Geology, geochemistry and mineralogy of the Loma de Hierro Ni-laterite deposit, Venezuela

Ni-laterite deposits host over 60% of the word land-based Ni resources (McRae, 2018). They formed from the weathering of Mg-rich ultramafic rocks exposed to the surface under favorable topography and climatic conditions. The typical Ni-laterite profile is characterized by a partially serpentinized p...

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Detalles Bibliográficos
Autores: Domènech Ortí, Cristina, Galí Medina, Salvador, 1949-, Ancco, Marite P., Villanova de Benavent, Cristina, Soler, Josep M., Meléndez, Willians, Rondón, José, Proenza Fernández, Joaquín Antonio
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2018
País:España
Institución:Varias* (Consorci de Biblioteques Universitáries de Catalunya, Centre de Serveis Científics i Acadèmics de Catalunya)
Repositorio:Recercat. Dipósit de la Recerca de Catalunya
OAI Identifier:oai:recercat.cat:2445/134888
Acceso en línea:https://hdl.handle.net/2445/134888
Access Level:acceso abierto
Palabra clave:Compostos de níquel
Laterita
Veneçuela
Prospecció geoquímica
Nickel compounds
Laterite
Venezuela
Geochemical prospecting
Descripción
Sumario:Ni-laterite deposits host over 60% of the word land-based Ni resources (McRae, 2018). They formed from the weathering of Mg-rich ultramafic rocks exposed to the surface under favorable topography and climatic conditions. The typical Ni-laterite profile is characterized by a partially serpentinized parent rock (protolith) at the bottom followed by a saprolite horizon (dominated by secondary Si- and Mg-bearing minerals), and a limonitic horizon, dominated by goethite that evolves to hematite with time (e.g. Golightly, 2010). Ni originally liberated from olivine is concentrated in different secondary minerals such as goethite in the limonite and garnierites, secondary serpentines and/or smectite in the saprolite zone (Pelletier 1996; Villanova-de-Benavent et al. 2014). Ni-laterites are classified according to their dominant Ni-bearing ore in (a) hydrous-Mg-silicate, (b) clay and (c) oxide type deposits (Brand et al. 1998)