Impact event

Lore & Background

Impact events have been found to regularly occur in planetary systems, though the most frequent involve asteroids, comets or meteoroids and have minimal effect. When large objects impact terrestrial planets such as the Earth, there can be significant physical and biospheric consequences, as the impacting body is usually traveling at several kilometres per second. The minimum impact speed for bodies striking Earth is 11.2 km/s, the escape velocity of Earth. While planetary atmospheres can mitigate some impacts through atmospheric entry, many large bodies retain sufficient energy to reach the surface and cause substantial damage, forming impact craters and structures that shape the dominant landforms across solid objects in the Solar System. Major impact events have significantly shaped Earth's history, including the hypothesized formation of the Earth–Moon system via a giant impact, the origin of water on Earth, and several mass extinctions. The prehistoric Chicxulub impact, 66 million years ago, is believed to be the cause of the Cretaceous–Paleogene extinction event and accelerated the evolution of mammals. Throughout recorded history, hundreds of Earth impacts have been reported, with some causing deaths, injuries, or property damage.

Reader's Guide

Impact events are fundamental to understanding the evolution of the Solar System and life on Earth. They have been implicated in the formation of the Earth–Moon system, the delivery of water and building blocks for life, and several mass extinctions, including the Cretaceous–Paleogene extinction event 66 million years ago. The prevalence of impact craters across solid Solar System objects provides the strongest empirical evidence of the frequency and scale of these events. The energy released depends on the impactor's diameter, density, velocity, and angle, with the minimum impact velocity on Earth being 11.2 km/s and the most probable impact angle being 45 degrees. The B612 Foundation has stated it is 100 percent certain Earth will be hit by a devastating asteroid, though the timing is uncertain, and the US National Science and Technology Council has warned that America is unprepared for such an event.

Did You Know?

• The minimum impact speed for bodies striking Earth is 11.2 km/s, the escape velocity of Earth.
• The prehistoric Chicxulub impact, 66 million years ago, is believed to have caused the Cretaceous–Paleogene extinction event and accelerated the evolution of mammals.

The Physics of Collision

When an astronomical body strikes a terrestrial planet, the resulting destruction is governed by a handful of physical parameters. The minimum velocity at which any object can reach Earth's surface is 11.2 kilometres per second, dictated by the planet's escape velocity. In practice, most asteroid impacts average closer to seventeen kilometres per second, and the most probable angle of entry is roughly forty-five degrees. Together with the object's diameter, density, and trajectory, these variables dictate how much kinetic energy is deposited at the point of contact. Although Earth's atmosphere acts as a partial shield, shredding smaller bodies during entry, sufficiently large impactors retain enough energy to strike the ground with devastating force. The result is the creation of impact craters and complex structures that, across the solid bodies of the Solar System, constitute the dominant landforms. Their sheer prevalence remains the strongest empirical evidence for how frequently and violently these collisions have shaped the cosmos. Frequency follows a clear inverse relationship with size: a one-kilometre asteroid strikes Earth roughly once every half million years, while a five-kilometre object arrives approximately once every twenty million years. The last known impact of a body ten kilometres or larger was the Chicxulub event sixty-six million years ago.

Sculpting the Solar System and Life

Since the Solar System first coalesced, impact events have played a defining role in its evolution. The very formation of the Earth–Moon system is hypothesized to be the product of a single colossal collision, while the unusual retrograde rotation of both Uranus and Venus has been attributed to interplanetary impacts. Early in the history of the Earth–Moon system, a period known as the Late Heavy Bombardment would have subjected the young planet to an intense barrage of strikes. Beyond reshaping planetary geology, impacts appear to have been instrumental in the evolutionary history of life itself. They may have delivered the molecular building blocks necessary for biology to take root, a premise central to the panspermia theory. Impacts have also been proposed as the original source of water on Earth. On the other hand, they have been implicated in several mass extinction events. The most consequential of these, the Chicxulub impact sixty-six million years ago, is believed to have triggered the Cretaceous–Paleogene extinction. Paradoxically, by clearing the ecological stage, that catastrophe accelerated the evolution of mammals toward dominance and ultimately set in motion the conditions that allowed humans to rise.

Witnessed Collisions in the Modern Era

Throughout recorded history, hundreds of Earth impacts and exploding bolides have been documented, some causing deaths, injuries, and significant property damage. Beyond our own planet, humanity has witnessed collisions firsthand. In July 1994, the Comet Shoemaker–Levy 9 broke apart and slammed into Jupiter, providing the first direct observation of an extraterrestrial collision between Solar System objects. These dramatic events have also left a mark on popular culture, with impact scenarios serving as a recurring plot and background element in science fiction for decades.

Preparing for the Inevitable

In April 2018, the B612 Foundation issued a stark warning: it is certain that a devastating asteroid will eventually strike Earth, though the timing remains unknown. That same year, physicist Stephen Hawking, in his final book Brief Answers to the Big Questions, identified an asteroid collision as the single greatest threat to the planet. The urgency of the issue was underscored in June 2018 when the US National Science and Technology Council cautioned that America was unprepared for such an event, prompting the release of the National Near-Earth Object Preparedness Strategy Action Plan. The logistical challenge is considerable. Progress, however, has been made. The experiment was considered highly successful, altering the orbital period of the target body by thirty-two minutes—far exceeding the success criterion of a change greater than seventy-three seconds.