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A geostatistical approach for mercury spatial patterns assessment in sediments in an old mining region: The Caveira Mine case study, Portugal

dc.contributor.authorMota, Natália
dc.contributor.authorFonseca, Rita
dc.contributor.authorAraújo, Joana
dc.contributor.authorIsabel Margarida Horta Ribeiro Antunes
dc.contributor.authorValente, Teresa
dc.contributor.authorBarroso, Ana
dc.contributor.authorAraújo, Alexandre
dc.contributor.authorAlbuquerque, Maria Teresa
dc.contributor.editorZanini , Andrea
dc.contributor.editorD'Oria, Marco
dc.date.accessioned2025-04-08T11:47:15Z
dc.date.available2025-04-08T11:47:15Z
dc.date.issued2022
dc.description.abstractMercury pollution is significant in many former mining communities worldwide, including in developing countries. Anthropic contributions to environmental Hg pollution are mostly connected to fuel fossil emissions, industrial and mining activities. Among mining operations, gold exploration contributes to the highest Hg contamination rates, given the processes, widely used in the past, of mixing Hg with the gold containing ore, to separate this metal from the bulk impurities. This study, as part of the GeoMaTre project, an ongoing collaborative network (2021-2024) between the Polytechnic Institute of Castelo Branco and the University of Évora, Portugal, aimed to evaluate the potential risk of mercury pollution in stream sediments in the Caveira area, an abandoned Cu, Pb, Zn, Ag, and Au mine, included in the Iberian Pyrite Belt, at South Portugal. This mine corresponds to a Gossan developed on pyrite mineralization, with high gold and silver content at the official beginning of its exploitation, in 1863, having exhausted the reserves in these precious metals in the 1920s. Until the date of its abandonment (1966) the exploitation focused on the remaining metals (Cu, Pb, Zn) and S. Currently, the surrounding area of Caveira mine is essentially composed of areas of waste accumulation, from mining activity, with little or no vegetation. Thirty-three sediment samples were collected from within 0 to 10 cm depth, in a grid of 1Km x 1Km. Hg was determined in samples preserved at about 4ºC at the time of collection, through a mercury analyzer (NIC MA 3000) based on thermal decomposition, gold amalgamation, and cold vapor atomic absorption spectroscopy detection.eng
dc.identifier.citationMOTA, Natália [et al.] (2022) - A geostatistical approach for mercury spatial patterns assessment in sediments in an old mining region: The Caveira Mine case study, Portugal. In 14th International Conference on Geostatistics for Environmental Applications (geoENV2022), Parma, 2022 - Ecology, Natural, Resources: Proceedings. Parma : Università. P. 2-3.
dc.identifier.urihttp://hdl.handle.net/10400.11/10118
dc.language.isoeng
dc.peerreviewedyes
dc.publisherUniversità di Parma
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.subjectCaveira mine
dc.subjectMercury
dc.subjectSequential Gaussian sSimulation
dc.subjectG clustering
dc.subjectProbability map
dc.titleA geostatistical approach for mercury spatial patterns assessment in sediments in an old mining region: The Caveira Mine case study, Portugalpor
dc.typeconference paper
dspace.entity.typePublication
oaire.citation.conferencePlaceParma, Itália
oaire.citation.endPage3
oaire.citation.startPage2
oaire.citation.title14th International Conference on Geostatistics for Environmental Applications (geoENV2022)
oaire.versionhttp://purl.org/coar/version/c_970fb48d4fbd8a85
person.familyNameantunes
person.familyNameAlbuquerque
person.givenNameIsabel Margarida
person.givenNameMaria Teresa
person.identifier.ciencia-idCB1E-FAD2-37D6
person.identifier.ciencia-id5A1C-8956-4C0A
person.identifier.orcid0000-0003-3456-5926
person.identifier.orcid0000-0002-8782-6133
person.identifier.ridM-1043-2013
person.identifier.ridB-1536-2013
person.identifier.scopus-author-id6701817085
person.identifier.scopus-author-id55507421600
relation.isAuthorOfPublication1db83c95-f80c-41bb-b5c6-437ab32d9683
relation.isAuthorOfPublicatione2c2d171-e148-4c23-9cf8-0eb6d810c15e
relation.isAuthorOfPublication.latestForDiscovery1db83c95-f80c-41bb-b5c6-437ab32d9683

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