Rhenium (Re)-osmium (Os) isotope and elemental data have been obtained for
coexisting silicates and sulphide from a spinel-lherzolite from Kilbourne H
ole, New Mexico. These results confirm that sulphide dominates the Os budge
t in mantle rocks, but a significant proportion of the Re is located in the
silicates. The silicates and interstitial sulphide yield indistinguishable
Os isotope compositions suggesting these phases were in equilibrium at the
time of xenolith eruption. However, sulphide inclusions in silicate minera
ls presence significantly less radiogenic Os isotope compositions, suggesti
ng that they have been shielded from reaction or diffusion by their silicat
e hosts. Diffusion rates in silicates and sulphides are likely to be rapid
at mantle temperatures. However, for the sulphide inclusions diffusion thro
ugh the silicate host is likely to be impaired by the high partition coeffi
cient for Os between sulphide and silicate phases, in the range of 10(4) to
10(6). Consequently, sulphide inclusions trapped in silicates may be unabl
e to equilibrate either with other minerals or with an intergranular melt,
and in principle may preserve significantly older Re-Os age information tha
n coexisting phases. (C) 1999 Elsevier Science B.V. All rights reserved.