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The Almadén district (Spain): Anatomy of one of the world’s largest Hg-contaminated sites

dc.contributor.authorHigueras, Pablo
dc.contributor.authorOyarzun Muñoz, Roberto
dc.contributor.authorLillo, Javier
dc.contributor.authorSánchez-Hernández, Jaime
dc.contributor.authorMolina Abril, José Antonio
dc.contributor.authorEsbrí Víctor, José María
dc.contributor.authorLorenzo Álvarez, Saturnino
dc.date.accessioned2023-06-20T12:59:34Z
dc.date.available2023-06-20T12:59:34Z
dc.date.issued2006
dc.description.abstractWe present data from an early reconnaissance survey (stream sediments, soil, and water Hg chemistry; plants and water crustaceans Hg intake) of the Almade´n district (central Spain), that was carried out to establish the potential environmental hazards derived from the anomalous mercury concentrations measured in this realm. The Almade´n mercury district (~300 km2) can be regarded as the largest geochemical anomaly of mercury on Earth. The district includes a series of mercury mineral deposits, having in common a simple mineralogy (dominant cinnabar: HgS, and minor pyrite: FeS2). The ore deposits have been mined for more than 2000 years, and the main mine of the district (Almade´n), has been active from Roman times to present day with almost no interruptions. The mercury distribution in soils of the district reveals the existence of high, and extremely high mercury values (up to 8889 Ag g-1), whereas concentrations in stream sediments and waters reach exceptional values of up to 16,000 Ag g-1 and 11,200 ng l-1 respectively. On the other hand, very high concentrations of methylmercury (MeHg) have been detected in calcines (up to 3100 ng g-1), sediments (0.32–82 ng g-1), and waters (0.040–30 ng l-1). Mercury gets incorporated to edible river crustaceans and plants. The red swamp crayfish Procambarus clarkii, has Hg concentrations of up to 9060 ng g-1 (muscle) and 26,150 ng g-1 (hepatopancreas). Regarding plants, the local wild asparagus (Asparagus acutifolius) yields values of up to 298 Ag g-1 Hg. Mercury also escapes to the atmosphere, and mineral deposits, together with metallurgical activities, generate strong anomalies of atmospheric Hg. The most important concentrations relate to the emissions from the Almade´n metallurgical roaster, in the order of 14,000 ng Hg m-3. Additionally, large open pit operations also contribute to the district atmospheric pool of mercury, with high concentrations above 1000 ng Hg m-3. Thus, no system (rocks, soils, sediments, waters, atmosphere, biota) in the Almadén district is free from strong Hg contamination.
dc.description.departmentDepto. de Mineralogía y Petrología
dc.description.facultyFac. de Ciencias Geológicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Ciencia y Tecnología
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/78655
dc.identifier.doi10.1016/j.scitotenv.2005.04.042
dc.identifier.issn0048-9697, ESSN: 1879-1026
dc.identifier.officialurlhttps://doi.org/10.1016/j.scitotenv.2005.04.042
dc.identifier.urihttps://hdl.handle.net/20.500.14352/52934
dc.journal.titleScience of the total environment
dc.language.isoeng
dc.page.final124
dc.page.initial112
dc.publisherElsevier
dc.relation.projectIDProject 1FD97-0814
dc.relation.projectIDREN2002- 02231
dc.relation.projectIDPPQ2003-01902
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject.cdu553
dc.subject.cdu550.4
dc.subject.keywordMercury
dc.subject.keywordContamination
dc.subject.keywordAlmadén
dc.subject.keywordSoils
dc.subject.keywordSediments
dc.subject.keywordWater
dc.subject.keywordAtmosphere
dc.subject.ucmGeoquímica
dc.subject.unesco2503 Geoquímica
dc.titleThe Almadén district (Spain): Anatomy of one of the world’s largest Hg-contaminated sites
dc.typejournal article
dc.volume.number356
dspace.entity.typePublication
relation.isAuthorOfPublication07e25399-5798-4f11-95b9-6084418bfe0b
relation.isAuthorOfPublication73f79f2c-b757-4200-9f96-a92cc96997f1
relation.isAuthorOfPublicationee8242f5-b953-4953-98a5-f802cbcac593
relation.isAuthorOfPublication.latestForDiscovery73f79f2c-b757-4200-9f96-a92cc96997f1

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