Saturn

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Introduction

SaturnSaturn, the sixth planet in our solar system and the second largest, has a diameter of 120,536 km, a mass of and spins every 10 and 1/4 hour. It is the least dense of the planets; its specific gravity (0.7) is less than that of water.

Like Jupiter, Saturn is about 75% hydrogen and 25% helium with traces of water, methane, ammonia and "rock", similar to the composition of the primordial Solar Nebula, from which the solar system was formed.

 

Rings

Saturn's ringsTwo prominent rings (A and B) and one faint ring (C) can be seen from the Earth. There are also four additional faint rings.

Though they look continuous from Earth, the rings are actually composed of innumerable small particles, each in an independent orbit.

Saturn's rings are extraordinarily thin: they're less than one km thick. Despite their impressive appearance, there's really very little material in the rings.

Moons

TitanSaturn has the most moons - 18 named ones and at least 4 unnamed ones. Only one moon is large: Titan. It is the second largest moon in the solar system. Titan is about half water ice and half rocky material, and is surrounded by a thick, opaque atmosphere; the surface cannot be seen at all in visible light. There are 6 medium-size moons and 11 small moons.

These moons are irregularly shaped and covered with craters caused by impact of cosmic debris. It is believed that fracturing by large impacts give rise to their irregular shapes.

 

Special Features

Saturn has bright spots that are probably similar to, but much larger than, terrestrial thunderstorms. It is not clear what the dark spots are, though they seem to resemble similar Jovian dark spots.

Saturn - North Temperate Belt The largest violet-coloured cloud belt is Saturn's North Equatorial Belt, whose true colour is brownish. The colour difference between the belts and zones may be attributed to a thicker haze layer.

The south hemisphere appears bluer than the north hemisphere because of differences in scattering of sunlight.

 

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