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  Solar System   |  Nebulae  |  Galaxies  |  Stars and Clusters  |  Equipment  |  Links                     Last edited 12 December 2001
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Technical Data:-

Diameter 120,200 km
Average Distance from Sun 1,427 million km
Size Compared to Earth(Diameter) 9x
Gravity compared to Earth

0.93

Cloud-Top Temperature -180°C
Length of Day 10 hours 14 mins
Length of Year 29.46 Years
Eccentricity of Orbit 0.056
Moons 22
Density

0.70gm/cm3

Atmosphere Hydrogen - 94%
Helium - 6%
Traces of Methane, Ammonia & Water Vapour

 

Saturn (the Roman God of Agriculture) has a diameter of 120,000 km which makes it the second largest planet in the Solar System!  Although it isn't quite as large as Jupiter, it still has a size to be reckoned with and across it's equator it could fit the Earth over nine times!  Saturn is another 'Gas Giant' but, beneath the atmosphere it has an ocean of molecular liquid Hydrogen which enfolds a shell of metallic Hydrogen.  The centre core itself is about as big as the Earth.   Another thing about Saturn is that it's shape is similar to that of a squashed football; it's flattened at the poles.  This is because the planet spins so fast that the centrifugal force makes the equator bulge outwards.

Saturn's atmosphere is a bit like Jupiter's except that it is colder and the cloud layers are thicker.  It is not a particularly dense planet either, the mass is so spread out that on average it's less dense than water!  Like Jupiter, it also seems to have big storms raging in its atmosphere and around the equator winds sweep about at 1,800 km/h.

The most famous feature(s) about Saturn though are it's rings.   They were first spotted by the great Italian astronomer Galileo Galilei but it was a few decades later that Christiaan Huygens (Dutch astronomer) discovered that they were seperate from the planet.  Then Cassini discovered the Cassini division and later on it was discoverd that there are actually many rings and that they are made of rock and ice.  The rings are quite insubstantial; at some points they may be only 1km thick!   Saturn also has a magnetic field 1,000 times stronger than Earth's.

Saturn's 22 moons are : Pan, Atlas, Prometheus, Pandora, Epimitheus, Janus, Mimas, Enceladus, Thethys, Telesto, Calypso, Dione, Helene, Rhea, Titan, Hyperion, Iapetus and Phoebe and 4 other out moons.  The most important one is Titan and scientists hope to find out what the Earth was like long ago through studying it.   It's also a rather large moon, being bigger than Mercury.  Titan is the only moon in the Solar System to have an atmosphere.  Scientists recently discovered day clouds on Titan and this adds to substantial evidence suggesting it has clouds, rain and seas like Earth.   The European Space Agency is planning a mission (the Huygens) to Titan to find out more about it.

Galileo Galilei discovered Saturn's rings in 1610 and it was in 1659 that Chistiaans Huygens realised they weren't physically attatched to Saturn.  Then in 1676 Italian-French astronomer Jean Dominique Cassini discovered the Cassini division in the rings.  The first pictures of Saturn's polar regions were taken in 1979 by the Pioneer 11 and a year later, in 1980, Voyager (the probe, not the Star Trek spaceship) took 17,500 colour pictures of the planet, measured wind speeds in Saturn's equatorial region and measured Titan's size. Voyager 2 passed even closer than Voyager in 1981.   On the 15th October 1997 the Cassini spacecraft was launched towards Saturn and it's expected to arrive in 2004.



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