Geología del yacimiento de Fe-Pb-Ag de la Mina Rica de Pulpí (Almería, España)
- Fernando J. Palero 1
- Àngels Canals 2
- Alexander van Driessche 3
- Juan Manuel García-Ruiz 1
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1
Instituto Andaluz de Ciencias de la Tierra
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2
Universitat de Barcelona
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- 3 Université Grenoble Alpes
ISSN: 0366-0176
Year of publication: 2020
Volume: 131
Issue: 4
Pages: 495-538
Type: Article
More publications in: Boletín geológico y minero
Abstract
The “Mina Rica” (the Rich Mine), located in the district of Pilar de Jaravía, in the municipality of Pulpi (Almería province, Spain), has become internationally renowned for the great geode of selenite gypsum discovered in its interior. The ore deposit is located in a NE-SW dextral shear band, affected by a system of NNE-SSW sinistral faults. The deposit is composed of two hectometric blocks of weakly deformed rocks with a pod shape, which are constituted by a folded and faulted alternation of limestone and dolomites, and to a lesser amount, gypsum and phyllites, all with a general NNESSW orientation and strong dipping to the W. In the time sequence of the mineral phases present in the “Mina Rica” we can distinguish a first stratabound, mineralization of iron carbonates that fossilizes the Serravallian age deformation. Baryte mineralization is associated with the Tortonian movements and celestine mineralization with the Messinian ones. Gypsum, which crystallized at a temperature of below 25ºC, was the last major sulphated mineral phase to be formed, and this took place after the Pliocene vertical replays. Moreover, this study – the cartographic underpinning of which has served as the basis for the recovery and musealization of the mine – has enabled us to discover the enormous potential that the “Mina Rica” has as a centre for geological and geo-mining practical teaching, beyond the indisputable lure of its Great Geode. We foresee that the results presented in this study will be the basis for the use of the “Mina Rica” as an educational tool to help train future generations of geologists and mining engineers.
Funding information
Este trabajo ha recibido financiaci?n del Ministerio de Educaci?n y Ciencia [MEC] a trav?s de los proyec-tos CGL2010?16882; CGL2010?12099-E, y CGL2016? 78971-P. Agradecemos el apoyo log?stico y t?cnico de Francisca Espinosa P?rez, Raquel Fern?ndez Penas y Mag? Baselga, as? como al Dr. Crist?bal Verdugo-Es-camilla por su ayuda con los an?lisis de difracci?n de Rayos X. Los autores agradecen las sugerencias y cometarios de dos de los revisores del trabajo, el Dr. Francisco Velasco y el Dr. Gabriel Ruiz de Almod?var. Agradecemos igualmente las facilidades concedidas por el ayuntamiento de Pulp? para la realizaci?n de este estudio y la Junta de Andaluc?a por su ayuda en el marco del Proyecto de Excelencia RNM 5384.Funders
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Ministerio de Economía y Competitividad
Spain
- 78971-P
- Ministério da Educação e Ciência Portugal