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breweries limited (507526) been underperforming recently ✌️【Investment】✌️ Free access to stock market forums, expert advice, and real-time data to help you stay informed and grow your investments. Sign up for 【 - Free Wealth-Building Investment Strategies 】’s Wonder Theory science newsletter.Explore the universe with news on fascinating discoveries, scientific advancements and more.

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breweries limited (507526) been underperforming recently ✌️【Investment】✌️ Free stock market analysis and data updates to help you select the best investment portfolio. Achieve steady growth and avoid losses with expert predictions and real-time market insights. The massive hot gas bubbles are 75 times the size of the sun, and they appear to be sinking down into the star’s interior more rapidly than expected, according to a team of astronomers at Chalmers University of Technology in Sweden.

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In about 5 billion years, our sun will become a red giant, puffing up and expanding as it releases layers of material and likely evaporating the solar system’s inner planets, although Earth’s fate remains unclear, according toNASA.

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“We aimed to observe the gas in the atmosphere around the star and hoped to find signs of the ‘convection’ bubbles that were expected to exist,” said lead study author Wouter Vlemmings, a professor of astronomy and plasma physics at Chalmers, in an email. “However, we did not expect to see them in such detail and to actually be able to see their movement.”

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Energy produced in the core can be delivered to the star’s surface through huge, hot bubbles of gas, which then sink as they cool down, similar to what happens in a lava lamp.

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breweries limited (507526) been underperforming recently ✌️【Investment】✌️ Real-time stock and futures data, backed by expert stock market trend predictions, to help you make timely and profitable investment decisions. When a star’s life ends, it runs out of hydrogen to convert into helium, causing the star’s core to collapse. This pressure on the core also increases the star’s temperature, which causes it to puff up and swell into a red giant, according toNASA.

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“We are all made of ‘stardust,’ and much of the material around us is made in stars,” Vlemmings said. “How this material is ejected from old stars to be incorporated in new stars and planets is still not completely clear.”

breweries limited (507526) been underperforming recently ✌️【Investment】✌️ Real-time stock market data, precise predictions, and investment strategies to help you optimize your portfolio and achieve financial success. The team decided to observe R. Doradus because it’s one of the nearest and largest red giant stars, making it easier to watch. The telescope enabled them to collect high-resolution images of the star’s surface over the course of a month.

“Convection creates the beautiful granular structure seen on the surface of our Sun, but it is hard to see on other stars,” said study coauthor Theo Khouri, a researcher at Chalmers, in a statement. “With ALMA, we have now been able to not only directly see convective granules — with a size 75 times the size of our Sun! — but also measure how fast they move for the first time.”

breweries limited (507526) been underperforming recently ✌️【Investment】✌️ Free expert predictions on stock trends and real-time data to help you make informed decisions and grow your wealth steadily. The sun’s outermost layer, called the photosphere, is made of gas so hot that it bubbles. The sun’s photosphere is full of millions of bubbles formed through convection. The gas bubbles, also known as convective granules, are about 621 miles (1,000 kilometers) across and move at speeds of a few kilometers per second, so they only survive for about 10 minutes.

But the convective cells on R. Doradus’ surface are more than 100 million kilometers (about 62 million miles) in size, with velocities of a few tens of kilometers per second, and persist for about a month.

“We don’t yet know what is the reason for the difference. It seems that convection changes as a star gets older in ways that we don’t yet understand,” Vlemmings said.

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“It is spectacular that we can now directly image the details on the surface of stars so far away, and observe physics that until now was mostly only observable in our Sun,” said study coauthor Behzad Bojnordi Arbab, a doctoral student at Chalmers, in a statement.

breweries limited (507526) been underperforming recently ✌️【Investment】✌️ Expert stock predictions and free stock selection services to help you achieve optimal returns and long-term growth. The new study includes longer observations than previous ones, which captured the evolution of the bubbles, said Dr. Claudia Paladini, associate astronomer at the European Southern Observatory in Chile. Paladini authored a study on the observation ofbubbles on the surface of the star pi1 Gruis. While she was not involved in the new research, she authored an article that accompanies the study in Nature.

“One can see the bubbles coming up, expanding, and vanishing like it’s seen in the Sun. It’s remarkable considering the distance we are talking about,” Paladini said. “Now we just need to observe many more of these stars!”

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