All of you are welcome in our article. In this article, I am talking about Saturn Moons –How many moons does Saturn have?. First of all, we know a bit about the 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 giant, 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 ħ. If you have to read about the Saturn planet in detail then you can read our article – Information about Saturn Planet.
How many moons does Saturn have?
There are many different satellites of Saturn, the sixth planet in our solar system, in which there is fewer than 1 kilometer in diameter moon and Giant Titan (which is larger than Mercury). In the rings of Saturn, millions of objects are circling Saturn – but many of them are only particles of small stone or dust. Overall, by 2010, Saturn had 62 known satellites whose orbits were tested. Of these, only 13 diameter was more than 50 km and 53 of these were named. Saturn’s seven moons are so big that they can get themselves round the shape of their gravity pulling.
Scientists are very interest in two moons: First is Titan, which is the second largest satellite of the solar system, and on which there is a dense atmosphere from Earth, which is also filled with nitrogen gas, and Second is Anseldas, which has gas and dust fountains And with the possibility of having a large reservoir of water under the surface of the southern pole.
Que. How many moons does Saturn have?
Ans:- Saturn planet has 62 total moons, 53 of which have been confirmed Moon and 9 moons are unconfirmed.
7 Main Moons of Saturn Planet
Saturn’s satellite system is one-sided: More than 96% of the masses in orbit around Saturn and its satellites and rings are orbiting it in just one satellite, Titan. Saturn is about 4% in 6 spherical moons. Combining more than 50 other satellites and rings, only 0.04% is formed.
Mimas is the seventh satellite from Saturn, the sixth planet in our solar system. This is the 20th largest satellite in the entire solar system. Mimas is the smallest known astronomical object, which has rounded itself with the pull of his gravity. The diameter is 396 km.
Seeing the low density of Mimas, it is known that almost all-the-whole is made of water ice and there is very little water in it. Due to the tidal force born of Saturn’s fierce gravitational force, the mice ball appears a little bit pitch – its axis is 10% less than the other axis. On the satellite, the fall of many meteorites has become a crusher crater. The vast crater of a herbal name is 130 km in diameter, which is one-third of the diameter of the entire satellite. The floor of this crater is somewhere at a depth of up to 10 km from the ground around it and the walls of this pit are 5 km high.
diameter, craters in their southern pole area are less than 20 km. It is just unknown why this is either – either a process is erasing the marks of big craters from here, or any process is preventing meteorites from falling into this area.
Enceladus is the sixth largest satellite of the sixth planet of our solar system Saturn. It is very small in size – its diameter is only 400 km, which is just one-tenth of the largest moon. Regardless of this small size, different types of things are seen on the surface from moles to trenches to meteor pits.
On the surface of the Enceladus, a thick layer of snow mostly extends. Enceladus albedo (white or brightness) is 1.38 due to this freezing surface, which is more than any other known object in the solar system.
Tethys is the fifth largest satellite of Saturn, the sixth planet in our solar system. It is the 16th largest satellite in the entire solar system and is bigger than the masses of smaller satellites on its own. Almost all-of-the-water ice, and barely 6% of it is stone. It is not conclusively estimated that in Tethys there are separate legs of stones and ice, or in the snow only It is known, but it has become known to the scientists that if there is a separate stone at its center then the diameter of the sphere will be 290 km or less.
The diameter of Tethys is approximately 1,066 km. For comparison, the diameter of the Earth’s Moon is approximately 3,470 km, that is, about threefold from Tethys.
Dione is the fourth largest satellite of Saturn, the sixth planet in our solar system. It is the 15th largest satellite in the entire solar system and is bigger than the masses of smaller satellites. Although it is mostly made of water ice, Saturn’s third most dense satellite after Titan and Enceladus, it is estimated that half a little less (46%) of its structure is stone. In the direction in which it orbits, on the side of that side, there is a lot of crushing crater created by the collision of meteorites, while on the other side the ice rocks are covered with glittering rocks.
Dione diameter is approximately 1,122 km. For comparison, the diameter of the Earth’s Moon is approximately 3,470 km.
Rhea is the second largest satellite of Saturn, the sixth planet in our solar system. It is the largest satellite of all the satellites in the Solar System. It was discovered in 1672 by the Italian astronomer Giovanni Domenico Cassini. Considering the density of Rhea, scientists estimate that this is made up of 25% of stone and 75% water ice. The temperature of this satellite depends on the sun.
Where the sun is coming, its temperature is -174 degrees centigrade (99 Calvin) and where it is dark it falls to -220 degrees centigrade (53 Calvin). Because of the meteorites falling from space on its surface, there are many caves, two of which are very large and keep the diameter of 400 to 500 km (diameter).
Titan is the largest moon of the planet Saturn. It is the only known moonland with environments, and is the only such celestial body in addition to Earth, with solid evidence of surface liquid locations, such as canals, oceans, etc.
On January 16, 2004, where he sent pictures of Titan’s tributaries in the brown-orange colors – mountains and lakes ponds. Due to the very dense atmosphere of Titan before it was not possible to see or draw its upper surface.
In the middle of August 2008, such images were shown at the conference of the International Astronomy Association in Brazilian Rio de Janeiro, and two such papers were presented, to which Titan’s equation with the Earth is clear.
Iapetus is the third largest satellite of Saturn, the sixth planet in our solar system. It is an eleventh largest satellite of all the satellites in the solar system. It was discovered in 1671 by Italian astronomer Giovanni Domenico Cassini.
The appetite is famous for the color of one part of it is quite light and the color of the other part is very thick. An elevated rock has been observed in the middle line of this satellite, which runs to half of this moon. The density of the Lapetus is quite small and scientific estimates show that there is only 20% of the stone and all the water is ice.
Confirmed Moons of Saturn
Unconfirmed Moons of Saturn
|1. S/2004 S7|
2. S/2004 S12
3. S/2004 S13
|4. S/2004 S17|
5. S/2006 S1
6. S/2006 S3
|7. S/2007 S2|
8. S/2007 S3
9. S/2009 S1