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A handy FAQ about meteorites, meteors and other small celestial bodies that Earth encounters in its travels around the Sun.
Most meteors you see in the form of shooting stars (meteor showers) are dust-sized particles that burn up as they pass through Earth's atmosphere. Sometimes larger meteors don't completely burn up in the atmosphere - instead they fall to Earth's surface. When these extraterrestrial objects are recovered from Earth's surface, they are known as meteorites.
Most meteorites are bits of asteroids from the asteroid belt between Mars and Jupiter, although some are bits of comets (meteors) or, very rarely, pieces of the Moon or Mars.
A meteoroid is a small body in our solar system that would only become a meteor were it to encounter Earth's atmosphere. A meteor doesn't technically become a meteorite unless it survives the journey to the ground.
The main difference between comets and asteroids is what they are made of. Asteroids are made up of metals and rock, while comets are composed of dust, rocky material and ice. They both orbit the Sun and were created during the formation of our solar system 4.5 billion years ago.
Meteor showers occur when Earth passes through the dust trail left behind by comets as they pass close to the Sun. The result can be spectacular displays of as many as hundreds of meteorites flashing across the sky like natural fireworks. Get tips on how to watch the next meteor shower.
Most meteorites are fragments that have broken away when two asteroids collide. A small proportion of meteorites also come from the Moon and Mars.
Scientists can tell if meteorites are from the Moon as their composition is very similar to samples brought back from the Apollo lunar mission. Martian meteorites can be identified due to their similarities to Mars’s atmospheric composition, which was detected by the Viking probe.
Meteorites from asteroids are around 4.5 billion years old. Meteorites from the Moon are older than 2.5 billion years, and meteorites from Mars may be as young as 165 million years.
Although few meteorites are observed hitting the ground - most fall into the sea - thousands of meteorites are collected each year. They can be found all over the world but are easiest to spot in dry places, such as the desert in Australia or Antarctica, where they do not erode quickly and are less likely to be hidden by vegetation.
No. Meteorites do contain radioactive elements, but not significantly more than any ordinary terrestrial rock.
No evidence of extraterrestrial organisms has been found in meteorites.
The impact of a comet or asteroid 66 million years ago is thought to have contributed to the extinction of around three quarters of all species living on Earth at the time, including many dinosaurs.
Yes. Asteroid and comet collisions with the Earth are a natural hazard. The risk is, however, relatively small. More information is available from the Spaceguard Centre and NASA's Near Earth Object Program.
There have been no recorded deaths due to a meteorite fall. The chances of witnessing a meteorite fall, let alone being hit by one, are very, very small.
The largest impact crater on Earth is in South Africa, called the Vredefort Dome. It is very ancient and poorly preserved, and measures roughly 300 kilometres across. The impact from the meteor would have been enormous.
Scientists predict that a meteorite around 30-50 metres across, capable of forming a kilometre-wide crater, will occur around every 1,000 years. However, the last impact of this size that we know of took place 55,000 years ago.
The chances are that a large meteorite will hit Earth again eventually, as there is a lot of asteroid activity in our solar system. Global observation networks are keeping constant vigil, so there should be plenty of warning about potential impacts. Scientists have proposed plenty of strategies to deflect or destroy Earth-bound asteroids, though these depend on the size of the asteroid.