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The solar system

Used by permission of The University of Texas McDonald Observatory

About 3,000 light-years from Earth, two mysterious “searchlights” of glowing stellar gas and dust emerge from the cocoon that surrounds a dying star, called the Egg Nebula. (STScI)

The solar system consists of a central star, our Sun, which has a family of planets, moons, meteors and comets orbiting around it.  In the planetarium we are mainly concerned with what can be seen with the naked eye.  As far as the solar system is concerned that means the Sun, the moon and the planets, Mercury, Venus, Mars, Jupiter, and Saturn.
 

As the planets, including Earth, orbit the Sun in the same plane or level, we see the planets in the sky only in the same plane.  This is the plane in which the Sun appears to move also and is known as the ECLIPTIC.  Students can remember the name ecliptic if it is explained that the Sun in its apparent path eclipses the stars as it moves in front of them.  Of course it is not the sun that is moving but the Earth in its annual journey around the Sun.  So the planets can only be found in the ecliptic.

When talking about distances we explained how incredibly far away the stars are.  So far away in fact that although they appear to move in space they do not appear to move relative to us, just as a jet plane very high up appears to move very slowly when we know it is travelling at least 400km/h.  Stars are so far away that
their movement cannot be discerned with the naked eye in our lifetime, or even several lifetimes.

So stars can be considered fixed in space.  Not so for some objects:

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