The interactions of Os-4, Os-5, and Os5C clusters with various sites of a M
gO(001) support were investigated theoretically with the aid of a scalar-re
lativistic density functional cluster model method. Adsorption geometries o
f C-4v clusters centered above a magnesium cation and the Os atoms oriented
either to the nearest surface oxygen anions (A) or between them (B) were c
onsidered. The influence of surface V-s and V-8(2-) defects on the adsorpti
on of the clusters was also investigated. The calculated base Os-Os distanc
es in supported Os-5 and Os5C square-pyramidal clusters are at most 0.1 Ang
strom longer (2.5-2.6 Angstrom) than the values calculated for the correspo
nding free osmium clusters but about 0.4 Angstrom (or more) shorter than th
e values determined by EXAFS spectroscopy for MgO-powder-supported clusters
formed by decarbonylation of [Os5C(CO)(14)](2-) and shown to retain the Os
5C frame. The experimental Os-Os distances characterizing the supported clu
sters are close to the experimental and calculated bond lengths for coordin
atively saturated osmium carbonyl clusters; this result favors the suggesti
on that the supported clusters characterized by EXAFS spectroscopy were not
entirely ligand-free. Calculated interaction strengths of the osmium clust
ers with the MgO(001) support range from nonbonding (defect-free site B whe
n the basal Os atoms are aligned between the nearest O anions) to very weak
(0.6 eV for Os5C at defect-free site A when the basal Os atoms are aligned
with the nearest O anions) to weak (similar to 2 eV for pure Os clusters a
t defect-free site A) to rather strong (similar to 9 eV for V-s defect site
A). The models reported here are inferred to be too simplified to capture
all the pertinent structural details of MgO-powder-supported osmium cluster
s, but they are sufficient to indicate a significant role of defect sites i
n the adsorption of supported osmium clusters and, we infer, other transiti
on metal clusters.