Saturn Is A Gas Giant

Saturn, along with the other gas giants’ rings are made up of mostly ice and large pieces of rock surrounded by an icy coating. Saturn’s ring system contains billions of ring particles that range in size from dust - size, icy grains to few even as large as mountains. Two of Saturn's tiny moons orbit in the gaps of Saturn's rings. The gaps they orbit inside of are known as Encke and Keeler gaps. These two moons make up the total of fifty - three moons that NASA has discovered and

Saturn is unique of all the planets, adorned with thousands of beautiful ringlets and has 63 moons with confirmed orbits. Fifty-three of the moons have been named, with Titan being the largest and the only one with an atmosphere. Saturn is mostly a massive ball of hydrogen and helium, much like the planet Jupiter.

Enceledus is the sixth-largest moon of Saturn which discovered by William Herdchel in 1789. Three spacecrafts contributed the main discovery of the Enceledus. Voyager I spacecraft found that Enceledus has a high albedo and is orbiting inside the E ring of the Saturn at the highest density point whereas Voyager II spacecraft observed that there are at least 5 type of terrain on the surface such as crater terrain, young terrain and so on. Cassina spacecraft discovered water-rich plumes venting from the south polar region which approved that the Enceledus is the source of the E ring and is able to create life. In addition the environment on Enceledus is perfect fits in all the chemical requirements for life existence.

Krogans’ lungs have evolved to be longer so that the carbon dioxide filled air can be cooled down and be exhaled as oxygen. Their skin is very rough, like a lizard’s, to combat the high temperatures of Venus. Their ursula stems (bones), are very durable to withstand the high atmospheric pressure of the planet.

Saturn is the most fascinating planet in our Solar System. Saturn was named after the Roman God, Saturn; however in Greek, his name was Cronos, King of the older Gods. Cronos was the father of Zeus and the God of Time and Ages. Saturn, the planet itself, is comprised of liquid and gas. It has 7 rings that are formed from ice, rock, and dust. It is the 6th planet from the sun, which is 885 million miles away. Saturn is surprisingly the 2nd largest planet. It has the capacity of 764 earths or 75,000 miles wide. Saturn has 62 moons; 53 known and 9 provisional. Over time, these moons were named after the older Gods; the first moon Titan. Saturn spins so fast on its axis, that its days are 10 hours long. Saturn is the 2nd largest planet, however

Saturn: a gas giant whose mass almost holds 100 earths. Ever since ancient times Saturn has efficiently mesmerized humankind. Recently there has been many observations of this fascinating planet. From the moons to the rings to the specs of dust- we are at awe. Some of the most intriguing parts of Saturn are the following: Enceladus’ Plumes, Titan’s Lakes, and Saturn’s Hexagon. Know there must be a question you must be pondering about. Which one of these three would bring the best yield to the process of scientific discovery? The answer: Saturn’s Hexagon.

Saturn's largest moon is Titan, is a bit bigger than the planet Mercury. Titan is the second largest moon. Saturn has a light orange look with white and gray rings. These rings are made up of ice, rocks, and dust. Saturn's rings are more than 270,000,000 kilometers wide but not even 1 kilometer thick, it also has more than 30 layers of the ring. It is made up of 94% hydrogen, 6% helium. Which means it is mostly gas. Its temperature is around minus 178 degrees Celsius.

Many questions posed by scientists about Saturn’s atmosphere had gone unanswered for many years, because, like with Jupiter, photos from Earth had not been of high enough quality. The Voyager probes were able to fix that. Information relayed back to Earth from the two probes (which reached Saturn nine months apart, Voyager 1 first in 1980, Voyager 2 in 1981) helped scientists get a much better understanding. Though the atmosphere was expected to be quite similar in composition to the Sun and to Jupiter, Saturn’s atmosphere was actually quite different. There was significantly less Helium in Saturn’s outmost atmosphere, leading to many interesting conclusions, including that heavier Helium was sinking lower in the atmosphere (Voyager- Saturn, NASA). Saturn was also determined to have a lighter density than any other planet and is, in fact, less dense than water. The varying composition of the atmosphere also leant ideas to why Saturn was far warmer than expected, calculating temperature based solely on solar energy, registering between 10 degrees Kelvin at the poles and 143 Kelvin closer to the equator, according to Voyager 1’s radio measurements (these also measured pressure) (Voyager- Saturn, NASA). One of the other things determined by the Voyager probes was the extreme speed of the wind on Saturn. Wind blows at speeds of about 500 meters per second near the equator (Voyager- Saturn,

Saturn is the second largest planet in the solar system. Jupiter is the only planet that is larger. The gas giant is 72 thousand miles in diameter, almost ten times the size of Earth. In spite of its huge size, though, Saturn weighs very little. It is a very light gas planet. Saturn is the least dense planet in the solar system-- so light, in fact, that it would float in water. This planet is mostly composed of hydrogen and helium, like Jupiter, but it is much less dense. The combination of its light weight and fast rotation causes Saturn to spread out, or oblate, its center. Since Saturn is a gas planet, it does not have a solid surface. Spacecraft are unable to land on this type of surface. The clouds that are seen when looking at Saturn are just the top layer of a very deep layer that covers a center of liquid hydrogen. The clouds are blown by constant winds that reach speeds up to one thousand miles per hour at the equator of the planet (“Great Space Place”).

Saturn’s axis is titled 26.73 ° comparable to Earth’s 23.5 ° tilt, which gives Saturn seasons. Saturn rotates in the same direction as Earth, which is east to west. Its rotation is surprisingly fast, being equivalent to only 10.7 earth hours. This causes Saturn’s equatorial radius to be 10 percent wider than its polar radius. However, its orbit around the Sun is quite a bit slower. One full orbit takes 29 years for Saturn to complete. As for weather, Saturn averages a temperature of about -168 ° C with winds as fast as 1800 kilometers an hour in the upper atmosphere.

“Furthermore, the icy rocks in the rings reflect the sunlight to produce the vivid colors. Saturn’s rings span two hundred and eighty-two kilometers, whereas Spes’ rings stretch a hundred and fifty thousand kilometers across. The immense size of these rings is primarily due to this planet’s relative youth of only three million years in contrast to Saturn’s age of four and a half billion years. Eventually, the icy rocks in outer rings of Spes will coalesce to form moons, similar to the fifty-three moons of Saturn. In other words, the ring system will slowly whittle away over the millennia, leaving only the inner bands. At present, Spes has a single moon on the periphery of the ring system. We can also see the three radiant suns in the

The extreme temperatures and the lack of a significant atmosphere so asteroids could hit the planet very easily are also huge environmental hazards.

They are similarities. All have dates and facts. For example in “The Mysteries of Saturn” it states, “in July 2004 the Cassini spacecraft entered Saturn’s orbit and began to collect valuable information” In “Cassini Mission” it states, “in December 2004 a probe was dropped into Titan’s atmosphere. Then the leader began gathering data.” According to the illustration the first picture of Earth, Mars, Venus, and Saturn together was taken by the Cassini in 2013. All of this information was gathered using improved technology.

Saturn is considered to be the second largest planet within our solar system. It consists of mostly hydrogen and helium. Saturn's rings are believed to be holding multiple fragments of comets, asteroids and even shattered moons that had broken up before entering the planet. The particles in the rings compare in size from a tiny dust-sized grains to chuck's almost the size of mountains. The ring system reaches about 175,000 miles. The ring system includes what can only be considered "braided rings", ringlets, and "spokes" which are dark features that form within the rings. The rings generally circle the planet at different rates. The shepherd satellites affects some planetary rings in different ways. In the case of Saturn, this planets satellites,

Cassini found a frosty crest shooting from this moon, and consequent perceptions have uncovered the spread contains complex natural chemicals. Tidal warming is keeping Enceladus warm, and hotspots connected with the wellsprings have been pinpointed. With warmth, natural chemicals and, possibly fluid water, Enceladus could be a spot where primitive life structures may develop. Inquiries encompassing Enceladus' "astrobiological potential" are at the heart of numerous examinations being directed in the Solstice