Iridium concentrations in successively smaller subsplits of melt rock
and melt breccia from the Chicxulub impact basin were tracked to isola
te and identify iridium carrier phases. Iridium-rich particles were is
olated from two samples, and a micrometer-scale, silicate-enclosed agg
regate of subhedral iridium metal grains was identified in one, confir
ming earlier reports of iridium at ground zero of the impact at the Cr
etaceous-Tertiary (K-T) boundary. The aggregate may be either a phase
formed after the collision or a relict of the Chicxulub basin-forming
meteorite. In either case, its presence indicates that even among the
largest impact structures on Earth, meteoritic components may be prese
rved within the crater.