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dc.contributor.author
Di Tommaso, Inés  
dc.contributor.author
Rubinstein, Nora Alicia  
dc.date.available
2019-05-13T19:58:52Z  
dc.date.issued
2007-09  
dc.identifier.citation
Di Tommaso, Inés; Rubinstein, Nora Alicia; Hydrothermal alteration mapping using ASTER data in the Infiernillo porphyry deposit, Argentina; Elsevier Science; Ore Geology Reviews; 32; 1-2; 9-2007; 275-290  
dc.identifier.issn
0169-1368  
dc.identifier.uri
http://hdl.handle.net/11336/76198  
dc.description.abstract
The Infiernillo Cu-(Mo) porphyry deposit is located in the San Rafael Massif, in southern Mendoza Province, Argentina. It is hosted by and genetically related to Lower Permian Gondwanan volcanic rocks, which developed in a magmatic arc tectonic setting. The alteration zone has an oval shape about 3 km × 2 km in size, with a NNE-SSW strike. It consists of a small central quartz neck with appreciable hematite surrounded by an intense quartz-injected zone with local pervasive potassic alteration. Outwards there is a well-developed phyllic halo with intense bleaching which consists of pervasive and vein-type silicification, sericitization and pyritization. Cu and Mo anomalies are approximately coincident and are located between the silicified zone and the phyllic halo. In the outer part of the alteration zone, small polymetallic veins with pyrite, arsenopyrite, galena and minor chalcopyrite, sphalerite and electrum in quartz gangue crop out. An Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), with three visible and near infrared (VNIR) bands, six shortwave infrared (SWIR) bands and five thermal infrared (TIR) bands, was used to characterize the Infiernillo porphyry deposit alteration area. A circular zoning pattern was clearly observed in the VNIR + SWIR band combination. Spectral analysis of the surface reflectance SWIR detected 2.20 and 2.26 μm absorptions. Field data and sample spectroscopic analyses obtained using a GER 3700 spectral radiometer and a SWIR reflectance spectrometer (Portable Infrared Mineral Analyzer PIMA) showed a good correlation with the ASTER data. The 2.20 μm absorptions, due to Al-hydroxyl, reveal the presence of clay minerals (Al-illite, kaolinite) and sericite, whereas the 2.26 μm absorption due to Fe-hydroxyl, resulted from jarosite. The field samples were also analyzed with a TIR portable spectrometer Micro-FTIR model 102. The TIR was useful for detecting surface silica and potassic alteration through analysis of five-band surface emissivity data. ASTER images provided preliminary mineralogic information and geo-referenced alteration maps at low cost and with high accuracy. In this way ASTER has been proven to be a powerful tool in the initial steps of ore deposit exploration.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
Elsevier Science  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Alteration Minerals  
dc.subject
Argentina  
dc.subject
Aster  
dc.subject
Mining Exploration  
dc.subject
Remote Sensing  
dc.subject.classification
Meteorología y Ciencias Atmosféricas  
dc.subject.classification
Ciencias de la Tierra y relacionadas con el Medio Ambiente  
dc.subject.classification
CIENCIAS NATURALES Y EXACTAS  
dc.title
Hydrothermal alteration mapping using ASTER data in the Infiernillo porphyry deposit, Argentina  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2019-05-02T17:55:41Z  
dc.journal.volume
32  
dc.journal.number
1-2  
dc.journal.pagination
275-290  
dc.journal.pais
Países Bajos  
dc.journal.ciudad
Amsterdam  
dc.description.fil
Fil: Di Tommaso, Inés. Secretaría de Industria y Minería. Servicio Geológico Minero Argentino; Argentina  
dc.description.fil
Fil: Rubinstein, Nora Alicia. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Geociencias Básicas, Aplicadas y Ambientales de Buenos Aires; Argentina  
dc.journal.title
Ore Geology Reviews  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://www.sciencedirect.com/science/article/pii/S016913680600076X  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/doi/https://doi.org/10.1016/j.oregeorev.2006.05.004