Spectroscopic comparison of aqueous Np(VI) and U(VI) species


Spectroscopic comparison of aqueous Np(VI) and U(VI) species

Müller, K.; Foerstendorf, H.; Tsushima, S.; Brendler, V.; Bernhard, G.

The distribution of aqueous species of actinide(VI) ions primarily defines their geochemical reactions and, thus, influences their migration behaviour in the environment. In aqueous solution, uranium and neptunium exist as actinyl ions AnO22+ (An = U, Np). They form different complexed species depending on their concentration level, pH range and the presence of potential ligands, such as carbonate. In recent years, the aqueous U(VI) system has been investigated intensively, in contrast to Np(VI). However, the thermodynamic data often arise from non-spectroscopic experiments mostly performed in the millimolar concentration range. [1] Up to now, a verification of the data of the different actinyl species by spectroscopic techniques providing direct molecular structural information is still incomplete. In particular, actinide solutions at lower concentrations and at neutral pH values, reasonably in an environmental context, were addressed seldom. [2]
In this study, the Np(VI) speciation at a submillimolar concentration range was investigated applying ATR FT-IR and NIR absorption spectroscopy, and computed modeling of updated NEA thermodynamic data. The findings are comparatively discussed with results obtained from U(VI) under identical conditions.
At ambient atmosphere, the formation of similar actinyl(VI) species can be derived from IR spectroscopic results at pH ≤ 4, namely the fully hydrated AnO22+ (An = U, Np) and monomeric hydrolysis products. At higher pH, the spectra evidence structurally different species contributing to the speciation of both actinides. At pH 5, the formation of (NpO2)2CO3(OH)3− probably occurs which is supported by modeling NEA data and results from NIR spectroscopy. For uranium, the presence of additional hydroxo complexes is assumed in this pH range.
1. Guillaumont, R. et al. Update on the Chemical Thermodynamics of U, Np, Pu, Am and Tc. Elsevier: Amsterdam, 2003; p 970.
2. Müller, K. et al. Inorganic Chemistry 2008, 47, (21), 10127-10134.

  • Lecture (Conference)
    Goldschmidt 2009 - "Challenges to Our Volatile Planet", 21.-26.06.2009, Davos, Schweiz
  • Geochimica et Cosmochimica Acta 73(2009)13S, A914

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