Diamonds were found in impact melt rocks and breccias at the Popigai i
mpact structure in Siberia. The diamonds preserve the crystallographic
habit and twinning of graphites in the preimpact target rocks, from w
hich they formed by shock transformation. Secondary and transmission e
lectron microscopy indicate that the samples are polycrystalline and c
ontain abundant very thin lamellae, which could represent stacking fau
lts, with local hexagonal symmetry, or microtwins. Microcrystalline un
its are less than or equal to 1 mu m. Infrared spectroscopy indicates
the presence of solid CO2 and water in microinclusions in the diamonds
, CO2 being under a pressure greater than 5 GPa (at room temperature).
Trace element and isotopic compositions confirm the derivation from g
raphite precursors.