The study of Re-187-Os-187 systematics in the orogenic lherzolite bodi
es of Baldissero, Beni Bousera, Lanzo and Lherz shows the extreme isot
opic heterogeneity of these massifs. Peridotites have Os-187/Os-186 ra
tios that cluster around the primitive mantle value (1.05-1.06) while
pyroxenites have extremely radiogenic Os-187/Os-186 ratios (from 1.78
to 8.9). These isotopic variations recorded by a single pyroxenite dem
onstrate that osmium is heterogeneously distributed on a very small sc
ale. The Os-187/Os-186 ratios of peridotites are comparable to those m
easured on abyssal peridotites, which suggests that they represent a M
ORB source type of mantle. The radiogenic Os-187/Os-186 ratios of pyro
xenites suggest that they are melts or cumulates formed similar to 1 G
a ago and that they they may represent old delaminated oceanic crust.
The preferential melting of pyroxenites durign the formation of oceani
c basalts may account for some of the radiogenic Os-187/Os-186 ratios
encountered in MORBs and OIBs.