1994
DOI: 10.1016/0146-6380(94)90118-x
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Geochemical characterization of lithofacies and organic facies in Cretaceous organic-rich rocks from Trinidad, East Venezuela Basin

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Cited by 30 publications
(21 citation statements)
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“…Ranges of average TOC and HI of the organic-rich samples in the Naparima Hill and Gautier Formations obtained from eight wells in the basin are 1.9 -7.9 wt% TOC and 191 -596 mg HC/g TOC, and 1.6-4.2 wt% TOC and 114-538 mg HC/g TOC, respectively. Requejo et al (1994) also showed that the source rocks belong to carbonate, siliceous, and siliciclastic lithofacies, with the latter two tending to be localized in south-central Trinidad.…”
Section: Source Characteristics and Oil-to-source Correlationmentioning
confidence: 93%
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“…Ranges of average TOC and HI of the organic-rich samples in the Naparima Hill and Gautier Formations obtained from eight wells in the basin are 1.9 -7.9 wt% TOC and 191 -596 mg HC/g TOC, and 1.6-4.2 wt% TOC and 114-538 mg HC/g TOC, respectively. Requejo et al (1994) also showed that the source rocks belong to carbonate, siliceous, and siliciclastic lithofacies, with the latter two tending to be localized in south-central Trinidad.…”
Section: Source Characteristics and Oil-to-source Correlationmentioning
confidence: 93%
“…All of these units show indications of deposition in deep neritic (outer shelf to upper slope) to bathyal environments (Koutsoukos & Merrick, 1986). The organic-rich Gautier and Naparima Hill formations, which constitute a stratigraphic thickness in excess of 3000 ft (915 m) in southern Trinidad (Ablewhite & Higgins, 1968), are considered the source rocks for the majority of petroleum in Trinidad (Requejo, Wielchowsky, Klosterman, & Sassen, 1994;Rodrigues, 1987). These units are broadly agecorrelative to the La Luna, Querequal and other upper Cretaceous source rock sequences in Venezuela and adjacent areas (Talukdar, Gallango, & Ruggiero, 1987;Zumberge, 1984).…”
Section: Stratigraphymentioning
confidence: 96%
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“…They both demonstrate dominant pregnanes, which is probably related to their high maturity (Eglinton et al, 1988;Requejo et al, 1994;Wingert and Pomerantz, 1986), along with C 27 > C 28 <C 29 normalized relative abundance of regular steranes. However, a distinct difference is also observed.…”
Section: Steroidsmentioning
confidence: 95%