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Impact event

Collisions between astronomical objects that shape planets and life.

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An impact event occurs when two astronomical objects collide, producing effects that can be measured. Such collisions happen regularly in planetary systems, but most involve small asteroids, comets, or meteoroids and cause little damage. When a large object strikes a rocky planet like Earth, however, the consequences can be severe for both the landscape and life, because the impacting body typically travels at several kilometers per second. The slowest possible speed for an object hitting Earth is 11.2 km/s—the planet’s escape velocity.

Impacts and the Earth

Although a planet’s atmosphere can reduce some of this energy during entry, many large bodies still have enough force to reach the ground and inflict major harm. These strikes create impact craters and structures, which are the dominant landforms on many solid bodies across the Solar System. The sheer number and widespread presence of these craters offer the strongest evidence of how often and how powerfully such events occur.

Impact events appear to have shaped the Solar System’s evolution since its beginning. Major collisions have significantly influenced Earth’s history; for instance, the formation of the Earth–Moon system is thought to have resulted from a giant impact. Similar interplanetary crashes have been proposed to explain why Uranus and Venus rotate backward. Impacts also seem to have played a key role in the history of life.

They may have delivered the raw ingredients for life—a core idea behind the panspermia theory—and have been suggested as the source of Earth’s water. Additionally, impacts are linked to several mass extinctions. The prehistoric Chicxulub impact 66 million years ago is believed to have caused the Cretaceous–Paleogene extinction event and also accelerated the evolution of mammals, leading to their dominance and eventually setting the stage for humans.

Over recorded history, hundreds of Earth impacts and exploding bolides have been reported, some causing deaths, injuries, property damage, or other significant local effects. One of the most famous modern events is the 1908 Tunguska event in a remote part of Siberia, Russia. The 2013 Chelyabinsk meteor event is the only known modern incident to result in numerous injuries, and its meteor is the largest recorded object to hit Earth since Tunguska.

The Comet Shoemaker–Levy 9 impact in July 1994 provided the first direct observation of an extraterrestrial collision in the Solar System, when the comet broke apart and struck Jupiter. In 2013, an extrasolar impact was observed around the star ID8 in the cluster NGC 2547 by NASA’s Spitzer Space Telescope and confirmed from the ground. Impact events also appear as plot elements in science fiction.

Current response status

In April 2018, the B612 Foundation stated, “It’s 100 percent certain we’ll be hit [by a devastating asteroid], but we’re not 100 percent certain when.” That same year, physicist Stephen Hawking wrote in his final book that an asteroid collision was the biggest threat to the planet. In June 2018, the US National Science and Technology Council warned that America is unprepared for an asteroid impact and released a “National Near-Earth Object Preparedness Strategy Action Plan.” According to 2013 testimony before the US Congress, NASA would need at least five years of preparation before launching a mission to intercept an asteroid. On 26 September 2022, the Double Asteroid Redirection Test successfully demonstrated asteroid deflection—the first such experiment by humanity—changing the target body’s orbital period by 32 minutes, well beyond the 73-second threshold for success.

Several major impacts have shaped Earth’s history, linked to the formation of the Earth–Moon system, the evolution of life, the origin of Earth’s water, and multiple mass extinctions. Impact structures, as the dominant landforms on many solid Solar System objects, provide the strongest evidence of prehistoric events. Notable examples include the hypothesized Late Heavy Bombardment early in the Earth–Moon system’s history and the confirmed Chicxulub impact 66 million years ago, which caused the Cretaceous–Paleogene extinction.

Frequency and risk

Small objects hit Earth frequently. There is an inverse relationship between an object’s size and how often it strikes. The lunar crater record shows that impact frequency decreases roughly as the cube of the resulting crater’s diameter, which is on average proportional to the impactor’s diameter. Asteroids about 1 km in diameter hit Earth every 500,000 years on average.

Larger collisions—with objects around 5 km—occur roughly once every 20 million years. The last known impact of an object 10 km or more in diameter was the Cretaceous–Paleogene event 66 million years ago. The energy released depends on the impactor’s diameter, density, velocity, and angle. For most near-Earth asteroids not studied by radar or infrared, diameter is estimated within a factor of two based on brightness, and density is generally assumed.

Lore & Background

Impact events appear to have played a significant role in the evolution of the Solar System since its formation. Major impact events have significantly shaped Earth's history, and the formation of the Earth–Moon system has been hypothesized to be the result of a giant impact. Interplanetary impacts have also been proposed to explain the retrograde rotation of Uranus and Venus. Impact events also appear to have played a significant role in the evolutionary history of life.

Impacts may have helped deliver the building blocks for life (the panspermia theory relies on this premise). Impacts have been suggested as the origin of water on Earth. They have also been implicated in several mass extinctions. The prehistoric Chicxulub impact, 66 million years ago, is believed to be the cause not only of the Cretaceous–Paleogene extinction event but acceleration of the evolution of mammals, leading to their dominance and, in turn, setting in place conditions for the eventual rise of humans.

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.

Reader's Guide

Throughout recorded history, hundreds of Earth impacts (and exploding bolides) have been reported, with some occurrences causing deaths, injuries, property damage, or other significant localised consequences. One of the best-known events recorded in modern times was the Tunguska event, which occurred in 1908 in a very sparsely populated part of Siberia, Russia. The 2013 Chelyabinsk meteor event is the only known such incident in modern times to result in numerous injuries. Its meteor is the largest recorded object to have encountered the Earth since the Tunguska event.

The Comet Shoemaker–Levy 9 impact provided the first direct observation of an extraterrestrial collision of Solar System objects, when the comet broke apart and collided with Jupiter in July 1994. An extrasolar impact was observed in 2013, when a massive terrestrial planet impact was detected around the star ID8 in the star cluster NGC 2547 by NASA's Spitzer Space Telescope and confirmed by ground observations. Impact events have been a plot and background element in science fiction.

Frequently Asked Questions

What kinds of effects can a large impact event cause?

Small impacts involving meteoroids or minor asteroids typically produce negligible results, but a large strike on a terrestrial planet can trigger dramatic physical and biospheric consequences, including mass extinction-level disruption of the environment.

How have impact events shaped the Solar System's history?

Impact events are credited with playing a pivotal role in the Solar System's evolution, including the formation of the Earth–Moon system and the shaping of Earth's geological and biological history over billions of years.

What types of objects are most commonly involved in impact events?

The vast majority of impact events involve asteroids, comets, or meteoroids colliding with a larger body. While most of these encounters have minimal observable effect, the larger ones can leave lasting marks on planetary surfaces and ecosystems.

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Sources

Compiled from Wikipedia and the sources listed below. Text from Wikipedia is available under CC BY-SA 4.0; this entry is adapted from it.

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