MECHANISMS OF NI SORPTION TO MN OXYHYDROXIDE FROM EXAFS AND IMPLICATIONS FOR NI ISOTOPE MASS BALANCE IN THE OCEANS
To examine the molecular mechanisms by which Ni is incorporated into Mn oxyhydroxides, we conducted sorption experiments at low and high ionic strength with synthetic birnessite. We measured Ni stable isotope ratios and collected Ni EXAFS spectra from our experimental products. At low ionic strength, in short-duration experiments, we found that sorbed Ni is 1.4‰ lighter than dissolved Ni. This contrasts with what is observed between seawater and natural crusts. We can fit the EXAFS spectra for these samples well with a linear combination of Ni in triple corner-sharing complexes on {001} (85%) and Ni occupying Mn vacancy sites (15%). In synthetic seawater (I=0.72m) at short durations, we observed an even larger fractionation (up to 4.0‰), although the fractionation was significantly smaller in longer duration experiments. EXAFS spectra for Ni in high ionic strength experiments are fit well with 65% of Ni in triple corner-sharing complexes and 35% in Mn vacancy sites. We hypothesize that competitive sorption on {001} by other cations drives Ni into Mn vacancy sites at a faster rate than observed at low ionic strength. We further speculate that the isotopic fractionation we observe is dominated by a kinetic effect that will continue to decrease over time and may even reverse once equilibrium is approached and nearly all sorbed Ni is occupying Mn sites within the birnessite structure.
[1] Peacock &. Sherman, 2007, Chem. Geol.; [2] Cameron & Vance 2014, GCA; [3] Gall et al., 2013, EPSL.