Comets- Identify the nucleus, coma, dust and ion tails of comets
- Demonstrate an understanding that the tails of comets develop when relatively close to the Sun
- Demonstrate an understanding of the mechanisms for the development of cometary dust and ion tails
Comets are ice and rock bodies. Typically their nucleus (the solid part) is no larger than an average asteroid.
As the comet approaches the sun, some water-ice evaporates and jets of gas and dust produce a spherical coma around the nucleus. The coma may be many times larger than the nucleus but is very thin, held by the comet’s very weak gravity.
The comet gets nearer to the sun and a tail forms in the opposite direction to the Sun. Really this is two tails. A curved dust tail forms and can be up to several millions of kilometres long. This tail forms because of radiation pressure from the Sun.
The dust tail is very bright to an observer because of the reflection of the ice particles from the Sun.
Particles from the solar wind hit the comet and an ion tail is produced which is more coloured but straighter than the dust tail.
Comets leave debris behind them. Some of this comes to Earth in the form of meteors.