Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
4691180 | Sedimentary Geology | 2006 | 27 Pages |
Abstract
The Peñas Rubias Syncline (southwestern Spain) exposes a well-preserved shallow-water platform succession containing a spectrum of facies corresponding to inner platform intertidal to supratidal environments, across to deeper-water middle to outer platform environments. Nineteen microfacies are recognized, which are grouped into seven facies association corresponding to: siliciclastic deltaic bars, mixed carbonate/siliciclastic shoals, carbonate mud mound boundstones, background platform carbonates, background platform siliciclastics, mixed tempestites and deep-water siliciclastic shales and sandstones. The age of the succession was determined mainly by foraminiferans and calcareous algae, which permit the succession to be assigned to the late Brigantian (latest Viséan). This upper Brigantian platform is the only record of sedimentation of this age in the region, and thus is key for interpreting the sedimentary and tectonic evolution of the Carboniferous rocks in Sierra Morena. Biotic and sedimentological features were analyzed in order to assess the controls on the sedimentation. Several factors have influenced sedimentological changes: turbidity, subsidence, siliciclastic discharges, storms and bioturbation. The siliciclastic discharges exerted a considerable control on the basal deposits, mostly in their percentage of quartz sand grains and as microconglomerates. However, they did not develop as large deltaic deposits, and their influence can be considered as virtually negligible in regards to the remaining part of the succession. Turbidity, as a result of higher percentage of silt and mud in suspension, seems to be the main factor controlling the change between the older intertidal deposits in the inner platform to the younger subtidal deposits of the middle and outer platform. As a result of the increase of the mud and silt in suspension, facies changed first to marlstones and nodular argillaceous limestones, and second, to predominantly calcimicrobial boundstones and shales in the uppermost part of the carbonate succession, as well as showing a marked change from photic-controlled benthic faunal and microfloral assemblages to assemblages more tolerant or better adapted to muddier dysphotic substrates. Bioturbation is also interpreted as one of the main controls influencing the different type of boundstones in the middle platform, permitting the vertical growth of dome-shaped mud-mounds or as sheet-like deposits. Storm influences seem to have exerted some control on the positive relief of the dome-shaped boundstones, which are usually capped by tempestites. The differential subsidence observed in the northwestern sector of the platform allowed the accumulation of many stacked dome-shaped mounds, a feature not recognized in southeastern parts. The general stratigraphical sequence seems to be controlled by eustasy and synsedimentary tectonics. The overall succession exhibits a pronounced deepening-upwards transgressive sequence from siliciclastic delta bars, mixed shoals, carbonates and shales of the middle platform with the growth of calcimicrobial boundstones and dark green shales, passing up into black shales at the top of the sequence, in the outer platform and, possibly, submarine slope settings. Although this transgressive sequence is in harmony with the 3rd-order glacioeustatic cycle defined for the late Brigantian in the western Palaeotethys, all these Brigantian rocks accumulated in a synsedimentary extensional regime, which is related to the initiation of a sinistral strike-slip regime, previously recognized as affecting only Serpukhovian and younger rocks in Sierra Morena. These synsedimentary faults allow us to recognize significant lateral variations in thickness over short distances.
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Physical Sciences and Engineering
Earth and Planetary Sciences
Earth-Surface Processes
Authors
P. Cózar, I.D. Somerville, S. RodrÃguez, R. Mas, P. Medina-Varea,