Please use this identifier to cite or link to this item: http://hdl.handle.net/1822/37490

TitleMetallogenesis at the Carris W–Mo–Sn deposit (Gerês, Portugal): constraints from fluid inclusions, mineral geochemistry, Re–Os and He–Ar isotopes
Author(s)Moura, António
Dória, A.
Neiva, A. M. R.
Gomes, C. Leal
Creaser, R. A.
KeywordsCarris
Tungsten
Portugal
Geochemistry
Fluid inclusions
Re–Os and He–Ar isotopes
Cards
Issue date2014
PublisherElsevier B.V.
JournalOre Geology Reviews
CitationA. Moura, A. Dória, A.M.R. Neiva, C. Leal Gomes, R.A. Creaser, Metallogenesis at the Carris W–Mo–Sn deposit (Gerês, Portugal): Constraints from fluid inclusions, mineral geochemistry, Re–Os and He–Ar isotopes, Ore Geology Reviews, Volume 56, January 2014, Pages 73-93, ISSN 0169-1368, http://dx.doi.org/10.1016/j.oregeorev.2013.08.001. (http://www.sciencedirect.com/science/article/pii/S0169136813001686)
Abstract(s)The Carris orebody consists of two partially exploited W–Mo–Sn quartz veins formed during successive shear stages and multipulse fluid fillings. They cut the Variscan post-D3 Gerês I-type granite. The most important ore minerals are wolframite, scheelite, molybdenite and cassiterite. There are two generations of wolframite. The earlier generation of wolframite is rare and has the highest WO4Mn content (91 mol%) and the most common wolframite contains 26–57 mol% WO4Mn. Re–Os dating of molybdenite from the ore quartz veins and surrounding granite yields ages of 279 ± 1.2 Ma and 280.3 ± 1.2 Ma, respectively which are in very good agreement with the previous ID-TIMS U–Pb zircon age for the Carris granite (280 ± 5 Ma). 3He/4He ratio of pyrite ranging between 0.73 and 2.71 Ra (1 Ra = 1.39 × 10−6) and high 3He/36Ar (0.8–5 × 10−3) indicate a mixture of a crustal radiogenic helium fluid with a mantle derived-fluid. The fluid inclusion studies on quartz intergrown with wolframite and scheelite, beryl and fluorite reveal that two distinct fluid types were involved in the genesis of this deposit. The first was a low to medium salinity aqueous carbonic fluid (CO2 between 4 and 14 mol%) with less than 1.95 mol% N2, which was only found in quartz associated with wolframite. The other was a low salinity aqueous fluid found in all the four minerals. The homogenization temperatures indicate minimum entrapment temperatures of 226–310 °C (average 280 °C) for the H2O– CO2–N2–NaCl fluid and average temperatures of 266 °C for scheelite and 242 °C, 190 °C and 160 °C for the last generations of beryl, fluorite and quartz, respectively. It was estimated that wolframite was deposited ~7 km depth, assuming a lithostatic pressure, probably due to strong pressure fluctuation caused by seismic events triggered by brittle tectonics during the exhumation event. Precipitation of scheelite and sulphides took place later, at the same depth, but under a hydrostatic or suprahydrostatic pressure regime, and probably caused by mixing between the magmatic–hydrothermal fluid and meteoric waters that deeply penetrated the basement during post-Variscan decompression.
TypeArticle
URIhttp://hdl.handle.net/1822/37490
DOI10.1016/j.oregeorev.2013.08.001
ISSN0169-1368
Publisher versionhttp://dx.doi.org/10.1016/j.oregeorev.2013.08.001
Peer-Reviewedyes
AccessRestricted access (UMinho)
Appears in Collections:CIG-R - Artigos (Papers)

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