|
| Solar System | Nebulae | Galaxies | Stars and Clusters | Equipment | Links Last edited - 12 December 2001 |
|
![]() |
![]() |
![]() |
|
| SATURN 1 | OCCULT01 | OCCULT02 | OCCULT03 |
![]() |
![]() |
![]() |
![]() |
| OCCULT04 | OCCULT05 | OCCULT06 | OCCULT07 |
![]() |
![]() |
![]() |
![]() |
| OCCULT08 | OCCULT09 | OCCULT10 | OCCULT11 |
![]() |
|||
| SA311101 |
![]()
(Please adjust your monitor such that you can see all 17 shades)
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. |
