Nepedia
Back to Discover
Advanced Reader
🚀

Impact event

space Maturity 9-11 Next article →

An impact event is a collision between astronomical objects in space. These collisions can involve asteroids, comets, or meteoroids. While many impacts are small and have minimal effects, larger ones can cause massive changes. When large bodies strike terrestrial planets like Earth, they carry immense energy. This energy comes from their high speed. Most impacts occur at several kilometers per second (km/s). The minimum speed for any object striking Earth is the planet's escape velocity.

Bolide
Bolide

The mechanism of an impact depends on the object's size and speed. As an object enters the atmosphere, the air can mitigate some of the energy. However, many large bodies retain enough energy to reach the surface. When they hit solid ground, they create impact craters. These craters are large structures that shape the landforms of the Solar System. Sometimes, an object does not reach the ground. Instead, it undergoes an airburst, which is an explosion in the atmosphere. The energy released depends on the object's diameter, density, velocity, and impact angle.

Chicxulub-animation
Chicxulub-animation

Impacts can be categorized by their size and how they release energy. Small objects, called meteoroids, frequently collide with Earth. Stony asteroids with a diameter of 10 to 20 meters enter our atmosphere about once a year. These often result in airbursts. For example, the 2013 Chelyabinsk meteor was about 20 meters wide. It produced an airburst 30 times more powerful than the atomic bomb dropped on Hiroshima. Larger objects, such as those with a diameter of 1 kilometer or more, are much rarer. Large collisions involving objects 10 kilometers wide happen only once every twenty million years on average.

Chelyabinsk meteor trace 15-02-2013
Chelyabinsk meteor trace 15-02-2013

Humans have documented many of these events throughout history. In 1908, the Tunguska event occurred in a remote part of Siberia, Russia. This massive explosion shattered windows hundreds of kilometers away and damaged many trees.

Tunguska Ereignis-1
Tunguska Ereignis-1

In 1994, the Comet Shoemaker–Levy 9 impact provided the first direct observation of a collision. We watched as the comet broke apart and hit Jupiter. Scientists like Eugene Shoemaker were vital to our understanding. He helped prove that meteorite impacts have significantly affected Earth's history.

Eugene Shoemaker
Eugene Shoemaker

Major impacts have shaped the very existence of our world. Scientists believe a massive impact early in Earth's history helped form the Earth–Moon system.

Artist's concept of collision at HD 172555
Artist's concept of collision at HD 172555

Some theories suggest that impacting comets delivered water to Earth. Others suggest impacts brought the building blocks of life through a process called exogenesis. However, impacts can also be destructive. The Chicxulub impact occurred 66 million years ago. This event caused the Cretaceous–Paleogene extinction event. It also accelerated the evolution of mammals, eventually allowing humans to rise.

Barringer Crater aerial photo by USGS
Barringer Crater aerial photo by USGS

We can also observe these events happening in other star systems. In 2013, NASA's Spitzer Space Telescope detected a massive planet impact around the star ID8. This was an extrasolar impact, meaning it happened outside our Solar System.

PIA18469-AsteroidCollision-NearStarNGC2547-ID8-2013
PIA18469-AsteroidCollision-NearStarNGC2547-ID8-2013

In our own system, the frequency of impacts is tied to the size of the object. There is an inverse relationship where larger objects hit much less often. For instance, asteroids 1 kilometer wide strike Earth every 500,000 years on average.

Today, humanity is working to prepare for future risks. The B612 Foundation and physicist Stephen Hawking have noted the threat of devastating asteroids. In 2022, the Double Asteroid Redirection Test was a major success. This was the first human experiment to deflect an asteroid. The mission changed the target body's orbital period by 32 minutes. This exceeded the success requirement of 73 seconds.

Such technology helps us defend our planet from future cosmic collisions.

593 words

Where will your curiosity go next?

Keep exploring at your chosen reading level.

🖼️ Images & Media (14)
File:Tunguska Ereignis-1.jpg
Tunguska Ereignis-1.jpg
File:Bolide.jpg
Bolide.jpg
File:Eugene Shoemaker.jpg
Eugene Shoemaker.jpg
File:Artist's concept of collision at HD 172555.jpg
Artist's concept of collision at HD 172555.jpg
File:Chicxulub-animation.gif
Chicxulub-animation.gif
Hiawatha v45 scene1 4k 5mtopo.1760.tif
File:Barringer Crater aerial photo by USGS.jpg
Barringer Crater aerial photo by USGS.jpg
File:Chelyabinsk meteor trace 15-02-2013.jpg
Chelyabinsk meteor trace 15-02-2013.jpg
File:2018 LA-orbit.png
2018 LA-orbit.png
File:Aitken Kagu big.jpg
Aitken Kagu big.jpg
File:Impact site of fragment G.png
Impact site of fragment G.png
File:Asteroid Collision Hubble.jpg
Asteroid Collision Hubble.jpg

+ 2 more

More to explore

🔬 Go deeper

More advanced topics to explore

🪜 Step back

Simpler topics to build understanding

What is Nepedia?

A free, ad-free encyclopedia for children. Every article is written at five reading levels, so the same page works for a five-year-old and a fifteen-year-old — use the level switcher above to see this one change. No account needed to read.