TY - JOUR
T1 - The bonding of ferrous iron to sulfur and oxygen in tetrahedral coordination
T2 - A comparative study using SCF Xα scattered wave molecular orbital calculations
AU - Vaughan, D. J.
AU - Tossell, J. A.
AU - Johnson, K. H.
N1 - Funding Information:
Ac~Zedgeme7ats--Prof. R. G. BURNS is thanked for his comments on the muscript and Mrs. V. M. BUNS for bibliographic assistance. The work was supported by NASA grant NGL 22-009-187 and by the National Science Foundation through the M.I.T. Center for Mate~a~ Science and Engineem.
PY - 1974/7
Y1 - 1974/7
N2 - Molecular quantum mechanical calculations have been performed on high-spin ferrous iron tetrahedrally coordinated to sulfur and oxygen, respectively. The molecular orbital energies obtained from the calculations are compared with experimental optical and X-ray emission spectra. Good agreement was found between calculated and experimental spectral transition energies for the optical absorption spectra of Fe2+ in sphalerite, of Fe2+ in FeAl2O4, staurolite and (Zn, Fe)O, and for the FeKβ X-ray emission spectra of FeCr2O4. This both clarified interpretation of the spectra and established the validity of the calculations. Distinct differences occur in the molecular orbital structures of the sulfide and oxide clusters. In the sulfide, the crystal field type (mainly Fe 3d) molecular orbitals lie within the nonbonding (mainly S 3p) orbitais in energy, whereas in the oxide, they lie well above the 02p nonbonding orbitals. This also results in a wider valence band in the oxide than in the sulfide. The crystal field type (Fe 3d) molecular orbitais have more ligand character in the sulfide than the oxide and the chalcophilic properties of iron are partly attributed to this observation.
AB - Molecular quantum mechanical calculations have been performed on high-spin ferrous iron tetrahedrally coordinated to sulfur and oxygen, respectively. The molecular orbital energies obtained from the calculations are compared with experimental optical and X-ray emission spectra. Good agreement was found between calculated and experimental spectral transition energies for the optical absorption spectra of Fe2+ in sphalerite, of Fe2+ in FeAl2O4, staurolite and (Zn, Fe)O, and for the FeKβ X-ray emission spectra of FeCr2O4. This both clarified interpretation of the spectra and established the validity of the calculations. Distinct differences occur in the molecular orbital structures of the sulfide and oxide clusters. In the sulfide, the crystal field type (mainly Fe 3d) molecular orbitals lie within the nonbonding (mainly S 3p) orbitais in energy, whereas in the oxide, they lie well above the 02p nonbonding orbitals. This also results in a wider valence band in the oxide than in the sulfide. The crystal field type (Fe 3d) molecular orbitais have more ligand character in the sulfide than the oxide and the chalcophilic properties of iron are partly attributed to this observation.
UR - http://www.scopus.com/inward/record.url?scp=4243902368&partnerID=8YFLogxK
U2 - 10.1016/0016-7037(74)90001-5
DO - 10.1016/0016-7037(74)90001-5
M3 - Article
AN - SCOPUS:4243902368
SN - 0016-7037
VL - 38
SP - 993
EP - 1005
JO - Geochimica Et Cosmochimica Acta
JF - Geochimica Et Cosmochimica Acta
IS - 7
ER -