Scientists confirm Jupiter

In 2020, a group of scientists reached an explanation of the strange contradictions in the upper atmosphere of Jupiter. They suggested that the improved mushballs to rain with ice during severe thunderstorms on the giant of the gas. However, at the time, the idea of ​​Slushee stones full of ammonia was very strange to be real, so they spent the next few years in an attempt to prove that it was wrong.

But Jupiter cannot be denied. A new research confirmed that the strange phenomenon is not only – it can occur on all the gas planets of the solar system.

In modernity The resultThe reported in the magazine of Science Advances, Planetary scientists at the University of California, UC Berkelegi confirmed that prominent storms of MushBalls, accompanied by fierce bitterness, spoke on Jupiter. The balls – the celestial bodies of ammonia and water covered in a solid crust of water ice – turns into a deeper layers of Jupiter, mixing from their atmosphere.

A postgraduate student at the University of California at Berkeley Chris Madele and Professor of Astronomy Emo de Patter participated in the composition of the study, which is currently undergoing the look of the peers. They admit that they initially believed that the theory was very complicated so that it was not real. “There is no way in the world, this is true,” said Muen. statement. “You should actually gather things to explain this, this seems very strange. I mainly spent three years in an attempt to prove this error. I couldn’t prove it wrongly.”

Jupiter is famous for the stormy weather, which is characterized by hurricanes, reasonable anti -storms, and the columns rich in ammonia that swallow the planet. The planet’s atmosphere is primarily consisting of hydrogen and helium gas with small amounts of ammonia and water.

Violent storms inside the turbulent Jupiter atmosphere generate mushballl balls and shallow lightning, according to the new research. These MushBalls are created by thunderstorms, which are about 40 miles (64 km) under the peaks of Jupiter Cloud. The clouds of thunderstorms carry a watery snow along the way to the high altitudes that are sometimes over the visible layer of clouds. Once they are on top, ammonia works like freezing, ice melting and combining it, and ultimately forms a watermelon liquid filled with water ice, creating a saving ball.

The idea of ​​MushBalls was presented for the first time as the interpretation of the Jovian puzzle that has long been controlled: Why ammonia is missing from the atmosphere of Jupiter. According to the paper, the mushballl rises by air until it becomes very heavy and retreats until it evaporates. By doing this, Mushballs redistributes ammonia and water from the upper atmosphere to the deep layers below the clouds, creating areas of exhausted ammonia that are visible in the radio notes of Jupiter.

“So you have, basically, this strange system that is operating below the deck of the cloud, walks along the road to the top of the atmosphere and then drowns deep in the planet,” Mail said. This chemical composition of the surfaces of the clouds does not necessarily reflect the deeper composition in Jupiter’s atmosphere.

The researchers behind the study invented the first three -dimensional perception of the upper planet’s atmosphere, which confirmed that Mushbals exists. In fact, cardiac deterrent storms can be found on other giant planets such as Saturn, Uranus and Neptune.

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Using notes of the microwave radiation scale in the Juno spacecraft, a very large group, and the Hubble Space Telescope, the researchers enables the weather to explore the depth of the weather and its effect on Jupiter. The 3D perception showed that although the majority of weather systems on Jupiter are shallow, with about 6 to 12 miles (from 10 to 20 km) below the surface of the planet’s visible cloud, other weather events go much deeper into the Jupiter layer. “Every time you look at Jupiter, it is often just the level of the surface,” said Mcéun. “It is shallow, but some things – storms and large colors – can merge.”

The study concluded that shallow weather events on Jupiter cannot explain the deeper part of the ammonia of Jupiter’s atmosphere. Instead, the interaction between wide -ranging events, such as columns and swirls, may be along with a phenomenon across storms, such as prominent storms in Mushbal, responsible for the exhaustion of Jupiter’s atmosphere.

Mondolence said that the tasks that were sent to Jupiter and other distant planets of the solar system can only see the upper atmosphere, which are in fact a very bad actor of what is on the planet. But these results show that although the top appears to be boiling, there is a very fixed and slowdown layer. “