Dark primitive asteroids account for a large share of K/Pg-scale impacts on the Earth

Abstract A dynamical model for large near-Earth asteroids (NEAs) is developed here to understand the occurrence rate and nature of Cretaceous–Paleogene (K/Pg) scale impacts on the Earth. We find that 16–32 (2–4) impacts of diameter D > 5 km ( D > 10 km) NEAs are expected on the Earth in 1 Gyr, with about a half of impactors being dark primitive asteroids (most of which start with semimajor axis a > 2 . 5 au). These results explain why the Chicxulub crater, the third largest impact structure found on the Earth (diameter ≃ 180 km), was produced by impact of a carbonaceous chondrite. They suggest, when combined with previously published results for small ( D ≲ 1 km) NEAs, a size-dependent sampling of the main belt. We conclude that the impactor that triggered the K/Pg mass extinction ≃ 66 Myr ago was a main belt asteroid that quite likely ( ≃ 60 % probability) originated beyond 2.5 au.