The conditions under which Saturn s storms are formed, how Saturn is formed

Saturn's storm begins with a huge dark cloud about the size of Earth.

Saturn storms are thought to approximate to Earth thunderstorms with radio noise produced in high-voltage lightning discharges. When the storm starts, the total area of the area engulfed by the storm is the size of 30 Earths. Astronomers have calculated that Saturn's storm will move at about 450 meters per second, 10 times the speed of jets on Earth and three times faster than a storm on Jupiter's surface.

On Earth, storms typically last only a few weeks, and as they mature, they gradually weaken and no longer draw new energy from their surroundings. On Saturn and other giant planets, storms can often last for months, years, or even centuries. And they usually don't fade down, but end their journey in the form of a merger.

On Saturn, the storm moves in a circular path across the planet. In Saturn's summer, the hot air moves in the opposite direction, becoming extremely unstable at a certain altitude, and due to the high content of ammonia in it, it eventually forms ice-like crystals.

Saturn is one of the eight planets of the solar system, the most obvious sign is the rings of Saturn around itself, in addition to the north pole of Saturn there is a mysterious hexagon, which fascinates astronomers, what is this hexagon, will it be the masterpiece of alien civilization?

Saturn (Latin: saturnus, symbol:

It is one of the eight planets in the solar system, and the distance to the sun ranks sixth in the solar system. Ancient Chinese Saturn was named by the ancient Chinese according to the Five Elements Doctrine combined with the color (yellow) of Saturn observed by the naked eye, also known as Zhenxing (often written as filling in the star). Saturn's English name comes from Saturn, the god of agriculture in Roman mythology.

Saturn is a gas giant composed mainly of hydrogen, with a small amount of helium and a small amount of elements, and its inner core consists of rock and ice, and its outer perimeter is covered by several layers of metallic hydrogen and gas. The outermost layer of the atmosphere is usually bland in appearance, although sometimes long-lived features appear. When Saturn's winds reach 1,800 km, the wind speed is significantly faster than that of Jupiter.

Saturn's planetary magnetic field strength is between that of Earth and the stronger Jupiter. Saturn has a significant ring system, the main components of which are ice particles and a small number of rock debris and dust. In 2019, 82 moons of Saturn were confirmed, the most of the eight planets.

Among them, Titan is the largest moon in the Saturn system and the second largest in the solar system, second only to Ganymede, larger than Mercury among the planets, and Titan is the only moon in the solar system with a significant atmosphere. One rotation of Saturn is equal to 10 hours, 33 minutes and 38 seconds, which is about half a day on Earth.

While both Saturn storms and Jupiter are gas giants, there are several reasons why Saturn storms are stronger than Jupiter:

Barometric pressure difference:Saturn's atmosphere is weaker than Jupiter's, and its air density and pressure are smaller than Jupiter's, so the same storm has a greater sphere of influence on Saturn.

Airflow Structure:The airflow in Saturn's atmosphere has a more complex structure, with many different airflow bands and storms, resulting in more abundant and complex storms.

Optical Properties:Saturn's gaseous atmosphere contains a large number of dust and ice particles, which have a certain optical and slippery effect on the development and impact of storms, making them more visible on Earth.

External factors:Saturn and Jupiter have different orbital positions, with Saturn being farther away from the Sun on average and having less radiation such as the solar wind along its path than Jupiter, making its storms last longer and be larger.

In summary, a combination of factors has contributed to the fact that Saturn's storm is stronger than Jupiter's.

Both Saturn and Jupiter's storms are very intense, but they differ in intensity and characteristics. It is difficult to directly compare their strength because of the differences in their formation mechanism, duration, and scale. However, we can analyze some of the characteristics of storms on these two starving planets for comparison.

The most famous storm on Jupiter is the Great Red Spot, a huge cyclone that has been going on for hundreds of years. The Great Red Spot is about 10,000 kilometers in diameter, large enough for the entire Earth to contain it. Jupiter's Great Digging Red Spot and other storms are primarily driven by a combination of intense heat transport from the gas giants, rapid rotation, and gas instability.

Jupiter's storms are very active, and new storm phenomena often appear on the surface.

There is also a great deal of storm activity on Saturn, the most famous of which is the Great White Spot. The Great White Spot is a huge storm system that appears every 30 years or so and can last for months or even a year. The Great White Spot is smaller in scale than Jupiter's Great Red Spot, but the wind speed is faster, reaching 500 meters per second.

Saturn's storms, like Jupiter's, are driven by a combination of heat transport, rapid rotation, and gas instability.

Overall, storms on Saturn may be more intense than those on Jupiter in terms of wind speed. However, in terms of duration and scale, Jupiter's Great Red Spot prevails. The storms of both planets are very unique and intense weather phenomena with their own characteristics.

The North Pole hexagonal storm of Saturn that we have learned, he is actually the hexagonal storm circle found over Saturn's Beijing, because this storm circle rotates at the same speed as Saturn, and its width is more than 32,190 kilometers, although the reason for the formation of this hexagonal storm has not been finally figured out until now, but I think it may actually be related to thermal convection, and, because such thermal convection is actually not mysterious, we can easily replicate it through experiments, which is very famous thermodynamic Bernal— Rayleigh convection.

Saturn is actually one of the eight planets in the solar system, so although it is no different from other planets, however, Saturn's unique planet has also left a deep impression on countless people, and recently, when Saturn moved to the closest position to Earth, the United States also released the latest Saturn taken by the Hubble Space Telescope this year**, **It is also very beautiful. In fact, this Saturn's ** not only shows us the recent appearance of Saturn's rings, but also brings great scientific value to astronomers.

This also helps astronomers understand the atmospheric dynamics and evolution of the gas giants in the solar system, in which the Hubble Space Telescope not only captures the details of Saturn's rings, but also records Saturn's atmospheric dynamics. More remarkably, however, the Hubble Space Telescope's photographs of Saturn** over the past two years have shown that the magical hexagonal storm at Saturn's North Pole is still raging as before.

In fact, this magical hexagon was discovered as early as 1981, but as for the cause and mechanism of this strange storm, according to the above, no one knows what the cause is, in fact, we can see from the comparison of the rings of two Saturns, and in the last two years, a major storm in the North Pole region of Saturn has disappeared, in addition, there has been a subtle change in the color of the banded structure in Saturn's atmosphere.

The question of what Saturn's hexagonal storm is like and how it formed is explained here today.

Causes of the formation of hexagonal storms: There are 6 vortices around the hexagonal storm, and the vortices squeeze against each other to form hexagons.

Saturn, the windiest planet in the solar system, is surrounded by mysterious rings. The fastest winds on Saturn can reach more than 1,000 miles per hour. A Saturn storm begins with a large dark cloud, about the size of Earth.

Saturn storms are found in both the northern and southern hemispheres, but the most intense storms occur near the equator. On July 22, 2012, a U.S. spacecraft photographed a powerful storm over Saturn, which lasted for about 200 days.

Three months before arriving at Saturn, the Cassini Saturn probe witnessed the whole process of two large storms on Saturn's surface and merging into one large storm, which is the second time that humans have seen this phenomenon on this ringed planet.

The two storms, which are about 1,000 kilometers in diameter, are moving westward relative to the rotation of Saturn's interior, and after about a month, they merge into a new major storm on March 19 and 20, 2004.

The storm to the north moved about twice as fast as the storm to the south, at 11 m-s and 6 m-s, respectively. They are like two cars on a highway chasing each other and spinning in a counterclockwise direction during the merger. This is exactly the opposite direction of rotation of hurricanes in the Southern Hemisphere of the Earth.

On 20 March, shortly after the merger, the newly formed storm was elongated in a north-south direction, with bright clouds at each end. Two days later, the shape of the new storm became more and more rounded, and the original two cloud spots spread out into a halo.

On November 27, storm swirls appeared near Saturn's North Pole, which was captured by NASA's Cassini probe about 400,000 kilometers away.

The Cassini probe captured cyclone-like storms at Saturn's polar regions, which can only be observed in the infrared band due to the darkness of Saturn's long winter North Pole. As Saturn slowly orbits the Sun, the light will eventually reach Saturn's North Pole.

The Cassini probe was launched in 1997 and has been orbiting the Saturn system since 2004.