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Chicxulub Impact Asteroid Likely Came from Rare Class of Primitive Meteorites

Researchers analyzing nickel isotopes in 66-million-year-old debris conclude the asteroid that wiped out the dinosaurs belonged to a rare class of carbonaceous chondrites known as CO chondrites.

New research suggests the asteroid that struck Earth 66 million years ago and triggered the mass extinction of the dinosaurs was an exceptionally rare type of space rock. Scientists analyzing nickel isotopes preserved in debris from the Chicxulub impact have concluded that the object most likely belonged to a class of primitive meteorites called carbonaceous chondrites of the Ornans type, or CO chondrites. The finding sheds new light on the nature of the impactor that reshaped life on Earth.

The study, published in a peer-reviewed journal, focuses on the chemical signature left behind in the global layer of sediment deposited after the impact. By measuring nickel isotope ratios in samples from the Cretaceous-Paleogene boundary — the geological layer marking the extinction event — researchers were able to distinguish between different types of meteoritic material. Nickel isotopes act as a fingerprint for the type of asteroid involved, because different classes of meteorites have distinct isotopic compositions.

CO chondrites are a rare subgroup of carbonaceous chondrites, which themselves make up only a small fraction of meteorites that fall to Earth. These primitive rocks are thought to contain some of the most ancient material in the Solar System, having remained largely unchanged since the formation of the planets. The new analysis indicates that the Chicxulub impactor was not a typical asteroid but an “oddball” object from a class that is seldom seen in the meteorite record.

The Chicxulub impact, centered on what is now the Yucatán Peninsula in Mexico, is widely accepted as the primary cause of the end-Cretaceous mass extinction that eliminated about three-quarters of Earth’s plant and animal species, including all non-avian dinosaurs. The collision released energy equivalent to billions of atomic bombs, triggering wildfires, tsunamis, and a prolonged period of darkness and cooling that disrupted ecosystems worldwide.

Previous studies had attempted to identify the type of asteroid responsible for the impact, with some suggesting it was a carbonaceous chondrite. However, the new nickel isotope data provides more precise evidence, narrowing the classification to the Ornans type. The researchers note that CO chondrites are distinguished by their small chondrules — spherical silicate inclusions — and their distinct chemical composition, which sets them apart from other carbonaceous chondrites.

The team analyzed samples from multiple sites around the world, including locations in Denmark, Italy, and New Zealand, to ensure the isotopic signature was consistent and not a local anomaly. The results showed a uniform nickel isotope anomaly across all sites, strongly supporting the conclusion that the impactor was a CO chondrite. This consistency also rules out the possibility that the anomaly came from terrestrial sources or volcanic activity.

Understanding the composition of the Chicxulub impactor has implications beyond geological history. It helps scientists model the frequency and effects of asteroid impacts on Earth and assess the potential risks posed by different types of near-Earth objects. If the dinosaur-killing asteroid came from a rare class of meteorites, it suggests that not all impactors pose the same threat, and that the specific composition of an asteroid influences the environmental consequences of a collision.

The research also adds to the broader effort to trace the origins of asteroids that have struck Earth. By comparing isotopic signatures from impact debris with those of known meteorite groups, scientists can build a more complete picture of the types of objects that have shaped our planet’s history. The Chicxulub impact remains the most recent large-scale extinction event, and its study continues to provide critical insights into the dynamics of the Solar System and the vulnerability of life on Earth.

The findings highlight the value of isotopic analysis in planetary science, offering a tool that can be applied to other impact events. Future studies may examine debris from other major impacts to determine whether they also involved rare types of asteroids or whether the Chicxulub event was unique in its choice of projectile. For now, the identification of the dinosaur-killing asteroid as a CO chondrite adds a new chapter to the story of Earth’s most famous cosmic collision.