A family of compounds has been discovered in which
pairs of octahedral rare-earth-metal clusters, each
centered by a late transition metal Z, share a common edge. These
R10Z2 units, sheathed and interbridged by
iodine
atoms, occur in the quaternary phases
Rb2La10I17Co2,
Cs2La10I17Z2 (Z
= Co, Ni, Ru, Os),
Cs2Ce10I17Os2,
and
Cs2Pr10I17Z2 (Z
= Co, Ru, Os) and in the ternary
La10I15Os2. All are
obtained as black, air-sensitive crystals from
reactions of RI3, R, Z, and RbI or CsI as appropriate in
welded Nb containers at 800−850 °C. The
structure
of
Cs2Ce10I17Os2
has been refined by single-crystal X-ray diffraction methods for
comparison with the isotypic
Cs2La10I17Co2
(monoclinic, C2/m, Z = 2,
R(F)/R
w = 4.0/4.4%),
and the structure of a unique ternary
La10I15Os2 has
been defined (triclinic, P1̄, Z = 1,
R/R
w = 5.0/5.1%). These new bioctahedral
clusters may be regarded as the
missing links between discrete clusters and infinite chains of
condensed octahedral clusters among rare-earth-metal
cluster halides that are stabilized by interstitial transition metals.
The biclusters in both structures are extensively
interconnected into three-dimensional arrays through bridging iodine
atoms. The structural interconversion between
Cs2La10I17Os2
and La10I15Os2 + 2CsI may be
easily visualized in terms of changes in iodide bridging modes
and
accommodation of cesium cations. All the biclusters contain an odd
number of cluster-bonding electrons, and this
feature has been confirmed by magnetic susceptibility studies.
EHMO cluster and band calculations on biclusters
and their structures are in agreement with the localized bonding
properties and ranges of electron counts.