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| [[File:Trinidad (Kuba) 03.jpg|thumb|Trinidad (Kuba) 03: released in the GFDL by [http://commons.wikimedia.org/wiki/User:Dino1948 Dieter Mueller].]] | | [[File:Trinidad (Kuba) 03.jpg|thumb|Trinidad (Kuba) 03: released in the GFDL by [http://commons.wikimedia.org/wiki/User:Dino1948 Dieter Mueller].]] |
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− | The geology of Cuba has been a challenge to geologists because of features such as the presence of well-preserved [[Jurassic]] [[ammonite]]s, the rich [[Tertiary]] [[foraminiferal]] faunas (including remarkable [[Paleogene]] [[orbitoids]]), the gigantic Upper [[Cretaceous]] [[rudistids]], the spectacular limestone Mogotes of Pinar del Rio, the extensive outcrops of [https://wwwf.imperial.ac.uk/earthscienceandengineering/rocklibrary/viewglossrecord.php?gID=00000000012 ultrabasic] [[igneous]] rocks, the [[chromite]] and [[manganese]] deposits, and the extraordinary structural complexity. In addition to these features, the numerous petroleum seeps, many of them coming out of [[Wikipedia:Basic_rock|basic]] igneous rock, have attracted much attention. | + | The geology of Cuba has been a challenge to geologists because of features such as the presence of well-preserved [[Jurassic]] [[ammonite]]s, the rich [[Tertiary]] [[foraminiferal]] faunas (including remarkable [[Paleogene]] [[orbitoids]]), the gigantic Upper [[Cretaceous]] [[rudistids]], the spectacular limestone Mogotes of Pinar del Rio, the extensive outcrops of [https://wwwf.imperial.ac.uk/earthscienceandengineering/rocklibrary/viewglossrecord.php?gID=00000000012 ultrabasic] [[Igneous rock|igneous]] rocks, the [[chromite]] and [[manganese]] deposits, and the extraordinary structural complexity. In addition to these features, the numerous petroleum seeps, many of them coming out of [[Wikipedia:Basic_rock|basic]] igneous rock, have attracted much attention. |
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| ==Regional setting== | | ==Regional setting== |
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| ===Barremian=== | | ===Barremian=== |
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− | During the [[Barremian]], deposition of [[platform]] carbonates continued in the north, grading from shallow-water algal types, with fewer [[evaporite]]s, to [[breccia]]s. South, west, and possibly east of the Bahamas Platform, deep-water sedimentation of [http://www.merriam-webster.com/dictionary/pelagic pelagic] (nannoplankton) carbonates continued. However, because of the late Neocomian tectonic activity, [[conglomerate]]s, derived from the previously deposited limestones in the Las Villas* belt and from the exposed granitic basement in the [[Cifuentes]]* belt to the south, became common. No Barremian sediments were deposited in some of the southern areas. However, the [http://geology.com/rocks/basalt.shtml basaltic] to intermediate flows possibly continued to accumulate over the southern part of the [[Wikipedia:Basic_rock|basic]] igneous basement. | + | During the [[Barremian]], deposition of [[platform]] carbonates continued in the north, grading from shallow-water algal types, with fewer [[evaporite]]s, to [[breccia]]s. South, west, and possibly east of the Bahamas Platform, deep-water sedimentation of [http://www.merriam-webster.com/dictionary/pelagic pelagic] (nannoplankton) carbonates continued. However, because of the late Neocomian tectonic activity, [[conglomerate]]s, derived from the previously deposited limestones in the Las Villas* belt and from the exposed granitic basement in the [[Cifuentes]]* belt to the south, became common. No Barremian sediments were deposited in some of the southern areas. However, the [http://geology.com/rocks/basalt.shtml basaltic] to intermediate flows possibly continued to accumulate over the southern part of the [[Wikipedia:Basic_rock|basic]] [[Igneous rock|igneous]] [[basement]]. |
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| ===Aptian=== | | ===Aptian=== |
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| A large trough-shaped basin formed in front of the thrust sheets, deeper near the thrust front and shallower northward. Early to middle Eocene [[flysch]] deposition in the trough began with sediments derived from limestones, such as the Sagua* and San Martin* formations, followed by an increase in volcanic and [http://www.geolsoc.org.uk/ks3/gsl/education/resources/rockcycle/page3598.html intrusive]-derived detritus, such as the lower Vega* and lower Manacas (Pica Pica) formations, and finally, capped by the intrusive and volcanic-derived coarse [[conglomerate]]s and [http://www.encyclopedia.com/doc/1O13-wildflysch.html wildflysch] of the upper Vega* (Rosas*) and upper Manacas (Vieja) Formations. In central Cuba, the rocks of the deep-water Vega* Formation became coarser grained through time. In western Cuba, the fine-grained clastics and other [http://www.merriam-webster.com/dictionary/pelagic pelagic] sediments of the Manacas Formation changed abruptly to the coarse [[breccia]]s of the Vieja Member. The breccia clasts reflect the lithology of the associated fault blocks. This suggests some subaerial [[erosion]] in central Cuba, whereas western Cuba was largely submarine. | | A large trough-shaped basin formed in front of the thrust sheets, deeper near the thrust front and shallower northward. Early to middle Eocene [[flysch]] deposition in the trough began with sediments derived from limestones, such as the Sagua* and San Martin* formations, followed by an increase in volcanic and [http://www.geolsoc.org.uk/ks3/gsl/education/resources/rockcycle/page3598.html intrusive]-derived detritus, such as the lower Vega* and lower Manacas (Pica Pica) formations, and finally, capped by the intrusive and volcanic-derived coarse [[conglomerate]]s and [http://www.encyclopedia.com/doc/1O13-wildflysch.html wildflysch] of the upper Vega* (Rosas*) and upper Manacas (Vieja) Formations. In central Cuba, the rocks of the deep-water Vega* Formation became coarser grained through time. In western Cuba, the fine-grained clastics and other [http://www.merriam-webster.com/dictionary/pelagic pelagic] sediments of the Manacas Formation changed abruptly to the coarse [[breccia]]s of the Vieja Member. The breccia clasts reflect the lithology of the associated fault blocks. This suggests some subaerial [[erosion]] in central Cuba, whereas western Cuba was largely submarine. |
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− | South of the front of the advancing volcanic and basic intrusive-rock thrust plate, a second series of basins developed parallel to the northern trough. Within these basins, which were carried piggyback by the thrust plate, lower Eocene igneous-derived sediments accumulated, but under quieter tectonic conditions (the Taguasco*, Bijabo*, Santa Clara*, Alkazar, Bacunayagua, Capdevila, and Universidad Formations, for example). | + | South of the front of the advancing volcanic and basic intrusive-rock thrust plate, a second series of basins developed parallel to the northern trough. Within these basins, which were carried piggyback by the thrust plate, lower Eocene [[Igneous rock|igneous]]-derived sediments accumulated, but under quieter tectonic conditions (the Taguasco*, Bijabo*, Santa Clara*, Alkazar, Bacunayagua, Capdevila, and Universidad Formations, for example). |
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| As the thrust sheets advanced, they overrode the lower to middle Eocene flysch, which had accumulated in front of them, and the flysch served as a lubricating medium for further thrusting. The [[subduction]] responsible for the uplift driving the thrusting ceased progressively from west to east, and volcanic activity continued in Oriente until the middle Eocene. Along what appears to be a north-[[dip]]ping subduction zone and south of the Jardines de la Reina Cays (Camaguey trench) is a filled trench, which is a remnant of an accretionary prism. This trench could be related to the exposures in Haiti's southern peninsula and the Muertos Trench. | | As the thrust sheets advanced, they overrode the lower to middle Eocene flysch, which had accumulated in front of them, and the flysch served as a lubricating medium for further thrusting. The [[subduction]] responsible for the uplift driving the thrusting ceased progressively from west to east, and volcanic activity continued in Oriente until the middle Eocene. Along what appears to be a north-[[dip]]ping subduction zone and south of the Jardines de la Reina Cays (Camaguey trench) is a filled trench, which is a remnant of an accretionary prism. This trench could be related to the exposures in Haiti's southern peninsula and the Muertos Trench. |