Skip to main content

Scientists Discover Way to Send Information into Black Holes Without Using Energy

3 comments

First Close Pair of Supermassive Black Holes Discovered

The universe is full of mysteries, but few are as fascinating as supermassive black holes—giant objects that sit at the centers of galaxies and shape their evolution. Now, scientists have made an extraordinary discovery: for the first time, they have found a very close pair of supermassive black holes orbiting each other, possibly on the verge of merging. This breakthrough could transform our understanding of how galaxies grow and evolve over time.

A Rare Discovery in a Distant Galaxy

The discovery was made in a galaxy called Markarian 501, located in the constellation Hercules. A research team led by Silke Britzen from the Max Planck Institute for Radio Astronomy carefully studied this galaxy using high-resolution radio observations collected over more than 20 years.

What they found was surprising. Instead of just one supermassive black hole at the center, there appears to be a pair of them—extremely close to each other and moving in a tight orbit. This is likely the first time scientists have detected such a close system that may soon merge into a single, even more massive black hole.

Why Supermassive Black Holes Matter

Almost every large galaxy, including our own Milky Way, is believed to host a supermassive black hole at its center. These objects can be millions or even billions of times more massive than the Sun.

However, one big question has puzzled scientists for years: how do these black holes grow so large?

Simply collecting gas and dust from their surroundings—known as accretion—is not enough to explain their enormous size within the age of the universe. Scientists believe that mergers between black holes play a key role. When galaxies collide, their central black holes eventually come together, forming a binary system before merging into one.

The Clue: Powerful Jets of Energy

The key to this discovery lies in the powerful jets of particles emitted by black holes. These jets travel at nearly the speed of light and can be observed using radio telescopes.

In the case of Markarian 501, scientists observed not one but two jets coming from the galaxy’s core. This was the first clear sign that something unusual was happening.

One jet was already known and points almost directly toward Earth, making it appear very bright. The second jet, however, is oriented in a different direction, which made it harder to detect. Thanks to long-term observations, researchers were able to identify and track this second jet over time.

A Cosmic Dance

As scientists analyzed the data, they noticed something remarkable: the second jet appeared to move in a repeating pattern. It starts behind the larger black hole and moves around it in a counterclockwise direction.

This motion suggests that the two black holes are orbiting each other—engaged in a cosmic dance.

Further analysis revealed that the pair completes one orbit approximately every 121 days. For objects of such enormous mass, this is incredibly fast. The distance between them is also surprisingly small—just a few hundred times the distance between Earth and the Sun.

In astronomical terms, this is extremely close.

A Glimpse of Gravitational Lensing

In June 2022, scientists observed something even more unusual: the radiation from the system appeared as a ring. This phenomenon, known as an Einstein ring, occurs when light is bent by a massive object due to gravity.

In this case, the light from one jet was bent by the gravity of the black hole in front of it, creating a ring-like appearance. This provided strong evidence that two black holes are indeed present in the system.

Why This Discovery Is Important

This finding is significant for several reasons:

  • First Close Pair Detection: While scientists have long believed that supermassive black holes merge, direct evidence of a very close pair has been missing—until now.

  • Understanding Galaxy Evolution: This system provides a real example of how galaxies grow through mergers.

  • Testing Theories: Current models struggle to explain the final stages of black hole mergers. This discovery offers valuable data to improve those models.

A Countdown to Collision

One of the most exciting aspects of this discovery is that the two black holes may merge relatively soon—possibly within the next 100 years.

Although this is a very short time in cosmic terms, the event will still not be directly visible from Earth due to the enormous distance between us and Markarian 501.

Even powerful instruments like the Event Horizon Telescope, which captured the first images of black holes, are not capable of resolving the two objects separately in this system.

Listening to the Universe: Gravitational Waves

Even if we cannot see the merger directly, scientists may still be able to detect it through gravitational waves.

These are tiny ripples in space-time produced by massive objects in motion, especially during events like black hole mergers. As the two black holes spiral closer together, they are expected to emit gravitational waves at very low frequencies.

These signals could be detected using pulsar timing arrays—networks of highly precise cosmic clocks.

Interestingly, recent studies in 2023 have already found evidence of a background of gravitational waves, possibly produced by many merging black hole pairs across the universe. The system in Markarian 501 could become a key target for linking these signals to a specific source.

A New Era in Astronomy

This discovery opens an exciting new chapter in astronomy. For the first time, scientists have a strong candidate for a supermassive black hole pair that is not just orbiting—but potentially about to merge.

By continuing to observe this system, researchers hope to learn more about:

  • How black holes interact in close pairs

  • How gravitational waves are produced in such systems

  • How galaxies evolve through mergers

In the coming years, this cosmic dance could provide one of the most detailed insights ever into one of the universe’s most powerful and mysterious events.

Final Thoughts

The detection of a close pair of supermassive black holes in Markarian 501 is more than just a scientific milestone—it is a glimpse into the dynamic and ever-changing nature of the universe.

It reminds us that even in the vast emptiness of space, dramatic events are constantly unfolding. And with each new discovery, we move one step closer to understanding the hidden forces that shape the cosmos.

Reference: S Britzen, H Olivares, Gopal-Krishna, F Jaron, I N Pashchenko, E Kun, F K Schinzel, J Becerra González, D Paneque, N R MacDonald, Detection of a second jet within the nuclear core of Mrk 501, Monthly Notices of the Royal Astronomical Society, 2026;, stag291, https://doi.org/10.1093/mnras/stag291

Comments

Post a Comment

Popular

Scientists Discover Way to Send Information into Black Holes Without Using Energy

For years, scientists believed that adding even one qubit (a unit of quantum information) to a black hole needed energy. This was based on the idea that a black hole’s entropy must increase with more information, which means it must gain energy. But a new study by Jonah Kudler-Flam and Geoff Penington changes that thinking. They found that quantum information can be teleported into a black hole without adding energy or increasing entropy . This works through a process called black hole decoherence , where “soft” radiation — very low-energy signals — carry information into the black hole. In their method, the qubit enters the black hole while a new pair of entangled particles (like Hawking radiation) is created. This keeps the total information balanced, so there's no violation of the laws of physics. The energy cost only shows up when information is erased from the outside — these are called zerobits . According to Landauer’s principle, erasing information always needs energy. But ...
3 comments
Read more

Black Holes That Never Dies

Black holes are powerful objects in space with gravity so strong that nothing can escape them. In the 1970s, Stephen Hawking showed that black holes can slowly lose energy by giving off tiny particles. This process is called Hawking radiation . Over time, the black hole gets smaller and hotter, and in the end, it disappears completely. But new research by Menezes and his team shows something different. Using a theory called Loop Quantum Gravity (LQG) , they studied black holes with quantum corrections. In their model, the black hole does not vanish completely. Instead, it stops shrinking when it reaches a very small size. This leftover is called a black hole remnant . They also studied something called grey-body factors , which affect how much energy escapes from a black hole. Their findings show that the black hole cools down and stops losing mass once it reaches a minimum mass . This new model removes the idea of a “singularity” at the center of the black hole and gives us a better ...
Post a Comment
Read more

How Planetary Movements Might Explain Sunspot Cycles and Solar Phenomena

Sunspots, dark patches on the Sun's surface, follow a cycle of increasing and decreasing activity every 11 years. For years, scientists have relied on the dynamo model to explain this cycle. According to this model, the Sun's magnetic field is generated by the movement of plasma and the Sun's rotation. However, this model does not fully explain why the sunspot cycle is sometimes unpredictable. Lauri Jetsu, a researcher, has proposed a new approach. Jetsu’s analysis, using a method called the Discrete Chi-square Method (DCM), suggests that planetary movements, especially those of Earth, Jupiter, and Mercury, play a key role in driving the sunspot cycle. His theory focuses on Flux Transfer Events (FTEs), where the magnetic fields of these planets interact with the Sun’s magnetic field. These interactions could create the sunspots and explain other solar phenomena like the Sun’s magnetic polarity reversing every 11 years. The Sun, our closest star, has been a subject of scient...
Post a Comment
Read more