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Ghostly Star Ribbon Reveals Hidden Dark Matter Beyond Milky Way

For billions of years, an ancient cluster of stars has been slowly tearing apart, leaving a faint, narrow ribbon across space. That delicate structure has now become the first stellar stream of its kind ever found beyond the...

For billions of years, an ancient cluster of stars has been slowly tearing apart, leaving a faint, narrow ribbon across space. That delicate structure has now become the first stellar stream of its kind ever found beyond the Milky Way, giving astronomers a new way to probe dark matter.

An international team, including researchers from Northwestern University in the United States, spotted the ghostly ribbon around a distant galaxy. The discovery, published Aug. 12 in the journal Nature, offers a fresh tool for studying the invisible substance that makes up most of the universe's mass.

A Faint Trail That Took Billions of Years to Form

Globular clusters are dense balls of stars held together by gravity. As one of these clusters orbits its host galaxy, the galaxy's gravitational pull can slowly strip stars away. Those stars do not scatter randomly. Instead, they keep moving along nearly the same path, creating long, thin streams that record the gravitational forces they have experienced.

Astronomers have found dozens of such streams inside the Milky Way. But until now, none had been detected in another galaxy. These structures are so faint that they usually vanish against the glow of their host galaxies.

The newly identified stream is the first globular cluster stellar stream ever observed outside our galaxy. Its discovery confirms a long-standing prediction and opens a new window for studying dark matter.

Reading Gravity Through Starlight

By analyzing the stream's shape, the researchers reconstructed the gravitational field of its host galaxy. That allowed them to estimate how much dark matter surrounds the galaxy and how it is distributed.

"The stars in a stellar stream all travel along nearly the same orbit, and that orbit is shaped by the galaxy's gravity," said Tjitske Starkenburg, a coauthor of the study from Northwestern. "By modeling that gravity, we can estimate the galaxy's total mass. We already know roughly how much of that mass comes from visible matter like stars, so the rest must be dark matter."

The study was co-led by Julie Kiel Holm of the University of Copenhagen and Sarah Pearson of the Technical University of Denmark. Starkenburg, an expert in extragalactic astronomy, works at Northwestern's Center for Interdisciplinary Exploration and Research in Astrophysics.

Dark matter remains one of the biggest unanswered questions in astrophysics. It does not emit, absorb, or reflect light, yet it exerts gravity and shapes the motion of galaxies. The new method could eventually help scientists map dark matter across many different galaxies and throughout the universe.

The discovery shows that even the faintest structures in the cosmos can carry profound information. A ribbon of stars, stretched thin over eons, now serves as a measurable trace of the invisible forces that govern galaxies.

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