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Space Science

Death Throes of Red Supergiant Star Observed In Real Time (cnn.com) 47

"For the first time, astronomers were able to observe the death throes of a red supergiant star in real time," writes Slashdot reader quonset from a report via CNN. "The fortuitous event came about when astronomers were first alerted in the summer of 2020 by a release of bright radiation detected by the University of Hawaii Institute for Astronomy Pan-STARRS telescope on Maui's Haleakal. Then, In the fall, astronomers witnessed a supernova form in the same spot." From the report: Before they go out in a blaze of glory, some stars experience violent eruptions or release glowing hot layers of gas. Until astronomers witnessed this event, they believed that red supergiants were relatively quiet before exploding into a supernova or collapsing into a dense neutron star. Instead, scientists watched the star self-destruct in dramatic fashion before collapsing in a type II supernova. This star death is the rapid collapse and violent explosion of a massive star after it has burned through the hydrogen, helium and other elements in its core. All that remains is the star's iron, but iron can't fuse so the star will run out of energy. When that happens, the iron collapses and causes the supernova. A study detailing these findings published Thursday in The Astrophysical Journal.

"It's like watching a ticking time bomb," said senior study author Raffaella Margutti, an associate professor of astronomy and astrophysics at UC Berkeley, in a statement. "We've never confirmed such violent activity in a dying red supergiant star where we see it produce such a luminous emission, then collapse and combust, until now." Some of these massive stars likely experience consequential internal changes that cause the tumultuous release of gas before they die, the finding has shown.

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Death Throes of Red Supergiant Star Observed In Real Time

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  • Red Supergiant (Score:1, Offtopic)

    by cstacy ( 534252 )

    Red supergiant? Something happened to Xi Jinping?

  • I want to know if LIGO saw anything.

    • Darn the luck, LIGO was busy looking for gravitational waves at the time.
      • Yeah, I expect so, but:

        https://astronomy.stackexchang... [stackexchange.com]

        Unless the star is quite symmetrical, it could produce GWs.

        • by necro81 ( 917438 )

          Unless the star is quite symmetrical, it could produce GWs.

          This is probably true. However, for all its incredible precision and sensitivity, LIGO can only spot the waves from much, much more energetic phenomena: the merger of of objects [google.com] with several-to-dozens of stellar masses apiece. The rapid mutual orbits of two stellar-mass objects represent huge displacements and accelerations, creating waves of detectable amplitude. The asymmetric wobbles of a single large star almost certainly do not register, u

  • by AntisocialNetworker ( 5443888 ) on Friday January 07, 2022 @05:14AM (#62151407)

    Not the first by nearly a millenium. The Crab Nebula supernova was observed by Chinese astronomers in 1054. Wikipedia article https://en.wikipedia.org/wiki/... [wikipedia.org].

    • by jabuzz ( 182671 )

      The Chinese astronomers didn't have telescopes. So beyond seeing a bright spot in the sky with mark one eyeballs they didn't make the sort of detailed useful observations that have been made in this instance.

      • by umghhh ( 965931 )

        The Chinese astronomers didn't have telescopes. So beyond seeing a bright spot in the sky with mark one eyeballs they didn't make the sort of detailed useful observations that have been made in this instance.

        The formulation of 'real time' is silly in both cases anyway. The event happened long time ago. The real interesting part is this: if you consider the 'real time' thing in relation to when the light came to us then the actual observation by Chinese 1000ya were done in real time as they observed the light coming in as it passed the earth. What they did in Hawaii is difficult to say as the article in question does not provide such details. but chances are they were making photos and analyzing these with compu

    • by dryeo ( 100693 )

      Were they observing the star that went supernova before it blew? That's what is different with these observations. Seeing supernovas is pretty common with today's telescopes as somewhere one is usually happening, even if billions of light years away.

  • In real time?! (Score:3, Insightful)

    by Gravis Zero ( 934156 ) on Friday January 07, 2022 @06:36AM (#62151507)

    the star at the heart of this new research, located in the NGC 5731 galaxy about 120 million light-years away from Earth

    This happened 120 million years ago!

  • by Klaxton ( 609696 ) on Friday January 07, 2022 @11:06AM (#62152097)

    The paper is here; https://iopscience.iop.org/art... [iop.org]

    This star is very far away of course. It got brighter in the summer of 2020. Then in the fall it went supernova and they got spectrographic data, which showed that there had been large mass ejections beforehand. Apparently this had not previously been seen or expected in a star that size.

    "symmetric emission lines that resulted from the photoionization of circumstellar material (CSM) shed in progenitor mass-loss episodes before explosion. Surprisingly, this novel display of pre-SN emission and associated mass loss occurred in a red supergiant (RSG) progenitor with zero-age main-sequence mass of only 10–12 Me"

    This part is kind of interesting;
    "ejection of stellar material following energy disposition into the stellar envelope as a result of gravity waves emitted during either neon/oxygen burning or a nuclear flash from silicon combustion."

    • I couldn't tell if they meant gravitational waves as in Einstein or gravity waves as in rock thrown in pond. Also, nuclear flash from silicon? Do they mean gamma rays? How would they get out in time?
      • by Klaxton ( 609696 )

        I don't understand that either, maybe someone more knowledgeable can explain.

        The term "silicon combustion" surely means that it is fusing, not burning in the usual sense of the word? But I have seen astronomers use that term in several places, maybe its just convenient.

        As I understand it, the latter stages of the stellar lifecycle can be pretty quick. It takes a long time to fuse the hydrogen into helium in the core, but progressively less time to generate and fuse through the heavier elements. Towards the

  • No it's not. Unless you're orbiting that star. And even then it's just close to real time.

    • You demonstrate a misunderstanding of "Real-Time". It doesn't mean that you are seeing something with no time delay due to the travel of light/radiation, it means that you see the event unfold in the amount of time and the order that it actually happened. Don't be a dumbass.

  • ... or it didn't happen!

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