A planet has been discovered outside our solar system, which is no less than hell. The day temperature here is 2000 degrees Celsius. The winds blow very fast. The amount of microscopic iron particles in the air is very high. These particles keep moving up and down rapidly in the atmosphere of this planet. Overall, the weather here is very bad.
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Scientists at Geneva University have discovered a hell-like planet that they could not even imagine. The name of this planet is WASP-76B. The weather here is very bad. There is wind but it blows very fast. There are very high amounts of microscopic iron particles in the air. The day temperature is 2000 degrees Celsius. The surprising thing is that this planet is bound to its star, like our moon. Therefore, strong winds keep blowing around it. The quantity of iron particles on this planet is also high. That means iron particles are present here. Due to high temperatures, they melt during the day and keep falling on the surface of the planet. It is an exoplanet i.e. it can also be called an outer planet.
The planet is external because it is not part of our solar system. Scientists have discovered 5200 exoplanets since 1990. Many of these planets are large, such as Saturn and Jupiter. Some are rocky and some are earthy. But it is not yet known whether they have livable conditions or not. WASP-76b has attracted a lot of attention recently. It is an extremely hot gas planet about 640 light years away from our Earth.
This planet, located towards Pisces, was discovered in the year 2013. It has been studied since then. Its host star is very close to its orbit. It completes one revolution around its star in only 1.8 days. One part of it always remains in light and the other part in darkness. That is why the mercury rises to 2000 degrees Celsius during the day. During the day, here iron particles start floating in the air. But when it is cold at night, iron particles fall from the air and settle on the ground. Recently scientists at Geneva University have discovered iron particles. Got it published in the Astronomy and Astrophysics Journal.
