Please use this identifier to cite or link to this item: http://hdl.handle.net/10553/49805
Title: The formation of Cu(II) complexes with carbonate and bicarbonate Ions in NaClO4 solutions
Authors: Millero, Frank J.
Santana-Casiano, J. Magdalena 
González-Dávila, Melchor 
UNESCO Clasification: 251002 Oceanografía química
230331 Química del agua
Keywords: Cu(II)
Metals
Carbonato complexes
Speciation
Pitzer equations, et al
Issue Date: 2010
Project: Estudio Del Comportamiento Químico Del Hierro en El Medio Marino en Presencia de Compuestos Orgánicos de Origen Fitoplanctónico 
Journal: Journal of Solution Chemistry 
Abstract: The inorganic behavior of most divalent metals in natural waters is affected by the formation of carbonate complexes. The acidification of the oceans will lower the carbonate concentration in the oceans. This will increase the concentration of free copper that is toxic to marine organisms. To be able to determine the effect of this acidification, reliable stability constants are needed for the formation of copper carbonate complexes. In this paper, the speciation of Cu(II) with bicarbonate and carbonate ions is investigated as a function of ionic strength and temperature in NaClO4 solutions. To fully examine the system, the dissociation of carbonic acid in the media were examined using the Pitzer equations in NaClO4 solutions to 6.5 mol⋅kg−1 at 25 °C. With this foundation, the stability constants for the formation of Cu(II) carbonate complexes were used to determine the activity coefficients for the complexes (CuHCO+3, CuCO3, Cu(CO3)2−2). Pitzer parameters for these complexes were determined at 25 °C and ionic strength (0 to 1.1 mol⋅kg−1) in NaClO4 solutions. Since the formation of Cu(II) carbonate complexes appear to be linearly related to the values for other metals, it is possible to use the correlations to estimate the carbonate constants for a number of other divalent metals.
URI: http://hdl.handle.net/10553/49805
ISSN: 0095-9782
DOI: 10.1007/s10953-010-9523-z
Source: Journal of Solution Chemistry [ISSN 0095-9782], v. 39 (4), p. 543-558
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