Saturn Planet

Planet Saturn – Information About Saturn Planet

Saturn is the sixth planet from the Sun, and after Jupiter, it is the largest planet in the solar system. Saturn is a gas demon, nine times bigger than Earth in the average diameter. While its average density is one-eighth of the Earth, with its large volume, it is slightly larger than 95 times the Earth. Its astronomical sign is ħ.

Saturn Planet

Planet Saturn – Information About Saturn Planet

Saturn’s internal structure is probably made of a core of iron, nickel, and rocks (silicon and oxygen compounds), which is surrounded by a thick layer of metallic hydrogen, liquid hydrogen and an intermediate layer of liquid helium and an external gaseous layer. The planet shows a light yellow color due to its upper ammonia crystals. It is believed that the electrical current within the metal-hydrogen layer, which promotes the planetary magnetic field of Saturn, which is weaker than Earth and is close to one-twentieth power of Jupiter. The outer atmosphere is generally lacking in monotony and clarity, although longitudinal figures can be seen. The wind speed on Saturn can reach 1800 km / h (1100 mi), which is faster than Jupiter but not as fast as it is on Neptune.

At least 62 moons are known to orbit Saturn; fifty-three is official Name. They do not include hundreds of “small moon” within the rings. Titan is the largest moon of Saturn and the second largest moon in the solar system. It is larger than Mercury planet and is the only moon of the solar system to store a large atmosphere.

Saturn Planet
Diameter120,536 km
Volume8.2713×1014 km3
Mass5.68 × 10^26 kg
Moons62 Moons
Orbit Period10,756 days
Temperature-178 °Celsius
Orbit Distance1,426,666,422 km
Surface gravity10.44 m/s2 (34.3 ft/s2)
Synodic period378.09 days
Mean density0.687 g/cm3

Internal structure

Saturn is declared a gas monster but it is not fully gaseous. The planet is mainly made of hydrogen, which becomes a non-ideal fluid when the density is above 0.01 g / cm3. This density increases as much as 99.9% of Saturn’s mass on one radius. The temperature, pressure, and density within the planet grow rapidly on the direction of all the cores, in which the deep layers of the planet, hydrogen causes a metal change.

Standard planetary models show that Saturn has the same inner texture as Jupiter, with a fraction of volume, a rocky core surrounded by hydrogen and helium, which is similar to the core of the earth, but denser. In 2004, they estimated that the core should be 9-22 times the mass of the Earth, which corresponds to a diameter of around 25,000 km. This core is surrounded by a thick liquid metallic hydrogen layer, which is followed by a liquid layer of helium-saturated molecular hydrogen, with gradual changes in the gas with increasing elevation. The outermost layer extends over 1,000km and is composed of a gaseous environment.

Saturn is a very warm inner part. Mercury in the core climbs to 11,700 degrees Celsius. Leaves 2.5 times more space than the planet receives as much energy from the sun. These falling droplets may be deposited in a helium shell around the core.

Atmosphere of Saturn

Saturn’s outer atmosphere comprises 96.3% of molecular hydrogen and 3.25% helium. This proportion of helium is much less in comparison to the abundance of this element in the sun. The amount of heavy elements from helium is not exactly known, but the ratios are assumed to match the initial extinction emanating from the formation of the Solar System. With a significant fraction located in the core area of ​​Saturn, the total mass of these heavy elements is estimated to be 19-31 times the mass of the Earth.

The quantity of ammonia, acetylene, ethane, propane, phosphine, and methane have been detected in Saturn’s atmosphere. The upper clouds are made of ammonia crystals, while lower level clouds appear to be either ammonium hydroxide (NH4SH) or water consisting of water. Ultraviolet radiation released from the Sun causes methane dissociation in the upper atmosphere and represents a series of hydrocarbon chemical reactions with the resultant products being taken down from whirlwind and diffusion. This light chemical cycle is cured by Saturn’s annual seasonal cycle.

Saturn Planetary Ring

Saturn is probably better known for the system of planetary rings which makes it visually unique. The rings extend from 6,630 km to 1,20,700 km on Saturn’s equator, on average, about 20 meters in thickness and 93 percent water ice with 7 percent amorphous carbon content and 7 percent amorphous carbon. The particle size particles that form rings are ranging from dust particles up to 10 meters. Although other gas monsters also have ring systems, Saturn is the largest and most visible.

There are two main concepts about the origin of rings. One hypothesis is that the rings are the remains of a destroyed moon of Saturn. The second hypothesis is that the rings are the basic nebulae material left from which Saturn is formed. Some of the central rings come from the Enceladus moon’s ice volcano. In the past, astronomers made the rings together with the planet when the planet formed the Billions of years ago. In spite of this, the age of these planetary rings is probably a few hundred million years old.

Moons of Saturn

Saturn has at least 62 moons, 53 of them have formal names. The largest moon, including Titan, rings, contains more than 90% of the mass in orbit around Saturn. Along with a weak atmosphere, Saturn’s second largest moon, Riya, may have its own weak ring system. Traditionally, most of Saturn’s Moon has been named on the legends of Greek mythology. Titan is the only satellite of a large atmospheric solar system, in which complex organic chemistry is found. This is the only satellite with hydrocarbon lakes.

Saturn’s Moon Enceladus has often been considered as a possible basis for microbial life. Evidence of this life involves the salt-rich particles of the satellite, in which an “ocean-like” association is found, which indicates that most of the extracted ice liquid salts from Enceladus comes from the evaporation of the water.

Orbit and Rotation

The average distance between Saturn and the Sun is more than 1.4 billion kilometers (9 AU). To complete a rotation around the Sun, with an average rotational speed of 9.69 km/second, it takes 10,759 Earth days of Saturn (or approximately 29½ years). The elliptical orbit of Saturn is 2.48 ° inclined relative to the orbital plane of the Earth. Due to the decentrality of 0.056, the distance between Saturn and Sun varies between about 155 million kilometers between the adjacent and the adjacent. Which is the closest and most distant point of the planet, along with its rotation path.

Visible figures on Saturn rotate at different rates which depend on latitude. These multiple rotating periods have been allocated for different areas (such as in the case of Jupiter). The system period is 10 hours 14 minutes 00 seconds (844.3 ° / day). System III is based on radio emission emitted from the planet during Voyager tour. It has a period of 10 hours 39 minutes 22.4 seconds (810.8 ° / day). As it is very close to System II, it has encroached to a great extent.

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