Mineralogy of atmospheric dust impacting the Rio Tinto mining area (Spain) during episodes of high metal deposition
This study is the first to investigate the mineral composition of the atmospheric particulate matter deposited at Rio Tinto, Spain, an historical mining district of world-class importance, with emphasis on metal-bearing particles and their environmental implications. The dustfall is composed of quartz, feldspars, phyllosilicates (mica, chlorite and/or kaolinite) and a variety of accessory heavy minerals, the most common being primary sulfides (pyrite, chalcopyrite with minor galena, sphalerite and bornite) and their oxidation products (notably goethite, hematite and jarosite). This mineral assemblage suggests a local source of wind-blown dust and it is consistent with the large deposition levels of sulfide-related elements (As, Bi, Cd, Cu, Pb, Sb and Zn) registered at the sampling site adjacent to the mine waste dumps. However, the generation of potentially harmful dust particles is not restricted to mine wastes. Anthropogenic metallic compounds arising from a nearby hazardous waste disposal centre can make a relevant additional contribution to the metal deposition, particularly for Fe, Ni, Cr and Mn. Atmospheric fallout is a major mechanism for metal input to soils and plants around or near the mining area. ; This study was supported by grants from the Spanish Ministry of Science and Innovation (Projects CRACCIE-CSD2007-0067 and CGL2008-06270-C02-02/CLI) and the Department of the Environment, and the Department of Innovation, Science and Enterprise (Projects RNM2007-02729 and RNM2009-5163M) of the Andalusia Autonomous Government. Karen Hudson-Edwards and an anonymous reviewer are thanked for their constructive comments and suggestions.