Ruthenium isotopes show the Chicxulub impactor was a carbonaceous-type asteroid

An impact at Chicxulub, Mexico, occurred 66 million years ago, producing a global stratigraphic layer that marks the boundary between the Cretaceous and Paleogene eras. That layer contains elevated concentrations of platinum-group elements, including ruthenium. We measured ruthenium isotopes in samples taken from three Cretaceous-Paleogene boundary sites, five other impacts that occurred between 36 million to 470 million years ago, and ancient 3.5-billion- to 3.2-billion-year-old impact spherule layers. Our data indicate that the Chicxulub impactor was a carbonaceous-type asteroid, which had formed beyond the orbit of Jupiter. The five other impact structures have isotopic signatures that are more consistent with siliceous-type asteroids, which formed closer to the Sun. The ancient spherule layer samples are consistent with impacts of carbonaceous-type asteroids during Earth's final stages of accretion.

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Publication Details

Journal
Science
Published
2024-08-15
DOI
https://doi.org/10.1126/science.adk4868
Citations
22
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
7.29
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article

Ruthenium isotopes show the Chicxulub impactor was a carbonaceous-type asteroid

Birger Schmitz, Alessandro Bragagni, François Tissot, Nils Meßling et al.
22 citations
Science
Astro and Planetary Science
7.29
article

Ruthenium isotopes show the Chicxulub impactor was a carbonaceous-type asteroid

Birger Schmitz, Alessandro Bragagni, François Tissot, Nils Meßling, Bo-Magnus Elfers, Philippe Claeys, Martin Bizzarro, Mario Fischer‐Gödde, Carsten Münker, W. D. Maier, Steven Goderis, Christian Koeberl, T. Mohr‐Westheide, W. U. Reimold, Jonas Tusch
article en
22 citations

Abstract

An impact at Chicxulub, Mexico, occurred 66 million years ago, producing a global stratigraphic layer that marks the boundary between the Cretaceous and Paleogene eras. That layer contains elevated concentrations of platinum-group elements, including ruthenium. We measured ruthenium isotopes in samples taken from three Cretaceous-Paleogene boundary sites, five other impacts that occurred between 36 million to 470 million years ago, and ancient 3.5-billion- to 3.2-billion-year-old impact spherule layers. Our data indicate that the Chicxulub impactor was a carbonaceous-type asteroid, which had formed beyond the orbit of Jupiter. The five other impact structures have isotopic signatures that are more consistent with siliceous-type asteroids, which formed closer to the Sun. The ancient spherule layer samples are consistent with impacts of carbonaceous-type asteroids during Earth's final stages of accretion.

ScienceVol. 385(6710)
California Institute of Technology (US), University of Copenhagen (DK), University of Vienna (AT), Museum für Naturkunde (DE), Vrije Universiteit Brussel (BE), University of Cologne (DE), Lund University (SE), Istituto di Scienze Marine del Consiglio Nazionale delle Ricerche (IT), Instituto de Geociencias (ES), National Research Council (IT), University of Florence (IT), University of Göttingen (DE), Cardiff University (GB), Hamburg University of Technology (DE)
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Openalex Percentile: Top 2%
Astro and Planetary Science
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