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yuvraaj hygiene products limited (531663) ✌️【Stock Market】✌️ Free stock data analysis to help you select stocks accurately and capture market trends. Astronomers have observed the detailed motions of giant gas bubbles on the surface of a nearby star for the first time, which rise and fall like the inside of a lava lamp.

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yuvraaj hygiene products limited (531663) ✌️【Stock Market】✌️ Precise stock market trend predictions with free real-time quotes for India, US, and European stocks. Whether you're looking for short-term gains or long-term growth, our expert advice ensures you make the best investment choices. The images show the surface of the star R. Doradus, a red giant star 180 light-years away in the Dorado constellation. The star has a diameter about 350 times that of the sun, and it serves as a preview for our sun’s future.

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.”

yuvraaj hygiene products limited (531663) ✌️【Stock Market】✌️ Free stock selection services backed by expert predictions. Our advanced analytics and real-time market data will help you stay ahead of the competition and make smart, profitable investment decisions. Stars produce energy within their cores through nuclear fusion by squeezing hydrogen atoms to form helium. This process heats the star and fuels it for billions of years.

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.

yuvraaj hygiene products limited (531663) ✌️【Stock Market】✌️ Expert market predictions, real-time updates, and personalized investment advice designed to help you succeed. Seize the best investment opportunities in global stocks, metals, and energy markets. This process, known as convection, mixes elements created in the core such as carbon and nitrogen throughout the star, according to the study authors. Convection is also the likely instigator of stellar winds, or rapid winds that can whisk elements made by the star into space to help create new stars and planets.

yuvraaj hygiene products limited (531663) ✌️【Stock Market】✌️ Gain access to professional investment advice, free market trend analysis, and real-time stock market data. Make informed decisions and unlock the full potential of your investments with expert predictions and guidance. 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.”

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“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.”

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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.

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“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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