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An asteroid breakup 160 Myr ago as the probable source of the K/T impactor

Author

Listed:
  • William F. Bottke

    (Southwest Research Institute, 1050 Walnut St, Suite 300, Boulder, Colorado 80302, USA)

  • David Vokrouhlický

    (Southwest Research Institute, 1050 Walnut St, Suite 300, Boulder, Colorado 80302, USA
    Institute of Astronomy, Charles University, V Holešovičkách 2, 18000 Prague 8, Czech Republic)

  • David Nesvorný

    (Southwest Research Institute, 1050 Walnut St, Suite 300, Boulder, Colorado 80302, USA)

Abstract

The terrestrial and lunar cratering rate is often assumed to have been nearly constant over the past 3 Gyr. Different lines of evidence, however, suggest that the impact flux from kilometre-sized bodies increased by at least a factor of two over the long-term average during the past ∼100 Myr. Here we argue that this apparent surge was triggered by the catastrophic disruption of the parent body of the asteroid Baptistina, which we infer was a ∼170-km-diameter body (carbonaceous-chondrite-like) that broke up Myr ago in the inner main asteroid belt. Fragments produced by the collision were slowly delivered by dynamical processes to orbits where they could strike the terrestrial planets. We find that this asteroid shower is the most likely source (>90 per cent probability) of the Chicxulub impactor that produced the Cretaceous/Tertiary (K/T) mass extinction event 65 Myr ago.

Suggested Citation

  • William F. Bottke & David Vokrouhlický & David Nesvorný, 2007. "An asteroid breakup 160 Myr ago as the probable source of the K/T impactor," Nature, Nature, vol. 449(7158), pages 48-53, September.
  • Handle: RePEc:nat:nature:v:449:y:2007:i:7158:d:10.1038_nature06070
    DOI: 10.1038/nature06070
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