Ghostly Trail Of Stars Reveals A New Way To Hunt Hidden Dark Matter
by
Aaron Leong
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Friday, August 14, 2026, 11:01 AM EDT
Hubble Space Telescope image showing the globular cluster stellar stream- Image: HUST / Holm et al.
For the first time, astronomers have discovered a globular cluster stellar stream outside the Milky Way, giving scientists a new way to map invisible dark matter in distant galaxies.
Composite image of HST ACS/WFC F555W and F814W observations of UGC 9050-Dw1 - Image: HUST / Holm et al
Located approximately 115 million light-years from Earth, the faint ribbon of stars was spotted unraveling around UGC 9050-Dw1, an ultra-diffuse galaxy. Ultra-diffuse galaxies contain relatively few stars spread across a vast volume of space, creating a nice, dark backdrop. And that background proved crucial: it allowed the faint, delicate stellar stream to stand out in archival images captured by the Hubble telescope.
The finding, detailed in the Nature journal, was co-led by Julie Kiel Holm of the University of Copenhagen and Sarah Pearson of the Technical University of Denmark, alongside researchers from Northwestern University and the University of Arizona.
Stellar streams form when the gravitational pull of a host galaxy tears apart a globular cluster, which is a tight sphere of up to millions of stars. Rather than scattering randomly into space, the escaped stars remain trapped in a narrow trail, orbiting along nearly identical paths. Because every star in the stream acts as a tracker of gravitational forces, these cosmic trails preserve a record of the unseen mass influencing their motion.
Artist's impression of stellar streams within the Milky Way - Image: NASA/JPL-Caltech/R. Hurt
Astronomers have previously mapped dozens of stellar streams within our own galaxy, but detecting them in external galaxies has been considered nearly impossible due to their extreme faintness. By running thousands of simulations to mirror the observed curvature and length of the stream in UGC 9050-Dw1, the team was able to reconstruct the galaxy's overall gravitational field. Subtracting the gravitational effect of visible stellar matter allowed researchers to calculate the amount and distribution of dark matter holding the system together.
Dark matter accounts for roughly 85% of all matter in the universe, yet because it neither absorbs, reflects, nor emits light, it cannot be observed directly—the only way around that is to rely on its gravitational imprint on visible objects to map its presence. The analysis confirmed that UGC 9050-Dw1 is shrouded in a heavy dark matter halo, thus validating both theoretical expectations and demonstrating that stellar streams can serve as gravitational scales for distant galaxies.
Consequently, extragalactic stellar streams offer a novel way to test how dark matter behaves on smaller scales. As concentrations of dark matter pass near a thin stellar stream, their gravitational pull can create visible gaps, kinks, or ripples in the stellar ribbon.