Genesis and New Mineral Chemistry Data of Carlosbarbosaite, a Potential U and Nb Ore Source from Miarolitic-, A-Type Granites and NYF Pegmatites of the La Chinchilla Pluton, Velasco Ranges, La Rioja, Argentina

Author:

Lira Raúl12,Parra Francisco J.3,Biglia Marco E.1,Morello Orquídea4,Guereschi Alina B.5

Affiliation:

1. Museo de Mineralogía y Geología “Dr. Alfred W. Stelzner”, FCEFyN, Universidad Nacional de Córdoba. Av. Vélez Sarsfield 249, X5000JJC, Córdoba, Argentina

2. Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET), Av. Vélez Sarsfield 249, X5000JJC, Córdoba, Argentina

3. Comisión Nacional de Energía Atómica, Subgerencia Regional Centro. Espinel 902, X5001BKW, Córdoba, Argentina

4. Comisión Nacional de Energía Atómica. Av. del Libertador 8250, (1429) Ciudad Autónoma de Buenos Aires, Argentina

5. Departamento de Geología Básica (Facultad de Ciencias Exactas, Físicas y Naturales, Universidad Nacional de Córdoba) and Centro de Investigaciones en Ciencias de la Tierra (CONICET - Universidad Nacional de Córdoba). Av. Vélez Sársfield 1611, X5016GCA, Córdoba, Argentina

Abstract

Abstract The La Chinchilla granite is a ∼3.75 km2 epizonal pluton of Lower Carboniferous age located in Sierra de Velasco, Sierras Pampeanas, Argentina. Equigranular micropegmatitic and porphyritic main granite types host abundant millimeter- to <2 m-sized miarolitic pegmatites and pockets of simple major mineralogy (±beryl). Both granite types host micrometer-sized accessory species [i.e., monazite-(Ce), several high field strength element oxide species, ilmenite, cassiterite, fluorapatite] and fluorite. A F-Na-rich fluid phase promoted strong albitization at late-miarolitic stages, along with crystallization of extremely F-rich polylithionite and fluorite, and the formation of replacing pyrochlore group species associated with a second generation of cassiterite. The increase of the Ta# from hydroxycalciopyrochlore to hydroxycalciomicrolite and from micromiarolitic cassiterite (cassiterite 1) to hydrothermal cassiterite (cassiterite 2) supports Nb-Ta fractionation at hydrothermal temperatures. Carlosbarbosaite [(UO2)2Nb2O6(OH)2·2H2O] occurs as a pseudomorphic or short-range transported phase. Low-T, hydrothermal carlosbarbosaite formed after the replacement of columbite-(Fe), U-free Nb-bearing ilmenite, and likely after U-bearing pyrochlore supergroup species and a columbite group mineral, plausibly due to interaction with a hydrothermal, U6+(±Nb±Ta)-enriched fluid, in some cases a SiO2-bearing fluid. This fluid likely represents a lower T, less alkaline, and more oxidizing fluid that evolved from the higher T F-Na-rich fluids active during the late-miarolitic hydrothermal stage. Low-T, hydrothermal carlosbarbosaite has the ideal U-,Nb-rich endmember composition, though it is significantly richer in Ca and poorer in total Nb+Ta but with higher Nb# than that from the type locality. Supergene fluids deposited the transported type, which attained economic concentrations in a fault zone where restricted, likely alkaline oxidizing conditions could have favored Nb mobility.

Publisher

Mineralogical Association of Canada

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