Also known as K-Pg mass extinction, Cretaceous-Paleogene extinction, Cretaceous-Paleogene mass extinction event, Cretaceous-Paleogene extinction event, end-Cretaceous extinction event, end-Cretaceous mass extinction event, end-Cretaceous extinction, end-Cretaceous mass extinction
extinction event ending the Mesozoic Era
The Cretaceous-Paleogene mass extinction was a catastrophic extinction event that ended the Mesozoic Era, eliminating most life on Earth including the dinosaurs. It matters because it was one of the most significant turning points in Earth's history, allowing mammals and other surviving species to diversify and eventually lead to the world we see today.
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The Cretaceous–Paleogene (K–Pg) extinction event, formerly known as the Cretaceous-Tertiary (K–T) extinction event, was a major mass extinction of three-quarters of the plant and animal species on Earth which occurred around 66 million years ago. The event caused the extinction of all of the non-avian dinosaurs and most other tetrapods weighing more than 25 kg (55 lb), with the exception of some ectothermic species such as sea turtles and crocodilians. It marked the end of the Cretaceous period, and with it the Mesozoic era, while heralding the beginning of the next and current geological era, the Cenozoic Era. In the geologic record, the K–Pg event is marked by a thin layer of sediment called the K–Pg boundary or K–T boundary, which can be found throughout the world in marine and terrestrial rocks. The boundary clay shows unusually high levels of the metal iridium, which is more common in asteroids than in the Earth's crust.
It is now generally thought that the K–Pg extinction resulted from the impact of a massive asteroid 10 to 15 km (6 to 9 mi) wide, creating the Chicxulub impact crater and devastating the global environment around 66.043 million years ago, primarily through a lingering impact winter which halted photosynthesis in plants and plankton. The impact hypothesis, also known as the Alvarez hypothesis, was bolstered by the discovery of the 180 km (112 mi) Chicxulub crater in the Gulf of Mexico's Yucatán Peninsula in the early 1990s. The timing of the ejecta layer, together with the match between fossil‑record ecological patterns and modeled environmental disruptions (such as darkness and cooling), supports the conclusion that the Chicxulub impact triggered the mass extinction. A 2016 drilling project into the Chicxulub peak ring confirmed that the peak ring contained granite ejected within minutes from deep in the Earth, but contained hardly any gypsum, the usual sulfate-containing sea floor rock in the region. The gypsum would have vaporized and dispersed as an aerosol into the atmosphere, causing longer-term effects on the climate and food chain. In October 2019, researchers proposed a mechanism of the mass extinction, arguing that the Chicxulub asteroid impact event rapidly acidified the oceans and produced long-lasting effects on the climate.
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