Cretaceous-Paleogene extinctionK-Pg boundaryChicxulub cratermass extinctionasteroid impact

Cretaceous-Paleogene Extinction Event: The Catastrophe That Ended the Dinosaurs

Cretaceous-Paleogene Extinction Event: The Catastrophe That Ended the Dinosaurs Approximately 66 million years ago, Earth experienced one of the most dramatic biological upheavals in its ...

Cretaceous-Paleogene Extinction Event: The Catastrophe That Ended the Dinosaurs

Approximately 66 million years ago, Earth experienced one of the most dramatic biological upheavals in its history. The Cretaceous-Paleogene (K-Pg) extinction event marked the end of the Cretaceous period and the beginning of the Paleogene, resulting in the disappearance of roughly 75% of all species on the planet. While most famous for the demise of the non-avian dinosaurs, this event reshaped the entire global ecosystem, clearing the path for the rise of mammals.

The transition is recorded in the geological record as the K-Pg boundary, a distinct layer of sediment found worldwide that separates the Mesozoic Era from the Cenozoic Era.

ภาพประกอบบทความ
ภาพประกอบจากบทความต้นฉบับ

Key Facts

  • Timing: Occurred approximately 66 million years ago.
  • Primary Cause: A massive asteroid impact at the Chicxulub crater in Mexico.
  • Major Victims: Non-avian dinosaurs, pterosaurs, and many marine reptiles.
  • Environmental Impact: Triggered a global blackout and freezing temperatures (impact winter) lasting at least a decade.
  • Contributing Factors: Volcanic activity from the Deccan Traps and sea-level regression.

The Chicxulub Impact: A Global Catastrophe

The most widely accepted cause of the mass extinction is the collision of a massive asteroid, several kilometers in diameter, with the Yucatán Peninsula in present-day Mexico. This event created the Chicxulub crater, a ring-shaped structure approximately 180 km (112 mi) wide.

topographic diagram showing round geographic features
Radar topography reveals the 180 km (112 mi)-wide ring of the Chicxulub crater

The energy released by this impact was equivalent to several million nuclear weapons detonating simultaneously. Because the asteroid struck a sulfur-rich region of shallow tropical seas, it spewed hundreds of billions of tons of sulfur and dust into the atmosphere. This created a worldwide blackout, blocking sunlight and causing temperatures to plummet, which disrupted photosynthesis and collapsed food chains globally.

Artistic impression of the asteroid slamming into tropical, shallow seas of the sulfur-rich Yucatán Peninsula in what is today Southeast Mexico.[218] The aftermath of this immense asteroid collision, which occurred approximately 66 million years ago, is believed to have caused the mass extinction of non-avian dinosaurs and many other species on Earth.[218] The impact spewed hundreds of billions of tons of sulfur into the atmosphere, producing a worldwide blackout, and freezing temperatures which persisted for at least a decade.[218]
Artistic impression of the asteroid slamming into tropical, shallow seas of the sulfur-rich Yucatán Peninsula in what is today Southeast Mexico.[218] The aftermath of this immense asteroid collision, which occurred approximately 66 million years ago, is believed to have caused the mass extinction of non-avian dinosaurs and many other species on Earth.[218] The impact spewed hundreds of billions of tons of sulfur into the atmosphere, producing a worldwide blackout, and freezing temperatures which persisted for at least a decade.[218]

Evidence for the Impact

Scientists have identified several geological markers that prove the impact occurred. One of the most significant is the presence of shocked quartz—grains of quartz with a microscopic structure that only forms under extreme pressure—and sanidine spherules found in the boundary clays.

Luis, left, and his son Walter Alvarez, right, at the K-T boundary in Gubbio, Italy, 1981
Luis, left, and his son Walter Alvarez, right, at the K-T boundary in Gubbio, Italy, 1981

Additionally, the K-Pg boundary is often visible as an abrupt change in rock color, as seen in the Raton Basin of Colorado, where dark-colored Cretaceous rocks are topped by lighter-colored Paleogene sediments.

rock striations with dark light boundary and surveying rod
The K–Pg boundary exposure in Trinidad Lake State Park, in the Raton Basin of Colorado, shows an abrupt change from dark- to light-colored rock

Extinction Patterns and Survivors

The extinction was not uniform; it was highly selective. While some groups were completely wiped out, others survived due to their diet or habitat.

Terrestrial Life

The most notable losses were the non-avian dinosaurs and pterosaurs. On land, plant communities suffered devastating losses, evidenced by a "fern spike" in the fossil record, where ferns—which are often the first to recolonize devastated landscapes—dominated shortly after the event.

Tyrannosaurus skeleton in museum display
Tyrannosaurus was among the dinosaurs living on Earth before the extinction

Mammals, birds, and crocodilians generally fared better. Many of these survivors were small, lived in burrows, or were detritus feeders (organisms that eat dead organic matter), which provided a buffer against the collapse of living plant populations.

Artist's rendering of a Thescelosaurus shortly after the K-Pg event
Artist's rendering of a Thescelosaurus shortly after the K-Pg event

Marine Life

The oceans experienced massive losses, particularly among the ammonites (coiled cephalopods) and rudist bivalves. Planktonic foraminifera and calcareous nannoplankton also saw severe declines, which crippled the marine food web from the bottom up.

spiral shell with embedded rock two centimeters across
Discoscaphites iris, an ammonite from the Owl Creek Formation (Upper Cretaceous), in Owl Creek near Ripley, Mississippi

bivalve shells seven centimeters across
Rudist bivalves from the Late Cretaceous of the Omani Mountains, United Arab Emirates. Scale bar is 10 mm.

Other Contributing Factors

While the Chicxulub impact was the primary trigger, researchers have investigated other stressors that may have weakened global ecosystems prior to the asteroid's arrival.

  • Deccan Traps: Massive volcanic eruptions in present-day India released vast amounts of carbon dioxide and sulfur, potentially causing climate instability.
  • Sea-Level Regression: A significant drop in sea levels during the Maastrichtian stage may have reduced shallow marine habitats.

Late Cretaceous global map (Turonian)
Late Cretaceous global map (Turonian)

Current scientific consensus suggests that while volcanism played a role, the asteroid impact was the decisive blow that caused the rapid mass extinction.

aerial view of the canyon with mesas and creek in background
Hell Creek Formation

Summary of the K-Pg Event

The following table summarizes the key aspects of the extinction event.

Overview of the Cretaceous-Paleogene Extinction Event
Feature Details
Approximate Date 66 Million Years Ago
Primary Driver Asteroid Impact (Chicxulub)
Key Geological Marker Iridium-rich K-Pg boundary layer
Major Extinctions Non-avian dinosaurs, Ammonites, Pterosaurs
Major Survivors Mammals, Birds, Crocodilians, Turtles
Climate Effect Impact Winter (Global cooling and darkness)

The river bed at the Moody Creek Mine, 7 Mile Creek / Waimatuku, Dunollie, New Zealand contains evidence of a devastating event on terrestrial plant communities at the Cretaceous–Paleogene boundary, confirming the severity and global nature of the event[163]
The river bed at the Moody Creek Mine, 7 Mile Creek / Waimatuku, Dunollie, New Zealand contains evidence of a devastating event on terrestrial plant communities at the Cretaceous–Paleogene boundary, confirming the severity and global nature of the event[163]

Frequently Asked Questions

Did all dinosaurs go extinct?

No. While non-avian dinosaurs were wiped out, avian dinosaurs—the ancestors of modern birds—survived the event.

What is the K-Pg boundary?

The K-Pg boundary is a thin layer of sediment found globally that marks the geological transition between the Cretaceous (K) and Paleogene (Pg) periods, characterized by high levels of iridium and shocked quartz.

How long did the "impact winter" last?

Evidence suggests that the freezing temperatures and worldwide blackout persisted for at least a decade following the collision.

Was the asteroid the only cause of the extinction?

While the asteroid is considered the primary cause, other factors such as the Deccan Traps volcanic eruptions and changing sea levels likely contributed to environmental stress.

Why did mammals survive when dinosaurs did not?

Many mammals were small, could burrow underground for protection, and had more flexible diets (such as eating detritus), making them less dependent on the immediate survival of living green plants.

References

  1. The abbreviation is derived from the juxtaposition of K, the common abbreviation for the Cretaceous, which in turn originates from the correspondent German term Kreide; and Pg, which is the abbreviation for the Paleogene.
  2. The former designation includes the term 'Tertiary' (abbreviated as T), which is now discouraged as a formal geochronological unit by the International Commission on Stratigraphy.[1]
  3. Shocked minerals have their internal structure deformed, and are created by intense pressures as in nuclear blasts and meteorite impacts.
  4. Ogg, James G.; Gradstein, F. M.; Gradstein, Felix M. (2004). A geologic time scale 2004. Cambridge, UK: Cambridge University Press. ISBN 978-0-521-78142-8.
  5. "International Chronostratigraphic Chart". stratigraphy.org. International Commission on Stratigraphy. 2015. Archived from the original on 30 May 2014. Retrieved 29 April 2015.