Insights into Caribbean tectonics from a detrital zircon U-Pb provenance study of siliciclastic strata in western and central Cuba

Patricia Ascanio-Pellon, D. Stockli, Daniel Ruiz-Arriaga, L. Stockli
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Abstract

The tectonic affinity and origins of the Jurassic, siliciclastic San Cayetano and Constancia formations exposed in western and central Cuba in the Caribbean region remain debated. The scarcity of modern geochronologic studies on these Cuban units hampers both sedimentary provenance and palinspastic reconstructions, resulting in Caribbean models that tend to oversimplify the formation of Cuba and correlate the Jurassic strata to various regions such as North America, South America, the Yucatán margin, or the conceptual Caribeana domain. Using laser ablation−inductively coupled plasma−mass spectrometry (LA-ICP-MS), we conducted a detailed detrital zircon (DZ) U-Pb provenance study of these Cuban siliciclastic strata that provides critical insights into understanding the formation of Cuba during the Early Jurassic rifting stages of Pangea. Results from 19 San Cayetano Formation samples show a dominant Oaxaquia (ca. 1 Ga) and Chiapas batholith (ca. 250 Ma) signature, while six Constancia samples display variable ca. 1 Ga and ca. 250 Ma grains. The Lower Cretaceous Polier Formation and the Paleocene Moncada Formation also display the same ca. 1 Ga and ca. 250 Ma signatures. After comparing these Cuban data with data from other regional DZ studies, we propose that that the San Cayetano and Constancia formations are correlative to the Todos Santos Formation located in the southwestern Yucatán region of Mexico. These Cuban units were predominantly deposited adjacent to the Chiapas batholith during the Early Jurassic in northwest−southeast-trending basins created by Pangean rifting. They were eventually sheared during eastward migration of the Caribbean plate and transported northward until they collided with the North American continent in the Paleogene. This DZ study provides new constraints on the tectonic provenance of western and central Cuba and improves plate tectonic reconstructions of the Caribbean.
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从对古巴西部和中部硅质碎屑岩地层的非铁质锆石 U-Pb 出处研究中洞察加勒比构造运动
加勒比地区古巴西部和中部出露的侏罗纪硅质碎屑岩圣卡耶塔诺地层和康斯坦西亚地层的构造亲缘关系和起源仍存在争议。对古巴这些地层单元的现代地质年代研究稀少,妨碍了沉积产地和古地层重构,导致加勒比模型倾向于过度简化古巴地层的形成,并将侏罗纪地层与北美、南美、尤卡坦边缘或加勒比概念域等不同地区相关联。利用激光烧蚀-电感耦合等离子体质谱法(LA-ICP-MS),我们对这些古巴硅质碎屑岩地层进行了详细的碎屑锆石(DZ)U-Pb 出处研究,为了解古巴在泛大陆早侏罗世断裂阶段的形成提供了重要的见解。来自 19 个 San Cayetano Formation 样品的研究结果显示了主要的 Oaxaquia(约 1 Ga)和 Chiapas 浴岩(约 250 Ma)特征,而 6 个 Constancia 样品则显示了可变的约 1 Ga 和约 250 Ma 岩粒。1 Ga 和约 250 Ma 的颗粒。下白垩统波利埃地层和古新统蒙卡达地层也显示出相同的约 1 Ga 和约 250 Ma 的特征。1 Ga 和大约 250 Ma 的特征。在将古巴的这些数据与其他地区的 DZ 研究数据进行比较之后,我们认为 San Cayetano 和 Constancia 地层与位于墨西哥尤卡坦西南部地区的 Todos Santos 地层相关。侏罗纪早期,这些古巴单元主要沉积在恰帕斯熔岩附近的西北-东南走向盆地中,这些盆地是由潘加山脉断裂形成的。它们最终在加勒比板块东移过程中被剪切并向北迁移,直至在古近纪与北美大陆相撞。这项 DZ 研究为古巴西部和中部的构造成因提供了新的制约因素,并改进了加勒比地区的板块构造重建。
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