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A cosmic breadcrumb trail leads astronomers to a discovery in another galaxy

A faint ribbon of stars in a distant galaxy has led astronomers to a discovery that could reveal secrets about one of our universe's greatest mysteries. Hidden within the Hubble Space Telescope's archival data, researchers found the barely visible trail of stars — the first globular cluster stellar stream detected outside the Milky Way. The […]

By deepak · August 14, 2026 · 4 min read

A faint ribbon of stars in a distant galaxy has led astronomers to a discovery that could reveal secrets about one of our universe's greatest mysteries.

Hidden within the Hubble Space Telescope's archival data, researchers found the barely visible trail of stars — the first globular cluster stellar stream detected outside the Milky Way. The celestial phenomenon, located in a galaxy roughly 115 million light-years from Earth, is the remnant of a dense ball of stars being slowly pulled apart by the gravity of its host galaxy. As the cluster loses stars, the remnants form a long, narrow stream.

Astronomers have found dozens of stellar streams within the Milky Way, but because these trails are faint and hard to detect, many more are likely left to be discovered. Now, with evidence that they occur in other galaxies, astronomers may be able to use them as cosmic tracers to understand better how galaxies form and evolve.

The finding, which was detailed in a study published Wednesday in the journal Nature, also allowed the team of astronomers to map the galaxy — known as UGC 9050-Dw1 — and its gravitational field by modeling the stream.

Because the galaxy's gravity influences the stellar stream's shape and motion, the researchers used the trail of stars to trace the galaxy's gravitational field. Through their modeling, they were also able to estimate the galaxy's total mass, how much of it is made up of visible objects, such as stars, and how much is composed of dark matter — a mysterious form of matter that cannot be seen but has gravity.

When the study team started to realize that it had found a stellar stream beyond our galaxy, "it was very exciting," said co-lead author Julie Kiel Holm, a doctoral fellow at the Niels Bohr Institute at Denmark's University of Copenhagen who studies globular clusters and the formation of stellar streams. "And then we sort of looked at each other and asked, 'Where do we go from here?'"

Dark matter intrigues scientists because they don't know what it is, yet they can see its gravitational influence on stars and galaxies. "About 80% to 85% of our universe, we think is dark matter, so that makes it very, very enticing to try and figure out what it is," Kiel Holm added.

Stellar streams have been used to help scientists map the dark matter within our own galaxy. Now, those same tools can be used to help better understand the dark matter composition and structure of other galaxies that share the universe.

The newly discovered stream is located within an ultra-diffuse galaxy — one that is spread out and extremely faint, which likely made the stellar stream easier to spot, the study authors speculated.

"At the same time, these ultra-diffuse galaxies are thought to be very massive, and you need to be massive in order to actually pull out stars from that parent cluster," said co-lead author Sarah Pearson, an associate professor at DTU Space, the National Space Institute at the Technical University of Denmark.

"So those two things together — the fact that it provides a faint background, but also has a strong enough tidal field to pull out stars from the cluster — is a great combination if you would want to find one of these," she added.

When trying to identify these streams, astronomers look for thin, elongated structures on their telescopes. The streams can also be tracked through their movement along the sky; however, doing so requires a telescope to be in the same position over time, and the technique has so far only been able to find stellar streams in the Milky Way.

"The area that the Hubble can see is actually not that big. So you have to be very, very lucky to be able to see this, and we don't really know where to look to basically target them," said study coauthor Tjitske Starkenburg, a research assistant professor at the Center for Interdisciplinary Exploration and Research in Astrophysics at Northwestern University in Evanston, Illinois.

The study authors predict that future telescope advancements will allow for further detection of these clusters within and outside our galaxy. Starkenburg pointed to NASA's Nancy Grace Roman Space Telescope that is expected to launch at the end of the month and will have a larger field of view, "like 100 Hubbles in one image."

Detecting a faint stellar stream in a galaxy outside the Local Group — our galactic neighborhood that consists of more than 50 galaxies that are gravitationally bound together — is remarkable, David Martínez-Delgado, an astrophysicist and researcher for the nonprofit foundation ARAID at the Center for Studies of the Cosmos Physics of Aragón in Teruel, Spain, said in an email. Martínez-Delgado was not involved with the new study.

Source: Read the original article on www.yahoo.com