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Message: <blockquote data-quote="imhotep" data-source="post: 30143602" data-attributes="member: 562115"><a href="https://imgbox.com/p27lFweN" target="_blank"><img src="https://thumbs2.imgbox.com/5c/f4/p27lFweN_t.jpg" alt="" class="fr-fic fr-dii fr-draggable " style="" /></a>Photos taken over a few weeks from 2023-07-18Astronomers 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.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.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 to NASA.The observations, made using the Atacama Large Millimeter/submillimeter Array, or ALMA, of telescopes in Chile, mark the first time researchers have tracked such detailed movements on the surface of a star other than the Sun.“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.”When stars ageVlemmings and his colleagues study what occurs as stars near the end of their lifetimes. 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.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.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 to NASA.As they near the end of their lives, the topmost layers of the stars blow off, and eventually the stars collapse or explode, releasing the elements created inside them into space.“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.”</blockquote>

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