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

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Webb Telescope Discovers a Giant Galaxy That Doesn’t Spin

 In the vast and mysterious universe, galaxies are expected to follow certain rules. One of the most basic is that they spin. From elegant spiral galaxies to massive elliptical ones, rotation is considered a natural outcome of how galaxies form and evolve. But now, scientists using the powerful James Webb Space Telescope have discovered something that challenges this long-held idea—a massive galaxy that doesn’t spin at all.

This surprising discovery is forcing astronomers to rethink how galaxies formed in the early universe and whether current theories are complete.

A Strange Discovery in the Early Universe

The galaxy, named XMM-VID1-2075, formed less than 2 billion years after the Big Bang. In cosmic terms, that’s incredibly early. At this stage, galaxies are expected to still be forming and actively rotating due to the motion of gas and matter falling into them.

However, when researchers studied this galaxy using the James Webb Space Telescope, they found something unexpected—it showed no signs of rotation.

This is highly unusual because galaxies typically gain spin during their formation. Gas flows inward, gravity pulls matter together, and this process naturally creates angular momentum, causing the galaxy to rotate. Seeing a galaxy without this motion, especially so early in time, is like finding a hurricane that isn’t spinning.

What Scientists Expected vs. What They Found

According to current models of galaxy formation, rotation begins early and continues throughout a galaxy’s life. Over billions of years, galaxies may collide and merge with others. These interactions can sometimes disrupt or even cancel out their rotation.

But here’s the key point: this process is believed to take a very long time.

That’s why finding a non-rotating galaxy in the early universe is so surprising. It suggests that something unusual happened much faster than expected.

Lead researcher Ben Forrest and his team were intrigued. Their observations revealed that instead of spinning in an organized way, the stars in this galaxy move randomly in different directions. This behavior is typically seen only in large, old galaxies much closer to Earth—not in young ones.

A Giant That Grew Up Too Fast

What makes this discovery even more fascinating is the size and maturity of the galaxy. XMM-VID1-2075 is not just any galaxy—it is extremely massive, containing several times more stars than our own Milky Way.

Even more surprising, it has already stopped forming new stars. This means it evolved very quickly, reaching a mature state in a short amount of time.

To better understand it, scientists compared this galaxy with others from the same period. While one galaxy showed clear rotation and another had an irregular structure, XMM-VID1-2075 stood out as completely different—no rotation, but strong random stellar motion.

This combination makes it what astronomers call a “slow rotator,” a type of galaxy that usually forms much later in the universe’s history.

How Can a Galaxy Stop Spinning?

The big question is: how did this happen?

One leading idea involves a dramatic cosmic collision. If two galaxies spinning in opposite directions collide, their motions could cancel each other out. This would result in a galaxy with little to no overall rotation.

There is some evidence supporting this theory. Scientists observed an unusual excess of light on one side of the galaxy, which could indicate the presence of another object interacting with it. This suggests that a major collision may have played a role in shaping its current state.

Unlike the gradual process of multiple mergers over billions of years, this scenario involves a single, powerful event that rapidly changed the galaxy’s structure.

The Role of Advanced Technology

Discoveries like this would not have been possible without the James Webb Space Telescope. Its advanced instruments allow scientists to study distant galaxies in incredible detail, even those formed billions of years ago.

Previously, such detailed observations were limited to nearby galaxies because distant ones appear too small and faint. But Webb has changed that, opening a new window into the early universe.

It allows astronomers to track how stars and gas move within galaxies, helping them understand their internal dynamics. This is exactly how researchers were able to detect the lack of rotation in XMM-VID1-2075.

What This Means for Our Understanding of the Universe

This discovery raises important questions about our understanding of galaxy formation.

Are non-rotating galaxies more common in the early universe than we thought?
Or is this galaxy a rare exception?

Some computer simulations have predicted that a small number of such galaxies could exist early on, but they were expected to be extremely rare. Finding one like this provides an opportunity to test those predictions.

If more spinless galaxies are discovered, scientists may need to revise current theories. It could mean that galaxies can evolve much faster and more violently than previously believed.

The Search Continues

Researchers are now actively searching for more galaxies like XMM-VID1-2075. By comparing real observations with simulations, they hope to understand how common these objects are and what processes create them.

Each new discovery helps refine our understanding of the universe’s history and the forces that shape it.

A New Cosmic Puzzle

The universe has always been full of surprises, and this discovery is a perfect example. A massive galaxy that doesn’t spin challenges one of the most basic assumptions in astronomy.

It reminds us that even with advanced technology and detailed theories, there is still much we don’t know.

As scientists continue to explore the cosmos with tools like the James Webb Space Telescope, we can expect more discoveries that push the boundaries of our understanding.

And perhaps, somewhere out there, more galaxies are quietly defying the rules—waiting to be found.

Reference:

  1. Ben Forrest, Adam Muzzin, Danilo Marchesini, Richard Pan, Nehir Ozden, Jacqueline Antwi-Danso, Wenjun Chang, M. C. Cooper, Adit H. Edward, Percy Gomez, Lucas Kimmig, Brian C. Lemaux, Ian McConachie, Allison Noble, Rhea-Silvia Remus, Stephanie M. Urbano Stawinski, Gillian Wilson, M. E. Wisz. A massive and evolved slow-rotating galaxy in the early Universe. Nature Astronomy, 2026; DOI: 10.1038/s41550-026-02855-0

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