THE chemical, mineralogical and isotopic characteristics of deposits a
t the Cretaceous/Tertiary (K/T) boundary are suggestive of a large imp
act event, the prime candidate1 being the Chicxulub crater in Yucatan,
Mexico. Spinel-bearing spherules, which may be associated with such i
mpacts, have been reported2 at several K/T boundary sites worldwide, b
ut their origin is still uncertain. We have examined the spinel-bearin
g material recovered from K/T boundary deposits at site 577 in the Pac
ific Ocean3 and find two distinct populations of particles: spherules
with dendritic spinel textures dispersed throughout the grains and irr
egularly shaped fragments with spinels essentially confined to the rim
. The morphology and composition of the particles are characteristic o
f melted and partially melted meteoritic ablation debris, but their lo
cation is difficult to reconcile with an impact on the Yucatan peninsu
la, some 10,000 km away. We suggest instead that the spinel-bearing pa
rticles at site 577 are derived from the impact of a 2-km asteroid in
the Pacific Ocean, and that several accretionary events of this type a
re required to explain the global distribution of spinel-bearing spher
ules at the K/T boundary.