Article

Computational Studies of Structural, Electronic, Spectroscopic, and Thermodynamic Properties of Methylmercury-Amino Acid Complexes and Their Se Analogues

Department of Chemistry, University of Manitoba, Winnipeg, Manitoba Canada R3T 2N2
Inorg. Chem., 2010, 49 (3), pp 870–878
DOI: 10.1021/ic900827m
Publication Date (Web): December 31, 2009
Copyright © 2009 American Chemical Society
*To whom correspondence should be addressed. E-mail: schrecke@cc.umanitoba.ca; wangf@ms.umanitoba.ca.

Synopsis

CH3Hg−Se bond is weaker than CH3Hg−S, but its formation is more favorable thermodynamically.

Abstract

Abstract Image

Quantum chemical calculations have been carried out to study the structural, electronic, spectroscopic, and thermodynamic properties of five methylmercury-amino acid complexes and their selenium analogues. The structural properties of methylmercury-amino acids are very similar to their Se analogues except for those properties that are directly related to the Se atom which has a larger covalent radius. Characteristic stretching frequencies are observed for Hg−S/Se and Hg−C bonds. Electronic properties of both methylmercury-amino acids and their Se analogues are different from each other, with the S complexes showing stronger electrostatic attractions which leads to stronger bonds to mercury. The methylmercury complexes with selenoamino complexes, however, are thermodynamically more favorable (ΔG of formation from suitable model reactants) than those of the corresponding amino acid complexes. This can be traced to the lower stability of the reactant selenoamino acids. Such different stability and favorability of formation might be responsible for the different physiological activity in biological systems such as the Hg−Se antagonism.

Full citation for reference 17; Tables S1 to S4 showing energetics obtained with smaller basis sets (Table S1), results for Priroda-PBE calculations (Tables S2, S3), and solvation energies (Table S4). This material is available free of charge via the Internet at http://pubs.acs.org.

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Received 28 April 2009
Published online 31 December 2009
Published in print 1 February 2010
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