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Silicification and dolomitization of anhydrite nodules in argillaceous terrestrial deposits: an example of meteoric-dominated diagenesis from the Triassic of central Spain

dc.contributor.authorAlonso Zarza, Ana María
dc.contributor.authorSánchez Moya, Yolanda
dc.contributor.authorBustillo Revuelta, María Ángeles
dc.contributor.authorSopeña, Alfonso
dc.contributor.authorDelgado Huertas, Antonio
dc.date.accessioned2023-06-20T18:59:03Z
dc.date.available2023-06-20T18:59:03Z
dc.date.issued2002
dc.description.abstractCauliflower-shaped nodules are widespread in a single red mudstone bed in the Buntsandstein (Triassic) facies of the Iberian Range. They consist mostly of quartz, dolomite and calcite, but other minerals, such as barite, kaolinite and iron oxyhydroxides, are also present. The nodules are spherical, ovoid or elongate in shape and range from 1 to 8 cm across. The surface of the nodules is irregular, and some show a pedogenic coating of microspar. The sedimentological and petrographic data suggest that the initial anhydrite nodules formed through a progressive increase in the porewater concentration of Ca2+ and SO4 2– in a vadose environment, occasionally under the influence of pedogenic processes. Partial replacement of the anhydrite by megaquartz occurred under more dilute conditions in the same type of setting, as indicated by the presence of organic filaments on the quartz crystal surfaces. In type A nodules, the dissolution of the innermost anhydrite was complete, and different types of quartz cement filled the porosity. Fracturing and meteoric cementation by calcite and minor amounts of kaolinite were the latest processes affecting these nodules. In type B nodules, the dissolution of the anhydrite was incomplete, inhibiting quartz cementation and enabling later dolomitization of the anhydrite. Dolomitization appears to have been driven by sulphate reduction, as indicated by the presence of bacterial bodies within the dolomite crystals. Dedolomitization and precipitation of barite, kaolinite and calcite spar cements occurred later under the influence of meteoric solutions. The nodules may mark the former locations of the water table and provide evidence for an episode of highly evaporitic conditions throughout wide areas of the basin. Their occurrence reveals not only a complex diagenetic history but is also indicative of palaeogeographic and palaeoclimatic conditions.
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/25384
dc.identifier.issn0037-0746
dc.identifier.officialurlhttps://www.sedimentologists.org/publications/sedimentology
dc.identifier.urihttps://hdl.handle.net/20.500.14352/59045
dc.journal.titleSedimentology
dc.language.isoeng
dc.page.final317
dc.page.initial303
dc.publisherBlackwell Publishing Ltd
dc.rights.accessRightsopen access
dc.subject.cdu552.5(234.1)
dc.subject.cdu551.3.051(234.1)
dc.subject.keywordAnhydrite nodules
dc.subject.keywordMeteoric diagenesis
dc.subject.keywordSilicification
dc.subject.keywordSpain
dc.subject.keywordSulphate-reduction dolomitization
dc.subject.keywordTriassic
dc.subject.ucmPetrología
dc.titleSilicification and dolomitization of anhydrite nodules in argillaceous terrestrial deposits: an example of meteoric-dominated diagenesis from the Triassic of central Spain
dc.typejournal article
dc.volume.number49
dspace.entity.typePublication
relation.isAuthorOfPublicationf29ff48e-a667-4a09-89eb-a8c1b3d55083
relation.isAuthorOfPublication1b1efc7b-2481-4fb7-85a3-b2329812ea95
relation.isAuthorOfPublication.latestForDiscovery1b1efc7b-2481-4fb7-85a3-b2329812ea95

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