Mina de Sn San Rafael Peru.pdf

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    Constraints on the genesis of lode-style tin mineralization: evidence from

    the San Rafael tin-copper deposit, Peru

    Michael S.J. MlynarczykMay 2005

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    Plan of the presentation

    Tin metallogeny in the Central Andes

    The San Rafael Sn-Cu deposit:- structural geology- alteration

    - mineralization- fluid inclusions- stable isotopes

    Genetic model

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    The metallogeny of the Central Andes

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    A collisional model for tin metallogeny

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    The San Rafael tin deposit

    ~ 1,000,000 tonnes Sn metal, average grade ~ 5 wt.% Sn

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    Geology of the San Rafael area

    granite

    slate

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    One major vein-breccia system (the San Rafael lode)

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    Variation in normative mineralogy: early sericitic andtourmaline alteration versus main-stage chloritization

    Freshgranite

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    Chemical zoning of hydrothermal tourmaline:from early dravite (Mg) to ore-stage schorl (Fe)

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    Physico-chemical conditions of chloritic alteration

    associated with main-stage cassiterite deposition

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    Ore mineralogy and metal zoning

    cas

    Upper zone: sulfides dominate, complex mineralogy(chalcopyrite, pyrite, arsenopyrite, sphalerite, galenapyrrhotite, needle-tin cassiterite, quartz, chlorite)

    Lower zone: oxides/silicates dominate, simple mineralogy(massive cassiterite, quartz, chlorite wolframite)

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    Fluid inclusion studies

    18 m

    15 m

    qtz

    cas

    Ore fluids of moderate T(360-230C) and fluctuatingsalinity (21-0 wt.% NaCl eq.)

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    Stable isotope studies

    34 S V-CDT ()

    18 O V-SMOW ()

    18 O V-SMOW ()

    cas

    qtz

    chl wol

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    Isotopic evolution of hydrothermal fluids at San Rafael

    Calculated valuesof 18 O and D forwater in equilibriumwith the different oreand gangue minerals(at the temperatureof their formation),exhibit a clearparagenetic trendof 18 O decrease.

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    Mineral stabili ty relationships for the tin stage (II) and thecopper stage (III) of the San Rafael paragenesis

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    Effect of cooling and mixing of magmatic and meteoricfluids on the oxygen isotope composition of

    precipitating quartz (A) and cassiterite (B)

    Only a scenario of mixing of a hot brine with a cooler,dilute fluid can reproduce the range of oxygen isotope

    compositions of quartz and cassiterite from the deposit

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    A genetic model for San Rafael

    qtz

    cas

    Early stage: lithostatic conditions, hot magmatic brines produce strongsericite + tourmaline alteration and sealed, barren, tourmaline-quartz veins.

    Main ore stage: mixing of magmatic brines and meteoric waters in the fault- jogs oxidation, dilution, cooling, and acid neutralization of the ore fluids massive precipitation of cassiterite as localized, high-grade ore shoots.

    Tectonic activity reopens the vein system transition to hydrostatic

    conditions + influx of heated meteoric waters.

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    Thank you for your attention...