W. Kee Leong, Y. Liu / Journal of Organometallic Chemistry 584 (1999) 174–178
175
The molecular structures of both 1b and 1c are
shown in Fig. 3, and selected bond parameters are
collected in Table 1. The X-ray crystal structure of 1c
reported here represents the first direct confirmation for
structural type C. In 1c, the Os(1)–Os(2) and Os(2)–
Os(3) bond lengths are much longer (0.0194 and 0.0170
This observation may be rationalised if we consider the
steric interactions involving the PPh3 ligands (Fig. 4).
In 1b, the steric effects of both PPh3 ligands impinge on
Os(3), while in 1c this is not the case. It may thus be
expected that 1b will have a greater tendency to distort
towards the S conformation in order to relieve the
strain, while the steric effects are ‘relayed’ round the
equatorial plane in 1c; the latter is evident in the bond
angles about the equatorial plane for Os(3), which show
that the equatorial carbonyls (CO(32) and CO(34)) are
bent away from Os(2) and towards Os(1).
If our discussions above were correct, then it would
appear that the relative orientation of ligands on clus-
ters can have very significant effects on both the gross
ligand sphere structure of the cluster as well as its
chemistry. For instance, we may expect that an
Os3(CO)10(PR3)2 cluster which exists in solution solely
as the B form will undergo halogenation less fa-
vourably; this is currently under investigation.
,
A, respectively) than the Os(1)–Os(3) bond, consistent
with the observation that a PR3 ligand tends to
lengthen the cis Os–Os bond [5,6]; the longer Os(1)–
Os(2) bond may be the consequence of a combination
of steric repulsions between CO(22) with P(1) and P(2),
which is also reflected in the Os(1)–P(1) bond being
longer than the Os(2)–P(2) bond by a 10| difference
(|=e.s.d.), as compared with a 5| difference for the
two Os–P bond lengths in 1b. It is also noteworthy that
the Os(1)–Os(2) bond length in 1c is the longest
,
at 2.9204(3) A; this is consistent with our earlier
suggestion that in the bromination reaction of
Os3(CO)10(PPh3)2, the isomer 1c is the one that under-
goes bromination and it involves cleavage of this bond
[4]. The most significant structural difference between
1b and 1c, however, is the greater degree of twisting of
the Os(CO)3(PPh3) units with respect to the Os(CO)4
unit in the former (Table 1).
2. Experimental
All reactions and manipulations were carried out
under nitrogen by using standard Schlenk techniques.
Infrared spectra were recorded as KBr disks. 31P-NMR
spectra were recorded on a Bruker ACF-300 FT-NMR
spectrometer and referenced to 85% aqueous H3PO4.
Microanalyses were carried out by the microanalytical
laboratory at the National University of Singapore.
In a recent exhaustive study on Os3(CO)11(PR3) clus-
ters, Pomeroy et al. have found that the nature of the
PR3 ligand can have profound structural implications
[6]. Essentially, their argument was that a better donor
PR3 ligand increases electron density at the Os atom of
the Os(CO)3(PR3) unit, leading to expansion of its filled
5d orbitals. This in turn causes an increase in repulsive
interaction with filled 5d orbitals on the other Os atoms
and hence a reduction in the bonding contribution of
the edge-bridging MOs. Steric effects from the PR3
ligand will then lead to lengthening of the cis Os–Os
bond as well as a propensity towards greater twisting of
the Os(CO)3(PR3) group, i.e. the adoption of what
Pomeroy et al. termed the S conformation, in order to
alleviate the 5d orbitals repulsive interaction.
Cluster
1 was prepared from the reaction of
Os3(CO)10(CH3CN)2 with two equivalents of PPh3.
Crystallisation from hexane/dichloromethane solution
gave a mixture of red crystals (1b) (Found: C, 39.86; H,
2.12. Calc. for C46H30O10Os3P2: C, 40.17; H, 2.18) and
yellow crystals (1c) (Found: C, 39.99; H, 2.14).
2.1. Crystal data for 1b
C46H30O10Os3P2, M=1375.24, monoclinic, space
From the electronic viewpoint, 1b and 1c should have
the same degree of expansion of the 5d orbitals at both
the Os(CO)3(PPh3) units. As measured by the Cax–Os–
Os–Cax torsion angles (Table 1), there is much less
twisting or distortion towards the S conformation in 1c.
group P21/n, a=14.8216(2), b=34.4785(2), c=
3
,
,
17.1059(3) A, i=92.373(1)°; U=8734.1(2) A ; Z=8;
zc=2.092 Mg m−3; v(Mo–Ka)=8.838 mm−1, T=
295 K, 56 987 reflections collected, 21 737 unique reflec-
tions, final R=11.13%, wR=8.44% for all data, 1106
parameters and three restraints.
2.2. Crystal data for 1c
C46H30O10Os3P2, M=1375.24, triclinic, space group
(
,
P1, a=12.5013(5), b=13.0248(5), c=14.2326(5) A,
h=71.784(1), i=79.384(1), k=89.220(1)°; U=
2161.23(14) A ; Z=2; zc=2.113 Mg m−3; v(Mo–
3
,
Ka)=8.929 mm−1
, T=295 K, 18 290 reflections
collected, 10 275 unique reflections, final R=4.11%,
wR=7.58% for all data and 550 parameters.
Fig. 1. Possible isomers for eq,eq-Os3(CO)10(PR3)2.