Astronomers observed a massive star in the Andromeda galaxy (M31-2014-DS1) that gradually faded and almost completely disappeared without producing the expected supernova explosion. The star's core collapsed under gravity when nuclear fuel ran out, but the resulting shock wave was too weak to destroy the star, causing most of the material to fall back inward and form a black hole instead of exploding. This 'failed supernova' phenomenon explains how stars can vanish without the dramatic explosion typically associated with their death, and suggests that many black holes may have formed silently throughout the universe without being detected.
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NASA Watched a Star Vanish From Andromeda Galaxy
Added:Imagine looking at the North Star one night, and discovering that it is gone.
No explosion, no warning, just an empty point in the sky where it had always been.
Scientists have now observed something remarkably similar in extraordinary detail.
For years, multiple telescopes followed a massive star in the Andromeda galaxy, recording how it changed, faded, and eventually almost completely disappeared.
No one saw anything destroy it.
Yet, something faint was still glowing where the star had been. So, how does a massive star simply disappear?
In this video, we will reconstruct the observations, investigate what remained behind, and uncover what truly happened.
Let's get started.
This star's disappearance was not the first strange thing astronomers noticed.
Years earlier, before it faded from view, M31-2014-dES1 had begun glowing more strongly in infrared light.
At the time, it did not look like a warning. There was no violent flash, no explosion, nothing dramatic enough to suggest that one of Andromeda's brightest stars was approaching its final moments.
Then, around 2016, its light began to collapse.
The star did not dim briefly and recover, it kept fading.
Astronomers returned again and again, comparing newer observations with older images.
Each time, the same object appeared weaker.
Eventually, the brilliant star that had once occupied that location was almost impossible to detect.
But, the location was not completely dark. A faint infrared glow remained.
That immediately suggested a possible answer.
The star may have released a cloud of dust around itself.
Dust can block visible light, making even a powerful star disappear from ordinary telescopes while still allowing its heat to appear in infrared observations.
Perhaps the mystery was simple. The star had not vanished. It was merely hidden.
But when astronomers measured the remaining glow, that explanation began falling apart. The source was not just obscured. It had lost most of its total brightness. If the original star were still shining behind the dust, its enormous energy should still be escaping somehow. It was not.
The cloud could explain why the star was difficult to see. It could not explain why the star's power had almost disappeared with it. And that left astronomers facing a far more disturbing question.
Was something still hiding inside the dust? Or was the dust all that remained?
The dust had hidden the center, but it had not solved the mystery.
So, astronomers brought in the most powerful infrared telescope ever built.
When the James Webb Space Telescope examined the exact location of the vanished star, it found that the area was not empty.
A faint, extremely red source remained buried inside a shell of gas and dust.
But it did not look like the massive star that had once been there.
Webb also detected material moving outward from the center. Something had pushed part of the star into space, but the debris was moving far more gently than material thrown out by a normal stellar explosion.
That created a new possibility.
Perhaps the star had survived some violent event and was now hidden inside the debris.
Or perhaps it had merged with another star, producing the dust while leaving behind a single, altered object. Both explanations could account for the material surrounding the source.
But neither could easily explain how weak the center had become.
Whatever remained was producing only a small fraction of the energy released by the original star.
Then astronomers searched for another clue.
NASA's Chandra X-ray Observatory looked toward the same location searching for high-energy radiation from the hidden center.
It found nothing powerful enough to identify what was there.
Now the mystery had become even sharper.
The original star was gone. A faint source remained. Material had been expelled, but there had been no normal explosion.
And the hidden center was almost completely silent.
The question was no longer whether the star was simply covered by dust. It was whether anything recognizable as the original star still existed.
To answer that, scientists had to reconstruct the final event inside its core.
And what they discovered was that the missing explosion had not been overlooked. It had tried to happen and failed.
The star's final battle lasted only seconds. Deep inside its core, nuclear fuel had run out. The pressure holding the star up collapsed, and gravity pulled the core inward with enormous force.
Normally, that collapse launches a shock wave powerful enough to tear the star apart in a supernova.
But this time, the shock began moving outward and then weakened.
It could not carry enough energy through the star.
Only some of the outer material escaped.
The rest slowed, turned around, and began falling back toward the collapsed core.
More matter poured inward.
>> [music] >> The core became heavier, denser, and impossible to support.
Then it crossed the final limit.
The missing star had become a black hole.
This was not a black hole arriving from somewhere else and swallowing the star.
The star created the black hole from within.
Astronomers call this a failed supernova. The core collapses, but the explosion never becomes strong enough to destroy the star in the brilliant flash normally expected. That is why no spectacular supernova appeared in Andromeda.
Most of the star fell inward, while only a small amount of material escaped into space.
The brilliant object astronomers had watched for years was replaced by an invisible black hole surrounded by faint debris.
The leading model suggests that the vanished star produced a black hole with around five times the mass of the sun.
Researchers are still testing whether a deeply hidden surviving star or a stellar merger could explain every clue.
But the continuing loss of energy and the weak ejection make black hole formation the strongest explanation.
And this changes the way astronomers must search for newborn black holes.
A normal supernova suddenly adds a bright object to the sky.
A failed supernova removes one.
If this type of collapse happens often, many black holes may already have been born without anyone noticing, hidden not behind spectacular explosions, but inside old telescope images where a star was visible one year and gone the next.
Astronomers had been waiting for the sky to light up. But the real signal was a star going dark.
The star did not explode. It simply disappeared and left a black hole behind.
And if this happened once, it may have happened many times without anyone noticing.
>> Mhm.
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