An international team of researchers led by scientists from the Vrije Universiteit Brussel has traced the global asteroid dust layer to within the Chicxulub impact crater in Mexico. “We have finally come full circle,” says Steven Goderis, a lecturer in geochemistry at VUB and lead author of the study. The amount of iridium found indicates that this must have been the epicentre of the space dust found around the world. Iridium is a silvery-white metal that is not very common on Earth, but was present in significant quantities in the meteorite.
In May 2016, drilling was done at the centre of the Chicxulub crater. Approximately 835 metres of rock was brought to the surface, which has provided a tremendous amount of new information about the impact and the period that followed. Based on an extensive geochemical analysis of the drill core, these high concentrations of iridium were found.
Goderis: “It is remarkable that we have found such high concentrations in the impact crater itself. In the first hours to months after impact, the crater was a very turbulent environment affected by tsunamis, oscillating waves and earthquakes. After circling in the atmosphere around the Earth for several years, the deposition of the iridium-rich dust released on impact may have lasted for several decades after the impact.”
Rapid precipitation of crater dust
The atmospheric precipitation of this asteroid dust thus imposes important time limits on the deposition of the crater rock just below this iridium layer. “This part of the crater returned to a relatively low-energy environment in a much shorter time than previously expected. The iridium layer reflects the timing of the recovery of life during the years to millennia after impact, indicating a very complex biological response to the rapidly changing environment at ‘ground zero’,” says Sean Gulick, research professor at the University of Texas at Austin and co-principal scientist of the drilling expedition. This means that life returned much faster than expected.
In addition to the Vrije Universiteit Brussel, the following universities and institutes are involved in the study: University of Padua, Japan Agency for Marine-Earth Science and Technology, Natural History Museum in Vienna, Lund University, University of Notre Dame, Université Libre de Bruxelles, KU Leuven, Arizona State University, University of Vienna, Universität zu Köln, University of Ghent, Utrecht University, Tokyo Institute of Technology, Florida State University, HNU Neu-Ulm University of Applied Sciences, Lunar and Planetary Institute, Durham University, Pennsylvania State University, University of Texas at Austin, Imperial College London, Vrije Universiteit Amsterdam and University of Alaska Fairbanks.
The study was published in the journal Science Advances.
S. Goderis, H. Sato, L. Ferrière, B. Schmitz, D. Burney, P. Kaskes, J. Vellekoop, A. Wittmann, T. Schulz, S. M. Chernonozhkin, P. Claeys, S. J. de Graaff, T. Déhais, N. J. de Winter, M. Elfman, J.-G. Feignon, A. Ishikawa, C. Koeberl, P. Kristiansson, C. R. Neal, J. D. Owens, M. Schmieder, M. Sinnesael, F. Vanhaecke, S. J. M. Van Malderen, T. J. Bralower, S. P. S. Gulick, D. A. Kring, C. M. Lowery, J. V. Morgan, J. Smit, M. T. Whalen, IODP-ICDP Expeditie 364 Wetenschappers, Globally distributed iridium layer preserved within the Chicxulub impact structure. Sci. Adv. 7, eabe3647 (2021).
Steven Goderis, [email protected], 0473-98 29 17