The Chicxulub Impact Produced a Powerful Global Tsunami
The Chicxulub crater is the site of an asteroid impact linked with the
Cretaceous-Paleogene (K-Pg) mass extinction at ∼66 Ma. This asteroid
struck in shallow water and caused a large tsunami. Here we present the
first global simulation of the Chicxulub impact tsunami from initial
contact of the projectile to global propagation. We use a hydrocode to
model the displacement of water, sediment, and crust over the first
10 min, and a shallow-water ocean model from that point onwards. The
impact tsunami was up to 30,000 times more energetic than the 26
December 2004 Indian Ocean tsunami, one of the largest tsunamis in the
modern record. Flow velocities exceeded 20 cm/s along shorelines
worldwide, as well as in open-ocean regions in the North Atlantic,
equatorial South Atlantic, southern Pacific and the Central American
Seaway, and therefore likely scoured the seafloor and disturbed
sediments over 10,000 km from the impact origin. The distribution of
erosion and hiatuses in the uppermost Cretaceous marine sediments are
consistent with model results.












kreuzaderny