We prese
nt a first-pri
nciples computatio
nal study of the i
nteractio
n of a
n H atom with the (010) surface of forsterite (Mg
2SiO
4). Periodic DFT-GGA calcu
latio
ns (PBE) are carried out usi
ng the SIESTA code with core pseudopote
ntials a
nd TZP localized basis sets. Pote
ntial e
nergy cur
ves are determi
ned for the approach of the H atom toward differe
nt sites of the surface: atop,
near, or i
n betwee
n the O, Mg, a
nd Si atoms. A
n outer adsorptio
n well is fou
nd for all i
nvestigated sites; it is deepest (162 meV) at a so-called 鈥渄isp
laced Mg鈥揙 bridge鈥?positio
n. The bi
ndi
ng at
this well is of the 鈥渨eak chemisorptio
n鈥?鈥渟tro
ng physisorptio
n鈥?type. A
n i
nner stro
nger chemisorptio
n well (670 meV deep) exists exclusi
vely
near a
n O site but
not strictly atop. Depe
ndi
ng o
n the path, we fi
nd acti
vatio
n barriers (25鈥?70 meV high) agai
nst chemisorptio
n, the lowest of these occurs for the top O site. Ge
neral tre
nds of the computed i
nteractio
n e
nergies qualitati
vely agree with the QM/MM results of Gouma
ns et al. [
lass="ref" href="#cit11">Mon. Not. R. Astron. Soc.2009, 393, 1403], but adsorption binding energies and barrier heights differ significantly.