Matches in SemOpenAlex for { <https://semopenalex.org/work/W2146305422> ?p ?o ?g. }
- W2146305422 endingPage "386" @default.
- W2146305422 startingPage "363" @default.
- W2146305422 abstract "Tin-polymetallic greisen-type deposits in the Itu Rapakivi Province and Rondônia Tin Province, Brazil are associated with late-stage rapakivi fluorine-rich peraluminous alkali-feldspar granites. These granites contain topaz and/or muscovite or zinnwaldite and have geochemical characteristics comparable to the low-P sub-type topaz-bearing granites. Stockworks and veins are common in Oriente Novo (Rondônia Tin Province) and Correas (Itu Rapakivi Province) deposits, but in the Santa Bárbara deposit (Rondônia Tin Province) a preserved cupola with associated bed-like greisen is predominant. The contrasting mineralization styles reflect different depths of formation, spatial relationship to tin granites, and different wall rock/fluid proportions. The deposits contain a similar rare-metal suite that includes Sn (±W, ±Ta, ±Nb), and base-metal suite (Zn–Cu–Pb) is present only in Correas deposit. The early fluid inclusions of the Correas and Oriente Novo deposits are (1) low to moderate-salinity (0–19 wt.% NaCl eq.) CO2-bearing aqueous fluids homogenizing at 245–450 °C, and (2) aqueous solutions with low CO2, low to moderate salinity (0–14 wt.% NaCl eq.), which homogenize between 100 and 340 °C. In the Santa Bárbara deposit, the early inclusions are represented by (1) low-salinity (5–12 wt.% NaCl eq.) aqueous fluids with variable CO2 contents, homogenizing at 340 to 390 °C, and (2) low-salinity (0–3 wt.% NaCl eq.) aqueous fluid inclusions, which homogenize at 320–380 °C. Cassiterite, wolframite, columbite–tantalite, scheelite, and sulfide assemblages accompany these fluids. The late fluid in the Oriente Novo and Correas deposit was a low-salinity (0–6 wt.% NaCl eq.) CO2-free aqueous solution, which homogenizes at (100–260 °C) and characterizes the sulfide–fluorite–sericite association in the Correas deposit. The late fluid in the Santa Bárbara deposit has lower salinity (0–3 wt.% NaCl eq.) and characterizes the late-barren-quartz, muscovite and kaolinite veins. Oxygen isotope thermometry coupled with fluid inclusion data suggest hydrothermal activity at 240–450 °C, and 1.0–2.6 kbar fluid pressure at Correas and Oriente Novo. The hydrogen isotope composition of breccia-greisen, stockwork, and vein fluids (δ18Oquartz from 9.9‰ to 10.9‰, δDH2O from 4.13‰ to 6.95‰) is consistent with a fluid that was in equilibrium with granite at temperatures from 450 to 240 °C. In the Santa Bárbara deposit, the inferred temperatures for quartz-pods and bed-like greisens are much higher (570 and 500 °C, respectively), and that for the cassiterite-quartz-veins is 415 °C. The oxygen and hydrogen isotope composition of greisen and quartz-pods fluids (δ18Oqtz-H2O=5.5–6.1‰) indicate that the fluid equilibrated with the albite granite, consistent with a magmatic origin. The values for mica (δ18Omica-H2O=3.3–9.8‰) suggest mixing with meteoric water. Late muscovite veins (δ18Oqtz-H2O=−6.4‰) and late quartz (δ18Omica-H2O=−3.8‰) indicate involvement of a meteoric fluid. Overall, the stable isotope and fluid inclusion data imply three fluid types: (1) an early orthomagmatic fluid, which equilibrated with granite; (2) a mixed orthomagmatic-meteoric fluid; and (3) a late hydrothermal meteoric fluid. The first two were responsible for cassiterite, wolframite, and minor columbite–tantalite precipitation. Change in the redox conditions related to mixing of magmatic and meteoric fluids favored important sulfide mineralization in the Correas deposit." @default.
- W2146305422 created "2016-06-24" @default.
- W2146305422 creator A5012907008 @default.
- W2146305422 creator A5018228756 @default.
- W2146305422 creator A5031302560 @default.
- W2146305422 creator A5055057445 @default.
- W2146305422 creator A5062017201 @default.
- W2146305422 creator A5076743623 @default.
- W2146305422 date "2005-03-01" @default.
- W2146305422 modified "2023-10-06" @default.
- W2146305422 title "Sn-polymetallic greisen-type deposits associated with late-stage rapakivi granites, Brazil: fluid inclusion and stable isotope characteristics" @default.
- W2146305422 cites W1521686919 @default.
- W2146305422 cites W1535539135 @default.
- W2146305422 cites W1548612573 @default.
- W2146305422 cites W1577817975 @default.
- W2146305422 cites W1588154159 @default.
- W2146305422 cites W183994653 @default.
- W2146305422 cites W192102247 @default.
- W2146305422 cites W1976231896 @default.
- W2146305422 cites W1990006396 @default.
- W2146305422 cites W1990581568 @default.
- W2146305422 cites W1996361224 @default.
- W2146305422 cites W2003892405 @default.
- W2146305422 cites W2008200349 @default.
- W2146305422 cites W2014541757 @default.
- W2146305422 cites W2014945279 @default.
- W2146305422 cites W2017934677 @default.
- W2146305422 cites W2025140431 @default.
- W2146305422 cites W2030987430 @default.
- W2146305422 cites W2035419363 @default.
- W2146305422 cites W2036565101 @default.
- W2146305422 cites W2038902246 @default.
- W2146305422 cites W2044485855 @default.
- W2146305422 cites W2044537972 @default.
- W2146305422 cites W2047456637 @default.
- W2146305422 cites W2048072603 @default.
- W2146305422 cites W2053024421 @default.
- W2146305422 cites W2055895721 @default.
- W2146305422 cites W2059927840 @default.
- W2146305422 cites W2065940550 @default.
- W2146305422 cites W2068202901 @default.
- W2146305422 cites W2081110574 @default.
- W2146305422 cites W2081149290 @default.
- W2146305422 cites W2084463468 @default.
- W2146305422 cites W2091694423 @default.
- W2146305422 cites W2109567412 @default.
- W2146305422 cites W2114810510 @default.
- W2146305422 cites W2119012997 @default.
- W2146305422 cites W2119996772 @default.
- W2146305422 cites W2129169912 @default.
- W2146305422 cites W2135785473 @default.
- W2146305422 cites W2135844641 @default.
- W2146305422 cites W2149206725 @default.
- W2146305422 cites W2153653187 @default.
- W2146305422 cites W2169746538 @default.
- W2146305422 cites W2181544355 @default.
- W2146305422 cites W2252589237 @default.
- W2146305422 cites W2258888910 @default.
- W2146305422 cites W2295385638 @default.
- W2146305422 cites W2297549454 @default.
- W2146305422 cites W2313236783 @default.
- W2146305422 cites W2325628207 @default.
- W2146305422 cites W2338438729 @default.
- W2146305422 cites W2339102711 @default.
- W2146305422 cites W2491208108 @default.
- W2146305422 cites W2502358655 @default.
- W2146305422 cites W2519196423 @default.
- W2146305422 cites W2531718170 @default.
- W2146305422 cites W2748958707 @default.
- W2146305422 cites W2890347532 @default.
- W2146305422 cites W2979595134 @default.
- W2146305422 cites W3087383627 @default.
- W2146305422 cites W313278945 @default.
- W2146305422 cites W3179955293 @default.
- W2146305422 cites W3198427848 @default.
- W2146305422 cites W3200525091 @default.
- W2146305422 cites W3207348335 @default.
- W2146305422 cites W810407324 @default.
- W2146305422 doi "https://doi.org/10.1016/j.lithos.2004.03.060" @default.
- W2146305422 hasPublicationYear "2005" @default.
- W2146305422 type Work @default.
- W2146305422 sameAs 2146305422 @default.
- W2146305422 citedByCount "50" @default.
- W2146305422 countsByYear W21463054222012 @default.
- W2146305422 countsByYear W21463054222013 @default.
- W2146305422 countsByYear W21463054222014 @default.
- W2146305422 countsByYear W21463054222015 @default.
- W2146305422 countsByYear W21463054222016 @default.
- W2146305422 countsByYear W21463054222017 @default.
- W2146305422 countsByYear W21463054222018 @default.
- W2146305422 countsByYear W21463054222019 @default.
- W2146305422 countsByYear W21463054222020 @default.
- W2146305422 countsByYear W21463054222021 @default.
- W2146305422 countsByYear W21463054222022 @default.
- W2146305422 countsByYear W21463054222023 @default.
- W2146305422 crossrefType "journal-article" @default.
- W2146305422 hasAuthorship W2146305422A5012907008 @default.
- W2146305422 hasAuthorship W2146305422A5018228756 @default.