Previously, it was not understood how long it took the star to accrete this product. For the very first time, researchers have now simulated how red supergiants may look when they are ingrained within these pre-explosion cocoons.
Old telescope archives reveal that images do exist of stars that went on to explode around a year after the image was taken. The stars look like typical in these images, suggesting they can not yet have actually constructed up the theoretical circumstellar cocoon. This recommends that the cocoon is put together in less than a year, which is thought about to be very fast.
Benjamin Davies from Liverpool John Moores University, and lead author of the paper, states “The thick material almost completely obscures the star, making it 100 times fainter in the visible part of the spectrum. This suggests that, the day prior to the star takes off, you likely would not be able to see it was there.” He adds, “Until now, weve only been able to get comprehensive observations of supernovae hours after theyve already taken place. With this early-warning system we can get ready to observe them real-time, to point the worlds best telescopes at the precursor stars, and enjoy them getting literally ripped apart in front of our eyes.”
Reference: “Explosion impending: the appearance of red supergiants at the point of core-collapse” by Ben Davies, Bertrand Plez and Mike Petrault, 13 October 2022, Monthly Notices of the Royal Astronomical Society.DOI: 10.1093/ mnras/stac2427.
Red supergiants are stars of spectral type K or M with a supergiant luminosity class (Yerkes class I). In terms of volume, they are the biggest stars in the universe.
An artists impression of Betelgeuses supernova. Credit: European Southern Observatory/L. Calçada
Astronomers from Liverpool John Moores University and the University of Montpellier have actually designed an early warning system to sound the alert when a huge star is about to end its life in a supernova explosion. The work was released today (October 13, 2022) in Monthly Notices of the Royal Astronomical Society.
In this brand-new research study, private investigators determined that enormous stars (generally in between 8 and 20 solar masses) in the last stage of their lives, the so-called red supergiant stage, will all of a sudden become around a hundred times fainter in noticeable light in the last couple of months before they die. This dimming is triggered by an unexpected build-up of material around the star, which obscures its light.
Red supergiants are stars of spectral type K or M with a supergiant luminosity class (Yerkes class I). Old telescope archives show that images do exist of stars that went on to explode around a year after the image was taken. Benjamin Davies from Liverpool John Moores University, and lead author of the paper, says “The dense material nearly completely obscures the star, making it 100 times fainter in the visible part of the spectrum. With this early-warning system we can get ready to observe them real-time, to point the worlds finest telescopes at the precursor stars, and view them getting literally ripped apart in front of our eyes.”
