Some reactions of the octahalodirhenate(III) ions. V. Polarographic

V. Polarographic reduction. F. Albert Cotton, William R. Robinson, and Richard A. Walton. Inorg. Chem. , 1967, 6 (6), pp 1257–1258. DOI: 10.1021/ic5...
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Vol. 6 , No. 6, June 1967

NOTES 1257

ligands containing phosphorus, and i t thus appears probable that “mixed” ligands containing both phosphorus and sulfur would yield much the same results as have been reported above. Acknowledgment.-The support of this research by the Petroleum Research Fund, administered by the American Chemical Society, is gratefully acknowledged.

-1.0 VOLTS vs SCE

0 DEPARTMENT OF CHEMISTRY, MASSACHUSETTS INSTITUTE O F TECHNOLOGY, CAMBRIDGE, MASSACHUSETTS 02139

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Some Reactions of the Octahalodirhenate(II1) Ions. V. Polarographic Reduction’ BY F. A . COTTON, W. R. ROBINSON, AND R. A. WALTON Received December 30,1966

Relatively few studies of the redox reactions of metal atom cluster compounds have been p ~ b l i s h e d . ~In ,~ those reported, the results (for M&z species) have been remarkably consistent with the molecular orbital description of the bonding given by Cotton and Haas4 for such systems. A comparable sort of MO analysis of the b ~ n d i n g has ~ . ~been carried out for the RezXS2species (X = C1, Br, and most recently,’ NCS) which have D i h symmetry. This treatment, which should also be applicable in its general features to any analogous technetium complexes, leads to the conclusion that there are two relatively low-lying, nonbonding o orbitals which are directed outward along the fourfold axis of the molecule. It would seem reasonable to suppose that a t least one and perhaps two electrons could be added to these orbitals, thus forming RezXs3- and RezXs4- species, without interfering with any of the components, U, K , or 6, of the Re-Re bond. Hence, the extremely short metal-metal distance and the eclipsed configuration should be maintained in the reduced species. Whether the RezXs4- species should have zero or two unpaired electrons will depend on how nearly degenerate the two nonbonding o orbitals are; this is difficult to predict with confidence. The investigations described here were undertaken to test the foregoing ideas. The results are also rele-

(1) Keiearch supported in part by t h e United States Atomic Energy Commission. (2) R. E. McCarley, B. G . Hughes, F. A. Cotton, a n d R Zimmerman, Inorg. Chem., 4, 1491 (1965). (3) R. A. Mackay a n d R. F. Schneider, ibid.,6, 549 (1967). (4) F. A. Cotton and T. E. Haas, ibid., S, 10 (1964). (5) F. A. Cotton, ibid., 4, 334 (1965). ( 6 ) F. A. Cotton and C. B. Harris, i b i d . , 6, 924 (1967) (7) P a r t I V of this series: F. A. Cotton, W. R. Robinson, I