7 1.5 2.4 1.0 0.2 0.0 0.8 7.6 4.3 0.2 Unknown 0.0 0.0 9.6 0.1 0.0 4.5 0.2 0.0 0.0 0.0 Wollastonite 0.0 0.0 0.0 0.0 1.6 1.0 0.3 1.4 0.2 0.0 Zircon 0.0 0.2 0.9 2.3 4.3 5.7 1.7 4.6 1.6 4.4

100.0 100.0 100.0 100.0 100.0 100.0 100.0 100.0 100.0 100.0

Heavy mineral % 0.45 0.60 0.39 0.51 0.43 0.59 0.33 0.42 0.73 0.21

K/S/A = Kyanite/Sillimanite/Andalusite

Table 4. Percentages of mineral species within the heavy mineral fraction.

The Effect of Provenance on Clay Mineral Diagenesis in Gulf of Mexico Shales

709

(Fig. 6) show that these sediments fall within the upper crust area and have a continental signature. The Cr/Th ratios also decrease when plotted with depth, suggesting a depletion of chromium in the sediment with respect to thorium. Similarly, ratios of other compatible (Ni, V) to incompatible (Th, Zr) elements decrease with increased depth (reflected in the negative correlations reported in Table 5). All of these elements are high-field strength elements, and are considered immobile. Their ratios should not change due to diagenesis, therefore their correla-tion with depth suggests a change in source over time. The increase in incompatibles suggests that the deeper sediments were derived from more fractionated rocks, felsic in composition.

To confirm the increase in felsic source material in deeper samples suggested by the trace-element data, the heavy mineral fraction was examined in a manner often used in sandstones. Heavy mineral species were grouped into suites based upon the major rock types in which they commonly occur (Boggs, 1992). Dolomite, ankerite, and siderite were grouped together as carbonates. The metamorphic group contained kyanite-andalusite-sillimanite, staurolite, wollastonite and garnet. Felsic igneous rocks are represented by tourmaline, biotite, mus-covite, zircon, rutile, monazite, sphene and apatite.

The percentage of the metamorphic suite and the felsic igneous heavy-mineral suite versus depth is shown in Figure 7. The felsic igneous heavy minerals show a consistent increase with depth from less than 10% to near 40% of the total heavy-mineral fraction. The metamorphic minerals show a more moderate increase with depth. The increase in felsic igneous heavy minerals with depth is consistent with the increase in felsic source suggested by the trace element data.

This mixed provenance is not unlike the source areas that provide sediment to the modern Gulf of Mexico. Varying mixtures of sediment from a dominantly metamorphic Appalachian source and a felsic, western North American source are controlled by a dynamic drainage system. Changes in river and deltaic positions, variations

in climate in the source areas, and changes in tectonic activity, can exert major controls on the mixture of these two areas at specific times. In the deeper part of the studied well, the felsic igneous source appears dominant, and this source has gradually diminished over time, relative to a metamorphic source.

Felsic igneous rocks are typically enriched in potassium. The observed increase in potassium with depth could be a result of an increase in a felsic igneous provenance, as suggested by Bloch et al. (1998).

PROVENANCE OR DIAGENESIS? Our previous work (Totten et al., 2002) reported the transformation of smectite to illite with increased depth.

This study confirms the increased K2O with depth, in the Ship Shoal area of the Gulf of Mexico. This is consis-tent with trends seen in other GOM mudrocks. Where did the potassium come from? If the potassium that is required for illite formation is imported into the mudrock from an external source, there should be a gradual in-crease in the total K2O content as the reaction progresses. In this study, the coefficient of causation (R2) suggests that only 17 % of the increase is depth related. A similar increase should be observed for Al2O3 if it is supplied from an external source, which is not observed in this study. Correspondingly, any silica released during the reaction that leaves the mudrock would cause the total SiO2 to decrease. This is also not observed in these rocks. In contrast, the growth of quartz with depth suggests that the released silica remains within the mudrock.

The increase in K2O could be due to an increase in a felsic source area. The increase in this source relative to a metamorphic province would not necessarily change the SiO2 or Al2O3 concentrations over a metamorphic terrain. In this scenario, the required elements for clay mineral transformations are within the rock itself, and do not need to be imported from outside the mudrock system.

CONCLUSIONS The mudrocks in this area of offshore Louisiana showed similar mineralogical changes as seen in Texas Gulf

Coast mudrocks. The smectite to illite transformation took place over a depth interval from 4800 to 13,600 ft (1463 to 4146 m) and is accompanied by the loss of K-feldspar and an increase in the amount of quartz.

Whole-rock Al2O3 and SiO2 did not show any depth-related trends. The amount of K2O varied between 2.5 and 3.6 wt % and showed a slight increasing trend with depth. However, only 17 % of the increase is depth re-lated. When K2O is normalized to TiO2 the correlation disappears.

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Figure 3. Concentrations of K+, Na+, and Ca2+ rinsed from the drilling mud coating on each sample with depth.

Provenance studies indicate that there was a mixed metamorphic and igneous sediment source for these rocks. The felsic igneous source increased over deeper parts of the well. Ratios of compatible to incompatible trace elements also indicate that the sediments had a more felsic signature at deeper depths. This suggests that felsic source rocks were the major contributors towards the sediment during the earlier depositional period. These felsic rocks are responsible for the increased potassium at deeper depths.

The most probable source of potassium for illite formation is K-feldspar, which was originally more abun-dant in the deeper, felsic-rich rocks. The silica released during illite formation stays in the mudrock in the form of microcrystalline quartz. The lack of strong depth-related trends of the major elements involved in the forma-tion of illite from smectite during burial diagenesis does not support open system behavior. The random variation in chemistry makes it difficult to assume an initial constant chemistry and is probably due to variations in prove-nance over time.

It is interesting to note that the whole-rock K2O content reported from the Texas Gulf Coast shows a greater increase with depth as compared with these samples (Berger et al., 1999; Land et al., 1997; Lynch, 1997; Mil-liken et al., 1994; Awwiller, 1993; Hower et al., 1976). This may indicate that the Texas Gulf Coast mudrocks may have had an even greater variation in provenance. Their proximity to the felsic, western North American source area could explain the higher potassium concentration relative to offshore Louisiana.

ACKNOWLEDGMENTS The authors would like to thank Al Falster of the University of New Orleans for all of his assistance in SEM,

XRD, and DCP analyses. We also sincerely thank Pierre Burnside of Tulane University for the XRF analyses.

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Figure 4. Variation in quartz and K-feldspar percentage (estimated from XRD peak area) with depth.

REFERENCES CITED

Anderson, D. N., 1976, Ancient delta systems in the Gulf Coast area: Gulf Coast Association of Geological Societies Transactions, v. 26, p. 4-9.

Awwiller, D. N., 1993, Illite/Smectite formation and potassium mass transfer during burial diagenesis of mud-rocks: A

study from the Texas Gulf Coast Paleocene-Eocene: Journal of Sedimentary Petrology, v. 63, p. 501-512. Basu, A., and E. Molinaroli, 1989, Provenance characteristics of detrital opaque Fe-Ti oxide minerals: Journal of Sedi-

mentary Petrology, v. 59, p. 922-934. Berger, G., B. Velde, and T. Aigouy, 1999, Potassium sources and illitization in Texas Gulf Coast mudrock diagenesis:

Journal of Sedimentary Research, v. 69, p. 151-157. Bloch, J., I. E. Hutcheon, and P. de Cartat, 1998, Tertiary volcanic rocks and the potassium content of Gulf Coast

shales—The smoking gun: Geology, v. 26, p. 527-530. Boggs, S., 1992, Petrology of sedimentary rocks: Macmillan Publishing Company, New York, 707 p. Boles, J. R., and S. G. Franks, 1979, Clay diagenesis in Wilcox and sandstones of southwest Texas: Implications of

smectite diagenesis on sandstone cementation: Journal of Sedimentary Petrology, v. 49, p. 55-70. Cuadros, J., and P. S. Altaner, 1998, Characterization of mixed-layer illite-smectite from bentonites using microscopic

chemical, and x-ray methods: Constraints on the smectite-to-illite transformation mechanism: American Miner-alogist, v. 83, p. 762-774.

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Figure 5. Variation in potassium with depth. Slight correlation with depth (r = 0.41). Only 17% of potassium increase is due to increasing depth (R2 = 0.17).

Gier, S., 1998, Burial diagenetic processes and clay mineral formation in the mollasse zone of Upper Austria: Clays and Clay Minerals, v. 46, p. 658-669.

Grigsby, J. D., 1990, Detrital magnetite as a provenance indicator: Journal of Sedimentary Petrology, v. 60, p. 940-960. Gunter, F., 1991, Principles and applications of inorganic geochemistry: Macmillan Publishing Company, New York,

626 p. Hanan, M. A., and M. W. Totten, 1996, Analytical techniques for the separation and SEM identification of heavy min-

erals in mud-rocks: Journal of Sedimentary Research, v. 66, p. 1027-1030. Hiscott, R. N., 1984, Ophiolitic source for Taconic-age flysch: trace element evidence: Geological Society of America

Bulletin, v. 95, p. 1261-1267. Hower, J., E. V. Eslinger, M. E. Hower, and E. A. Perry, 1976, Mechanism of burial metamorphism of argillaceous

sediment: 1. Mineralogical and chemical evidence: Geological Society of America Bulletin, v. 87, p. 725-737.

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K2O (Wt %)

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Figure 6. Chromium versus thorium of whole-rock shales. Samples plot between upper crust (UC) and the North American Shale Composite (NASC). Samples do not cluster tightly, suggesting a random variation in source material.

Land, L. S., L. E. Mack, K. L. Milliken, and F. L. Lynch, 1997, Burial diagenesis of argillaceous sediment, South Texas Gulf of Mexico sedimentary basin: A reexamination: Geological Society of America Bulletin, v. 109, p. 2-15.

Lynch, L. F., 1997, Frio shale mineralogy and the stoichiometry of the smectite to illite reaction: The most important

reaction in clastic sedimentary diagenesis: Clays and Clay Minerals, v. 45, p. 618-631. Lynch, L. F., K. L. Milliken, D.N. Awwiller, and L. E. Mack, 1999, Tertiary volcanic rocks and the potassium content

of Gulf coast shales—The smoking gun: Comment and reply: Geology, v. 27, p. 663-665. Milliken, K. L., L. E. Mack, and L. S. Land, 1994, Element mobility in sandstones during burial; whole-rock chemical

and isotopic data, Frio Formation, South Texas: Journal of Sedimentary Research, v. 64, p. 788-796. Polastro, R. M., 1985, Mineralogical and morphological evidence for the formation of illite at the expense of illite/

smectite: Clays and Clay Minerals, v. 33, p. 265-275. Schneiderman, J. S., 1995, Detrital opaque oxides as provenance indicators in River Nile sediments: Journal of Sedi-

mentary Research, v. 65, p. 668-674. Taylor, S. R., and S. M. McClennan, 1985, The continental crust: Its composition and evolution: Blackwell Scientific

Publications, Oxford, U.K., 312 p. Totten, M. W., M. Dixon, and M. A. Hanan, 2005, Diagenesis of mixed-layer clay minerals in the South Timbalier area,

Gulf of Mexico: Gulf Coast Association of Geological Societies Transactions, v. 55, p. 821-829. Totten, M. W., M. A. Hanan, D. Mack, and J. Borges, 2002, Characteristics of mixed-layer smectite/illite density sepa-

rates during burial diagenesis: American Mineralogist, v. 87, p. 1571-1579.

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Totten, M. W., M. A. Hanan, and B. Weaver, 2000, Beyond whole-rock geochemistry of shales: The importance of

assessing mineralogic controls for revealing tectonic discriminants of multiple sediment sources for the Ouachita Mountain flysch deposits: Geological Society of America Bulletin, v. 112, p. 1012-1022.

Totten, M. W., and H. Blatt, 1993, Alteration in the non-clay-mineral fraction of pelitic rocks across the diagenetic to

low-grade metamorphic transition, Ouachita Mountains, Oklahoma and Arkansas: Journal of Sedimentary Petrol-ogy, v. 63, p. 899-908.

Totten, M. W., and H. Blatt, 1996, Sources of silica from the illite to muscovite transformation during late-stage

diagenesis of shales: Siliciclastic diagenesis and fluid flow: Concepts and Applications: Society of Economic Paleontologists and Mineralogists Special Publication No. 55, p. 85-92.

Figure 7. Percentage of heavy-mineral groups versus depth. Minerals associated with felsic source areas increase with depth.

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Ratios r Cr/Th -0.46

Ni/Th -0.38 V/Th -0.47 Cr/Zr -0.47 Ni/Zr -0.45 V/Zr -0.49 Cr/La -0.25 Ni/La -0.20 V/La -0.27

Sr/Rb -0.78

Table 5. Correlation coefficients of compatible versus incompatible element ratios with depth.

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