小行星
地质学
古近纪
钌
白垩纪
天体生物学
古生物学
同位素
地球科学
物理
化学
核物理学
生物化学
催化作用
作者
M. Fischer-Gödde,Jonas Tusch,Steven Goderis,Alessandro Bragagni,T. Mohr‐Westheide,Nils Meßling,Bo-Magnus Elfers,Birger Schmitz,W. U. Reimold,W. D. Maier,Philippe Claeys,Christian Koeberl,F. L. H. Tissot,Martin Bizzarro,Carsten Münker
出处
期刊:Science
[American Association for the Advancement of Science (AAAS)]
日期:2024-08-16
卷期号:385 (6710): 752-756
标识
DOI:10.1126/science.adk4868
摘要
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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