{"id":4124,"date":"2022-01-07T15:54:56","date_gmt":"2022-01-07T15:54:56","guid":{"rendered":"https:\/\/www.icterra.pt\/?p=4124"},"modified":"2022-01-07T15:54:56","modified_gmt":"2022-01-07T15:54:56","slug":"in-situ-la-icp-ms-trace-element-analysis-of-magnetite-as-a-vector-towards-mineral-exploration-a-comparative-case-study-of-fe-skarn-deposits-from-sw-iberia-ossa-morena-zone","status":"publish","type":"post","link":"https:\/\/www.icterra.pt\/legacy\/index.php\/2022\/01\/07\/in-situ-la-icp-ms-trace-element-analysis-of-magnetite-as-a-vector-towards-mineral-exploration-a-comparative-case-study-of-fe-skarn-deposits-from-sw-iberia-ossa-morena-zone\/","title":{"rendered":"In situ LA-ICP-MS trace element analysis of magnetite as a vector towards mineral exploration: A comparative case study of Fe-skarn deposits from SW Iberia (Ossa-Morena Zone)"},"content":{"rendered":"<p style=\"text-align: justify;\"><span style=\"font-size: 12pt; font-family: arial, helvetica, sans-serif;\">Miguel Maia, Pedro Barrulas, Pedro Nogueira, Jos\u00e9 Mir\u00e3o, Fernando Noronha, In situ LA-ICP-MS trace element analysis of magnetite as a vector towards mineral exploration: A comparative case study of Fe-skarn deposits from SW Iberia (Ossa-Morena Zone), Journal of Geochemical Exploration, Volume 234, 2022, 106941, ISSN 0375-6742,<\/span><br \/>\n<span style=\"font-size: 12pt; font-family: arial, helvetica, sans-serif;\">https:\/\/doi.org\/10.1016\/j.gexplo.2021.106941. <\/span><\/p>\n<p id=\"sp0105\" style=\"text-align: justify;\"><span style=\"font-size: 12pt; font-family: arial, helvetica, sans-serif;\">The Azenhas and Alvito Fe-deposits are located at SW of the Iberian\u00a0<a class=\"topic-link\" title=\"Learn more about Variscan from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/hercynian-orogeny\">Variscan<\/a>\u00a0belt, in a wide Fe-Zn ore district (Montemor-Ficalho Belt), part of the Ossa-Morena Zone. Both deposits are dominantly composed of\u00a0<a class=\"topic-link\" title=\"Learn more about magnetite from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/magnetite\">magnetite<\/a>\u00a0ores that display distinct ore formation processes and, at the Azenhas deposit, massive magnetite ores are mainly hosted in\u00a0<a class=\"topic-link\" title=\"Learn more about amphibolites from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/amphibolite\">amphibolites<\/a>\u00a0(Middle Cambrian \u2013 Ordovician), with a genesis arguably associated with metamorphic-metasomatic reactions promoted by fluid circulation through several\u00a0<a class=\"topic-link\" title=\"Learn more about thrust faults from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/geological-fault\">thrust faults<\/a>\u00a0that led to and expressive tectonic pilling. Contrastingly, the Alvito massive magnetite ores are formed by the\u00a0<a class=\"topic-link\" title=\"Learn more about emplacement from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/emplacement\">emplacement<\/a>\u00a0of a gabbro-dioritic suite in contact with calcite-dolomite marbles, constituting a typical calcic exoskarn Fe-skarn deposit. Primary and secondary magnetite were identified and characterized, and further selected for in situ\u00a0<a class=\"topic-link\" title=\"Learn more about laser ablation from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/laser-ablation\">laser ablation<\/a>\u00a0coupled inductively mass spectroscopy (LA-ICP-MS) trace element analysis. Results show that primary magnetite (Mag I) from the Azenhas deposit is discriminated by higher concentrations of Mg, Cr, Mn, Zn, Co, and Sn, whereas secondary magnetite (Mag II) is depleted in most trace elements, although displaying relatively higher concentrations of V, Ga, Mo, and Pb. The application of T<sub>Mg-Mag<\/sub>\u00a0geothermometer reinforced the discriminatory indexes, with Mag I displaying higher-temperature estimations (ca. 770\u00a0\u00b0C) when compared to Mag II (ca. 420\u00a0\u00b0C), thus suggesting that primary ores are associated to higher temperature processes than previously assumed.<\/span><\/p>\n<p id=\"sp0110\" style=\"text-align: justify;\"><span style=\"font-size: 12pt; font-family: arial, helvetica, sans-serif;\">Characterization of the ores from Alvito deposit revealed primary magnetite characterized by abundant\u00a0<a class=\"topic-link\" title=\"Learn more about ilmenite from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/ilmenite\">ilmenite<\/a>\u00a0and Al-spinel oxy-exsolutions which led to high measured Al concentrations in magnetite. The trace element content indicates high-temperature hydrothermal magnetite, underlining the contribution of hot\u00a0<a class=\"topic-link\" title=\"Learn more about hydrothermal fluids from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/hydrothermal-fluid\">hydrothermal fluids<\/a>\u00a0from the igneous body emplacement, also supported by the T<sub>Mg-Mag<\/sub>\u00a0geothermometer (ca. 685\u00a0\u00b0C). The anomalous presence of Co (max. 156\u00a0ppm) and Ni (max. 100\u00a0ppm) concentrations in Mag I from Alvito, along with pentlandite-magnetite assemblages, suggest that prone conditions were sustained for the development of Ni-bearing ores and that magnetite composition could be an interesting geochemical proxy for the exploration of such\u00a0<a class=\"topic-link\" title=\"Learn more about mineralization from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/mineralization\">mineralization<\/a>.<\/span><\/p>\n<p id=\"sp0115\" style=\"text-align: justify;\"><span style=\"font-size: 12pt; font-family: arial, helvetica, sans-serif;\">The Mn\u00a0+\u00a0Al versus Ti\u00a0+\u00a0V discriminant diagram shows that primary ores from both deposits plot in the\u00a0<a class=\"topic-link\" title=\"Learn more about skarn from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/skarn\">skarn<\/a>\u00a0field. The combination of magnetite analyses with whole-rock\u00a0<a class=\"topic-link\" title=\"Learn more about geochemistry from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/geochemistry\">geochemistry<\/a>\u00a0and field geology, allowed us to define criteria that can be applied in the discrimination of Fe-deposits and contribute to improve the geological models of the studied\u00a0<a class=\"topic-link\" title=\"Learn more about ore deposits from ScienceDirect's AI-generated Topic Pages\" href=\"https:\/\/www.sciencedirect.com\/topics\/earth-and-planetary-sciences\/ore-deposit\">ore deposits<\/a>, thus beneficiating future exploration in SW Iberia.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Miguel Maia, Pedro Barrulas, Pedro Nogueira, Jos\u00e9 Mir\u00e3o, Fernando Noronha, In situ LA-ICP-MS trace element analysis of magnetite as a vector towards mineral exploration: A comparative case study of Fe-skarn deposits from SW Iberia (Ossa-Morena Zone), Journal of Geochemical Exploration, Volume 234, 2022, 106941, ISSN 0375-6742, https:\/\/doi.org\/10.1016\/j.gexplo.2021.106941. The Azenhas and Alvito Fe-deposits are located at [&hellip;]<\/p>\n","protected":false},"author":3,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[16],"tags":[],"_links":{"self":[{"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/posts\/4124"}],"collection":[{"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/comments?post=4124"}],"version-history":[{"count":1,"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/posts\/4124\/revisions"}],"predecessor-version":[{"id":4125,"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/posts\/4124\/revisions\/4125"}],"wp:attachment":[{"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/media?parent=4124"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/categories?post=4124"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.icterra.pt\/legacy\/index.php\/wp-json\/wp\/v2\/tags?post=4124"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}