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Astronomers Spot Galaxies Moving in Sync Across a 50 Million Light Year Stretch

Astronomers Spot Galaxies Moving in Sync Across a 50-Million-Light-Year Stretch

Astronomers have identified a rare 50-million-light-year cosmic filament in which 14 galaxies spin together.

Written by Gadgets 360 Staff | Updated: 5 December 2025 21:31 IST

Astronomers Spot Galaxies Moving in Sync Across a 50-Million-Light-Year Stretch

Photo Credit: Lyla Jung

An illustration showing the cosmic web on the left, and a zoom in on the filament in question in middle

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Highlights

Galaxies found rotating in sync along a vast cosmic filament
Alignment challenges standard models of galaxy spin formation
Filament offers rare view of early cosmic flow and evolution

Scientists‍‌‍‍‌‍‌‍‍‌ from across the globe have discovered one of the largest rotation systems in the cosmos: a 50-million-light-year-long cosmic filament with a chain of galaxies all spinning together. The 5.5 million light-year line of the cosmic filament, made up of dark matter and gas, is home to 14 gas-rich galaxies. The team followed the galaxies' movement and saw that the galaxies were all rotating along with the filament. The paper published in MNRAS today, the findings, changes the galaxy evolution models that are most widely ‍‌‍‍‌‍‌‍‍‌accepted.

Discovery of a Giant Spinning Filament

According to the paper, astronomers‍‌‍‍‌‍‌‍‍‌ have mapped a huge dark matter filament filled with galaxies about 140 million light years away. In the 50 million light-year structure, the team found 14 hydrogen-rich galaxies arranged in a 5.5 million light year chain. Incredibly, all these galaxies spin in the same direction as the filament, which is a lot of alignment for it to be just a coincidence. Galaxies on the far sides of the filament are going in opposite directions, which suggests the whole filament is ‍‌‍‍‌‍‌‍‍‌spinning.

JWST Spots an Exoplanet Losing Its Atmosphere in a Huge Helium Stream

How Galaxies Gain Their Spin

This rotating filament offers a rare window into galaxy evolution. The filament appears young and “dynamically cold” – its galaxies are gas-rich, star-forming and moving slowly. Astronomers describe it as a “fossil record” of cosmic flows, which could reveal how angular momentum flows from the large-scale web into individual galaxies.

Such strong alignment was not predicted by existing models, so researchers hope to refine simulations of cosmic structure formation using this data.

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