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Lacustrine chalky carbonates: origin, physical properties and diagenesis (Palaeogene of the Madrid Basin, Spain)

dc.contributor.authorArribas Mocoroa, María Eugenia
dc.contributor.authorBustillo Revuelta, María Ángeles
dc.contributor.authorTsige Beyene, Meaza
dc.date.accessioned2023-06-20T09:42:18Z
dc.date.available2023-06-20T09:42:18Z
dc.date.issued2006
dc.description.abstractThe Palaeogene lacustrine chalky carbonates of the Madrid Basin are a peculiar type of very soft and friable carbonate facies with high porosity despite being covered by more than 800 m of sediment. Similar physical properties to those described in marine chalk reservoirs emphasize the interest in analysing and characterizing these carbonate facies within a lacustrine depositional system. Lithologically, they are calcitic and/or dolomitic poorly cemented carbonate muds with no significant amounts of skeletal debris. Clay minerals such as illite, smectite and palygorskite are present between the carbonate crystals. Palygorskite is the most common, covering the carbonate crystals and forming sheets between them. These lacustrine chalky carbonates were formed in the basinal areas of the lake as the result of inorganic carbonate precipitation and/or detrital sedimentation related to episodic reactivation of the adjacent fan systems. Their petrological, geochemical and physical properties indicate that few textural and compositional modifications occurred during diagenesis. Their main physical properties are a very low dry bulk and grain density (1.6–2.2 and 2.62 g/cm3, respectively) and medium to high porosity (10–40%) due to micropores ( < 2 Am, 70%) and macropores (>2 Am, 30%). The convergence of lacustrine sedimentation dynamics (rapid sedimentation), the original mineralogy of these calcareous lacustrine muds (relatively stable low-magnesian calcite and dolomite), the early formation of the palygorskite cement of these muds, and the retention of Mg-enriched fluids in the pore system, were decisive in the partial inhibition of calcite cementation, compaction and recrystallization. The chalky carbonates are also intercalated between impermeable littoral carbonate facies that impeded fluid flow through their pore systems.
dc.description.departmentDepto. de Mineralogía y Petrología
dc.description.facultyFac. de Ciencias Geológicas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/17289
dc.identifier.doi10.1016/j.sedgeo.2004.01.012
dc.identifier.issn0037-0738
dc.identifier.officialurlhttp://www.elsevier.com/locate/sedgeo
dc.identifier.urihttps://hdl.handle.net/20.500.14352/50216
dc.journal.titleSedimentary Geology
dc.language.isoeng
dc.page.final351
dc.page.initial335
dc.publisherElsevier B.V.
dc.rights.accessRightsopen access
dc.subject.cdu552.5(460.27)
dc.subject.keywordChalky carbonates
dc.subject.keywordLacustrine deposits
dc.subject.keywordPhysical properties
dc.subject.keywordOverpressure
dc.subject.keywordPalygorskite
dc.subject.keywordPalaeogene
dc.subject.ucmPetrología
dc.titleLacustrine chalky carbonates: origin, physical properties and diagenesis (Palaeogene of the Madrid Basin, Spain)
dc.typejournal article
dc.volume.number166
dspace.entity.typePublication
relation.isAuthorOfPublication4e978fda-4ea7-4a75-a2b7-643341f81141
relation.isAuthorOfPublicationd05d351d-a062-4537-8a68-9c05b3a3003d
relation.isAuthorOfPublication.latestForDiscovery4e978fda-4ea7-4a75-a2b7-643341f81141

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