Initial Reports of the Deep Sea Drilling Project 1984
DOI: 10.2973/dsdp.proc.75.130.1984
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Organic Geochemistry of Cretaceous Black Shales from Deep Sea Drilling Project Site 530, Leg 75, Eastern South Atlantic

Abstract: Five-hundred ten meters of Cretaceous sediments were drilled north of the Walvis escarpment in Hole 53OA during Leg 75. An immature stage of evolution for organic matter can be assigned to all the samples studied. Black shales are interbedded with red and green claystone in the bottom sedimentary unit, Unit 8, which is of Coniacian to late Albian age. The richest organic carbon contents and petroleum potentials occur in the black shales. Detrital organic matter is present throughout the various members of a se… Show more

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Cited by 11 publications
(8 citation statements)
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References 6 publications
(5 reference statements)
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“…Although our results are specific to Site 364 and the margins of northern South Atlantic, periodic black shales of similar age (Early Cretaceous) have been reported elsewhere in the proto‐Atlantic, for example, at Site 530 in the Angola basin (e.g., Deroo et al, ; Katz, ; Meyers et al, ; Rullkötter et al, ; Stow & Dean, ); Site 511 in the Falkland Plateau (e.g., Deroo et al, ), and Site 367 in Gambia Abyssal Plain (e.g., Hofmann et al, ; Wagner et al, ). There are also numerous publications on the astronomically controlled formation of black shales in the Late Cretaceous, for example, from Site 959 in the Ivorian Basin (Beckmann et al, ; Holbourn et al, ), Leg 207 (Sites 1257–1261) at Demerara Rise (Hofmann & Wagner, ; Meyers et al, ), Site 530 in the Angola basin (e.g., Arthur et al, ; Deroo et al, ; A. Forster et al, ; Stow & Dean, ), the Western Interior Seaway (Eldrett et al, ), and ODP Site 1138 in the Indian Ocean (Dickson et al, ). These results suggest that the proposed depositional mechanism for Site 364 of a hydrographically restricted basin that was preconditioned to astronomically controlled variations in terrestrial runoff was probably a common feature of the proto‐Atlantic region during the Cretaceous.…”
Section: Discussionsupporting
confidence: 75%
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“…Although our results are specific to Site 364 and the margins of northern South Atlantic, periodic black shales of similar age (Early Cretaceous) have been reported elsewhere in the proto‐Atlantic, for example, at Site 530 in the Angola basin (e.g., Deroo et al, ; Katz, ; Meyers et al, ; Rullkötter et al, ; Stow & Dean, ); Site 511 in the Falkland Plateau (e.g., Deroo et al, ), and Site 367 in Gambia Abyssal Plain (e.g., Hofmann et al, ; Wagner et al, ). There are also numerous publications on the astronomically controlled formation of black shales in the Late Cretaceous, for example, from Site 959 in the Ivorian Basin (Beckmann et al, ; Holbourn et al, ), Leg 207 (Sites 1257–1261) at Demerara Rise (Hofmann & Wagner, ; Meyers et al, ), Site 530 in the Angola basin (e.g., Arthur et al, ; Deroo et al, ; A. Forster et al, ; Stow & Dean, ), the Western Interior Seaway (Eldrett et al, ), and ODP Site 1138 in the Indian Ocean (Dickson et al, ). These results suggest that the proposed depositional mechanism for Site 364 of a hydrographically restricted basin that was preconditioned to astronomically controlled variations in terrestrial runoff was probably a common feature of the proto‐Atlantic region during the Cretaceous.…”
Section: Discussionsupporting
confidence: 75%
“…This observation suggests that rhythmically paced changes in the depositional environment occurred in the basin during the Early Cretaceous. This cyclicity bears a strong resemblance to the astronomically paced formation of organic‐rich sapropels at Deep Ivorian Basin (ODP Site 959) during the Coniacian (Beckmann et al, ); at Demerara Rise (Leg 207) during the Cenomanian–Turonian (Flögel et al, ; Hofmann & Wagner, ; Meyers et al, ); at Site 530 during the Cenomanian–Turonian (Arthur et al, ; Deroo et al, ; A. Forster et al, ; Stow & Dean, ); and at Site 1138 during the Cenomanian–Turonian (Dickson et al, ).…”
Section: Discussionmentioning
confidence: 91%
“…Generally, all of the samples from Site 742 have low hydrogen and oxygen indices with no preference for maturity near the origin. Samples with low T max and hydrogen and oxygen indices were probably an admixture of several kerogens deposited in an oxygenated environment (Deroo et al, 1984).…”
Section: Rock-eval Pyrolysismentioning
confidence: 99%
“…One means of generating carbon with low HI, OI, and T max would be deposition in an oxygenated environment, along with the admixture of reworked carbon of high maturity. The reworked carbon would depress both HI and OI without significantly affecting the T max of the fresh, immature carbon (Deroo et al, 1984).…”
Section: Rock-eval Pyrolysismentioning
confidence: 99%
“…Values of Samples 119-741A-1R-1, 109-110 cm, and 119-741A-4R-2, 140-150 cm, which have only 0.15% and 0.17% TOC, respectively, are plotted within the type I/type II regime of the modified van Krevelen plot. Deroo et al (1984) estimated that Rock-Eval instrument function becomes erratic near these levels, so these points are possibly spurious.…”
Section: Rock-eval Pyrolysismentioning
confidence: 99%