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We know essentially when these supernovae happen, but we aren’t able to predict exactly when a...
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 <h1> Astronomers develop &#8216 early warning system&#8217  for stars about to go supernova	</h1> By Georgina Torbet October 16, 2022 Share One of the most dramatic cosmic events is a supernova, when a massive star runs out of fuel. The star explodes in an enormous burst of energy that can be seen even in other galaxies.
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Astronomers develop ‘ early warning system’ for stars about to go supernova

By Georgina Torbet October 16, 2022 Share One of the most dramatic cosmic events is a supernova, when a massive star runs out of fuel. The star explodes in an enormous burst of energy that can be seen even in other galaxies.
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We know essentially when these supernovae happen, but we aren’t able to predict exactly when a...
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They include our famous neighbor Betelgeuse. These stars used to be massive stars around eight to 20...
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We know essentially when these supernovae happen, but we aren&#8217;t able to predict exactly when any given star will go supernova. Now, though, a team of astronomers has come up with an &#8220;early warning system&#8221; for stars approaching this critical point. The astronomers from Liverpool John Moores University and the University of Montpellier simulated the development of a group of pre-supernova stars called red supergiants, which are some of the largest stars (though not necessarily the most massive).
We know essentially when these supernovae happen, but we aren’t able to predict exactly when any given star will go supernova. Now, though, a team of astronomers has come up with an “early warning system” for stars approaching this critical point. The astronomers from Liverpool John Moores University and the University of Montpellier simulated the development of a group of pre-supernova stars called red supergiants, which are some of the largest stars (though not necessarily the most massive).
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They include our famous neighbor Betelgeuse. These stars used to be massive stars around eight to 20 times the mass of the sun, but as their fuel runs out, they switch from fusing hydrogen to fusing helium, and they puff up to a larger size while cooling down.
They include our famous neighbor Betelgeuse. These stars used to be massive stars around eight to 20 times the mass of the sun, but as their fuel runs out, they switch from fusing hydrogen to fusing helium, and they puff up to a larger size while cooling down.
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This artist’s impression shows the supergiant star Betelgeuse as it was revealed thanks to differe...
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Calçada The researchers found that these red supergiant stars become suddenly much fainter in their...
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This artist’s impression shows the supergiant star Betelgeuse as it was revealed thanks to different state-of-the-art techniques on European Southern Observatory ’s Very Large Telescope. European Southern Observatory/L.
This artist’s impression shows the supergiant star Betelgeuse as it was revealed thanks to different state-of-the-art techniques on European Southern Observatory ’s Very Large Telescope. European Southern Observatory/L.
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Calçada The researchers found that these red supergiant stars become suddenly much fainter in their last few months of life. Their brightness drops by as much as a hundred times as they produce dusty material that obscures the light they give off, making them appear fainter. This dropping brightness will be a clue to an impending supernova.
Calçada The researchers found that these red supergiant stars become suddenly much fainter in their last few months of life. Their brightness drops by as much as a hundred times as they produce dusty material that obscures the light they give off, making them appear fainter. This dropping brightness will be a clue to an impending supernova.
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“The dense material almost completely obscures the star, making it 100 times fainter in the visible part of the spectrum. This means that, the day before the star explodes, you likely wouldn&#8217;t be able to see it was there,” lead author Benjamin Davies of Liverpool John Moores University explained in a statement. “Until now, we’ve only been able to get detailed observations of supernovae hours after they’ve already happened.
“The dense material almost completely obscures the star, making it 100 times fainter in the visible part of the spectrum. This means that, the day before the star explodes, you likely wouldn’t be able to see it was there,” lead author Benjamin Davies of Liverpool John Moores University explained in a statement. “Until now, we’ve only been able to get detailed observations of supernovae hours after they’ve already happened.
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With this early-warning system, we can get ready to observe them in real time, to point the world’s best telescopes at the precursor stars, and watch them getting literally ripped apart in front of our eyes.” The research is published in the journal Monthly Notices of the Royal Astronomical Society. <h4> Editors&#039  Recommendations	</h4> How to watch this week&#8217;s solar eclipse in person or online Hubble captures a tempestuous pair of Herbig-Haro objects Astronomers spot a monster black hole &#8216;practically in our backyard&#8217; How NASA is building an instrument to withstand the brutal conditions of Venus Here&#8217;s how NASA will drop off a sample of an asteroid NASA&#8217;s Lucy spacecraft swings by Earth on its way to Trojan asteroids Something strange is up with this black hole This oddball pair of stars is producing dust shells like clockwork Heaviest element ever discovered in exoplanet atmospheres is a puzzle NASA asteroid crash left a comet-like trail 6,000 miles long How to watch SpaceX and NASA launch Crew-5 mission today This Mars rover is looking for a new mission Snoopy is heading to space. NASA explains why Watch the highlights of SpaceX&#8217;s Crew-5 launch to space station How to watch SpaceX&#8217;s Crew-5 astronauts arrive at space station Look out, space billboards could be coming to a sky near you Watch four astronauts welcomed to the International Space Station See Jupiter&#8217;s icy moon Europa up close and personal in Juno image
With this early-warning system, we can get ready to observe them in real time, to point the world’s best telescopes at the precursor stars, and watch them getting literally ripped apart in front of our eyes.” The research is published in the journal Monthly Notices of the Royal Astronomical Society.

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