Saturn, the second largest solar system, circulates about 900 million miles (1,400,000,000 km) of the sun.
Today in Saturn is 10 hours, but one year can reach up to 29 years.
Saturn is a gas planet, or a gas giant, mostly composed of hydrogen with a small amount of helium, methane, water and ammonia.
The planet is not dense, in fact it can float on the water. Saturn's fascinating rings consist of watery ice, rock and dust. There are also wonderful consequences for the weather in Saturn.
The temperature on the surface of the clouds of Saturn is about -400 F (or 240 C below zero). This temperature is cool enough to freeze the ammonia, and then increase its density and fall into a warmer and lower atmosphere, which resolves again.
Saturn's solid core probably contains nickel, iron, rock and metal hydrogen. The inside of the planet is very hot due to the high pressure of its attractiveness, the temperature reaches more than (11,700 C). Scientists estimated the overall temperature of the planet (176C).
Satellite recorded wind speed on Saturn and exceeding 1,000 mph (1609 km)
Saturn has thunderstorms stretching for thousands of kilometers. Thunderstorms on Saturn are 10,000 times stronger than those on Earth's surface.
Lightning in Saturn produces radio waves known for electrostatic discharge.
Long-term storms called white leaves may take months or even years.
The North Pole of Saturn is the place of a permanent hurricane with a width of more than 1200 km and a wind speed of approximately 330 miles per hour (531 km).
Monitor the storms elsewhere on the planet, including the equator, a spot where the white spot disappears and appears Earth almost every 30 years.
Rain in the rain:
In 2013, the Keck telescope in Hawaii detects ice-depositions on Saturn circles that fall into the planet's ionosphere.
These electrically charged water drops draw dark lines on top of the planet's atmosphere.
Lynne parallel to the equator of the planet and magnetically linked to the bright Saturn rings.
Light spaces between lines match the spaces between the rings of Saturn.
Scientists speculate that the rain generated by the rings consisted of 10 olympic sizes of water on Saturn's atmosphere every day.
This rain can contribute to higher than expected temperatures in the ionosphere of Saturn.
Scientists in 2013 used new data to describe how Saturn, next to Jupiter and probably Uranus and Neptune, faces rain of diamonds.
Intense electric storms can separate organic compounds such as methane and release pure carbon which in turn falls into the planet's surface.
At low heights atmospheric pressure is strong enough to convert carbon atoms into graphite and then into their diamond shape.
Finally, the pressure and heat build up to the point where the diamond melts.
More than 1000 tons of diamonds come from lightning strike and fall into Saturn's atmosphere every year.