Polycrystalline diamonds (framesites) from the Venetia kimberlite in South
Africa contain silicate minerals whose isotopic and trace element character
istics document remobilization of older carbon and silicate components to f
orm the framesites shortly before kimberlite eruption. Chemical variations
within the garnets correlate with carbon isotopes in the diamonds, indicati
ng contemporaneous formation. Trace element, radiogenic, and stable isotope
variations can be explained by the interaction of eclogites with a carbona
titic melt, derived by remobilization of material that had been stored for
a considerable time in the lithosphere, These results indicate more recent
formation of diamonds from older materials within the cratonic lithosphere.