Transition to the Paleogene Period
The transition from the Cretaceous to the Paleogene Period marks a significant milestone in the geological timeline of Earth. This transition is heralded by the Cretaceous–Paleogene (K–Pg) extinction event, a massive extinction event that occurred approximately 66 million years ago. This event led to the end of the Mesozoic Era and the beginning of the Cenozoic Era, signaling a dramatic reshaping of Earth's biodiversity and ecosystems.
Geological and Environmental Changes
The Cretaceous–Paleogene boundary is marked geologically by a thin layer of sedimentary rock rich in iridium, which is rare in Earth's crust but abundant in meteorites. This has led to the hypothesis that a large asteroid impact at the Chicxulub crater in the Yucatán Peninsula was a major factor in the extinction event. The aftermath of this impact likely caused global wildfires, a "nuclear winter" effect, and disrupted photosynthesis, leading to the collapse of food chains.
The climate across this boundary saw significant shifts. The Cretaceous had been characterized by a warm climate with high sea levels, but the impact event resulted in a rapid cooling known as the "impact winter." This was followed by a period of global warming as the Paleogene climate stabilized.
Biological Impact and Evolution
The mass extinction at the K–Pg boundary saw the disappearance of approximately 75% of all species, including the iconic non-avian dinosaurs. This loss of species created ecological niches that allowed mammals and other groups to diversify and proliferate, leading to the rise of modern mammals and eventually human evolution.
The Paleogene Period is divided into three epochs: the Paleocene, Eocene, and Oligocene. Each of these periods saw continued evolution and radiation of species. The Paleocene saw the recovery and diversification of life forms; the Eocene brought about the establishment of modern plant and animal families, and the Oligocene marked significant geological and climatic changes, including the establishment of polar ice caps.
Stratigraphy and Detection
The K–Pg boundary layer is detected in sediments worldwide, often as a thin layer of clay. Its unique composition, including high concentrations of iridium, shocked quartz, and tektites, provides evidence for the extraterrestrial impact hypothesis. This boundary is crucial for stratigraphic studies as it provides a distinct marker for the end of the Mesozoic and the onset of the Cenozoic.