TY - JOUR
T1 - Ruthenium isotopes show the Chicxulub impactor was a carbonaceous-type asteroid
AU - Fischer-Gödde, Mario
AU - Tusch, Jonas
AU - Goderis, Steven
AU - Bragagni, Alessandro
AU - Mohr-Westheide, Tanja
AU - Messling, Nils
AU - Elfers, Bo-Magnus
AU - Schmitz, Birger
AU - Reimold, Wolf U.
AU - Maier, Wolfgang D.
AU - Claeys, Philippe
AU - Koeberl, Christian
AU - Tissot, François L. H.
AU - Bizzarro, Martin
AU - Münker, Carsten
PY - 2024
Y1 - 2024
N2 - 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.
AB - 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.
U2 - 10.1126/science.adk4868
DO - 10.1126/science.adk4868
M3 - Journal article
C2 - 39146402
AN - SCOPUS:85201502764
VL - 385
SP - 752
EP - 756
JO - Science
JF - Science
SN - 0036-8075
IS - 6710
ER -