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Copyright by Nysha Chaderton 2009 - The University of Texas at ...

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Chapter Four: <strong>The</strong> Evolution <strong>of</strong> the Tobago Forearc Basin<br />

<strong>The</strong> objective <strong>of</strong> this chapter is to define the timing and structural history <strong>of</strong> the<br />

Tobago Basin and its rel<strong>at</strong>ionship to the larger accretionary prism processes, as well as to<br />

interpret the origin <strong>of</strong> two major str<strong>at</strong>igraphic units—the Scotland Form<strong>at</strong>ion (lower to<br />

middle Eocene (possibly Oligocene) and the Oceanic Form<strong>at</strong>ion (middle Eocene to<br />

middle Miocene)—which fill the basin. <strong>The</strong> Scotland and the Oceanic Form<strong>at</strong>ions<br />

comprise known hydrocarbon reservoir and seal units, respectively, in the basin.<br />

Understanding their individual depositional and post-depositional histories will in turn<br />

enable a better understanding <strong>of</strong> younger Tertiary units <strong>of</strong> similar setting in this basin.<br />

<strong>The</strong> Oceanic Form<strong>at</strong>ion<br />

<strong>The</strong> Oceanic Form<strong>at</strong>ion was first recognized in the l<strong>at</strong>e 1800’s <strong>by</strong> Jukes-Brown<br />

and Harrison (1890), who produced a detailed map <strong>of</strong> the geology <strong>of</strong> Barbados and<br />

identified the Coral Rock, the Oceanic Series, the Scotland Series, and the Joes River<br />

Form<strong>at</strong>ion. <strong>The</strong>y interpreted the Oceanic Series as a<strong>by</strong>ssal sediments th<strong>at</strong> had been raised<br />

to their current position <strong>by</strong> tectonic uplift.<br />

Until the l<strong>at</strong>e 1970’s, because most geological research on Barbados centered on<br />

hydrocarbon explor<strong>at</strong>ion, the clastic succession <strong>of</strong> the Scotland Form<strong>at</strong>ion had been<br />

extensively studied and the Oceanic Form<strong>at</strong>ion was largely ignored. This situ<strong>at</strong>ion<br />

changed when Robert Speed began in the early 1980’s to investig<strong>at</strong>e the structure and<br />

sediment<strong>at</strong>ion <strong>of</strong> the Barbados Accretionary Prism. Speed described the Oceanic<br />

Form<strong>at</strong>ion as consisting <strong>of</strong> calcareous clays and muds and marls with volcanic ash layers<br />

(Speed and Torrini, 1989, Speed 1991, 1994). Likewise, micro-paleontologic analysis <strong>of</strong><br />

the Oceanic units <strong>by</strong> Saunders et al. (1984) led to the conclusion th<strong>at</strong> these sediments had<br />

been deposited in 2,000 to 4,000 m <strong>of</strong> w<strong>at</strong>er.<br />

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