Black holes continue to “burp” stars they destroyed years before — and astronomers have no idea why

  • Astronomers made the discovery after years of observing black holes
  • Stars involved in tidal disturbances are torn apart within hours

Black holes are among the most talked about objects in the universe, yet scientists still have so much to learn when it comes to understanding their mysterious behavior.

We already know that the notoriously messy eaters will gobble up anything that gets in their way.

But what astronomers didn’t realize was that the cosmic monsters then “ejected” an eclectic mix of stars, gas, planets, and dust that they had destroyed years earlier.

This surprise only came to light when experts decided to monitor black holes for several years after they were involved in tide disruption events (TDEs).

Traditionally, objects have only been studied for a few months after a TDE — what happens when stars get too close to a black hole and are blown to pieces in a process called spaghettiification.

Mysterious: Scientists know that black holes are notoriously messy eaters, devouring everything in their path. What they didn't realize, however, is that the cosmic monsters were

Mysterious: Scientists know that black holes are notoriously messy eaters, devouring everything in their path. What they didn’t realize, however, is that the cosmic monsters were “belching up” a mixture of stars, gas, planets and dust that they had destroyed years earlier (stock image)

What is a “Tidal Disturbance Event”?

When a star gets too close to a black hole, it undergoes “spaghettification,” where it is stretched vertically and compressed horizontally by the strong gravitational field.

These are called tidal disruption events (TDEs) and emit light, radio, and other waves for up to a few weeks or months as they occur.

This is because the elongated material eventually spirals around the black hole and heats up, creating a flash that astronomers can detect millions of light-years away.

Although black holes cannot be observed directly, scientists can observe a TDE because these events emit light, radio, and other waves for up to a few weeks or months as they occur.

In the process, some of the gas and dust left over from a shattered star is ejected from the black hole.

The rest then forms a thin Frisbee-like structure around itself, a so-called accretion disk, which gradually feeds the stellar material towards the black hole.

However, scientists at the Harvard and Smithsonian Center for Astrophysics have found that some of this material can resurface in between two and six years after a TDE.

They found that up to half of the 24 black holes they observed later had “burp” seizures, although they have no idea why.

“If you look years later, a very, very large fraction of these black holes that have no radio emission at this early point in time will actually suddenly ‘turn on’ radio waves,” lead author Yvette Cendes told Live Science.

“I call it a ‘burp’ because we have a kind of lag where this material doesn’t come out of the accretion disk until much later than people expected.”

Although black holes cannot be observed directly, scientists can observe a TDE because these events emit light, radio, and other waves for up to a few weeks or months as they occur

Although black holes cannot be observed directly, scientists can observe a TDE because these events emit light, radio, and other waves for up to a few weeks or months as they occur

The question is, where is it stored before it’s “belched” again?

Scientists know for sure that it’s not coming from inside a black hole, because the objects have an event horizon where gravity is so strong that even light can’t escape.

Cendes added: “We do not fully understand whether the material observed in radio waves originates from the accretion disk or whether it is stored somewhere near the black hole.”

“However, black holes are definitely messy eaters.”

The researchers plan to continue monitoring the black holes they observe, especially as some of them continue to get brighter after TDE.

They are also calling for improved computer modeling to better represent how black holes can “belch” years later, which experts say will improve understanding of this strange behavior.

The new research has been published in the arXiv preprint database but has not yet been peer-reviewed.

WHAT’S IN A BLACK HOLE?

Black holes are strange objects in the universe that get their name from the fact that nothing can escape their gravity, not even light.

If you venture too close and cross what is known as the event horizon, the point where no light can escape, you will also be trapped or destroyed.

With small black holes, you would never survive such a close approach anyway.

The tidal forces near the event horizon are enough to stretch any matter until it’s just a chain of atoms, a process physicists call “spaghettification.”

But for large black holes, like the supermassive objects at the cores of galaxies like the Milky Way, which weigh tens of millions if not billions of times the mass of a star, crossing the event horizon would be uneventful.

Since it should be possible to survive the transition from our world to the world of the black hole, physicists and mathematicians have long wondered what that world would look like.

They turned to Einstein’s equations of general relativity to predict the world inside a black hole.

These equations work well until an observer reaches the center or singularity where, in theoretical calculations, the curvature of spacetime becomes infinite.

Drew Weisholtz

Drew Weisholtz is a Worldtimetodays U.S. News Reporter based in Canada. His focus is on U.S. politics and the environment. He has covered climate change extensively, as well as healthcare and crime. Drew Weisholtz joined Worldtimetodays in 2023 from the Daily Express and previously worked for Chemist and Druggist and the Jewish Chronicle. He is a graduate of Cambridge University. Languages: English. You can get in touch with me by emailing: DrewWeisholtz@worldtimetodays.com.

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