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Short Intro Text

Comets are large balls of rock, ice, dust and gases. They contain frozen leftovers from the early Solar System. Material that is about 4,600 million years old!

Scientists think that comets could have hit the Earth when the Solar System was very young. They may have brought water and organic compounds with them. These are the ingredients needed for life.

During most of their orbit, comets are hard to see. This is because they are small and made of dusty ice which does not reflect much light from the Sun. As a comet get closer to the Sun, the ice in the comet heats up. Some of this ice turns into a gas. The gas gets lit up by the Sun's light, making it easier to spot with a telescope.

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An image of Comet Hale-Bopp, displaying a bright nucleus with a glowing white and blue tail, extending across the star-filled background of space
Credit
This work by Loke Kun Tan on March 30, 1997 from the Red Rock Canyon Park in California is licensed under Creative Commons Attribution 4.0 International
Comet Hale Bopp
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Astronomers have discovered about 4,000 comets in our Solar System so far. Most comets come from beyond Pluto, in the Oort Cloud. We have not fully explored these dark and distant parts of space yet. So there are probably billions more comets out there!

 

The Oort Cloud

The Oort Cloud is a huge sphere of icy rocks beyond the Kuiper Belt. It is thought to surround the entire Solar Solar System

The Oort Cloud is about 2 light years away from Earth. This means it takes light - travelling at 300,000 kilometres every second - 2 years to reach Earth from the Oort cloud! The Oort Cloud is sometimes used to mark the edge of our Solar System. 

We think most of the comets in our Solar System come from the Oort Cloud, but we do not know much else about it. Because it is so far from the Sun, the objects in the Oort Cloud are too dark for astronomers to observe. 

The Voyager spacecraft have travelled further than any other space probe. Voyager 1 and Voyager 2 left Earth in 1977. It will take them about 300 years to reach the inner edge of the Oort Cloud. It could take 30,000 years to fly past it!

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Diagram of the Solar System showing the location of the Oort Cloud and Kuiper Belt. The Sun and the orbits of the planets are depicted on the left, with the Kuiper Belt beyond Neptune. The Oort Cloud, a spherical shell of icy objects, surrounds the Solar System at distances of 5,000 to 100,000 Astronomical Units (AU)
Credit
This work by Jedimaster is licensed under Creative Commons Attribution 4.0 International
What are the different parts of a comet?

The solid centre of a comet is called its nucleus. It is made of solid chunks of ice along with frozen gases, rocks and dust. You can think of it as a giant, dirty snowball. The nucleus is usually only hundreds of metres across, but can be the size of a small town! Astronomers have seen comets releasing jets of gas and dust from their nucleus, like a geyser.

As a comet gets closer to the Sun, the ice in the comet heats up. Some of this ice turns into a gas. The gas (plus dust and some water) forms a cloud around the nucleus, called a coma. You can think of the coma as the comet’s atmosphere. The coma can be as large as a planet!

Sunlight and super-fast particles from the Sun (solar wind) can push the coma into a large tail. This tail always points away from the Sun. The gas in the tail contains charged particles called ions, so this tail is sometimes called the ion tail. Some comets ion tails are over a million kilometres long!

Comets can also leave a trail of small rocks and dust in their path. This is known as the dust tail. When the Earth passes through a comet's dust tail, debris from the comet falls through our atmosphere. This creates meteor showers.

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Diagram of a comet showing its structure with labels: nucleus, coma, dust tail, and ion tail. The sunlight and solar wind direction are indicated by an arrow, influencing the direction of the tails. The comet's orbit is represented by a dashed line
Credit
This work by The Schools' Observatory is licensed under All rights reserved
Anatomy of a comet
Why do comets sometimes get close to the Sun?

Comets sometimes get close to the Sun because they have very elliptical orbits. This means that they go around the Sun in a large, stretched out oval shape, rather than a circle.

The furthest point from the Sun in an orbit is called aphelion. The aphelion of most comets is way beyond the planet Neptune.

The closest point from the Sun in an orbit is called perihelion. The perihelion of some comets can be closer to the Sun than the planet Mercury! These kinds of comets are called 'sungrazers'. These comets may end up crashing into the Sun. Or the heat from the Sun will cause them to break into pieces and evaporate away.

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Illustration of a comet's orbit around the Sun. The diagram shows how the comet's tails get longer as it approaches the Sun. The gas (ion) tail always points away from the Sun, while the dust tail curves along the comet's orbital path
Credit
This work by NASA is licensed under Creative Commons Zero v1.0 Universal
The path of a comet around the Sun (not to scale)
What are some well-known comets?
  • Halley’s comet – British astronomer Edmund Halley observed this comet in 1682 and correctly predicted it would return in 1757. This is also thought to be the comet included in the 1066 Bayeux Tapestry.  
  • Shoemaker-Levy 9 – this comet crashed into the gas giant planet Jupiter in 1994.
  • 81P/Wild 2 – visited by NASA’s Stardust mission in 2004. The spacecraft brought dust from the comet back to Earth.
  • 67P/Churyumov-Gerasimenko – ESA’s Rosetta mission visited this comet in 2014 and became the first spacecraft to land on a comet.