Astronomers report CDG‑2, about 300 million light‑years away in the Perseus Cluster, appears to be ~99.9% dark matter and is visible only through a few bright globular star clusters and a faint halo. The team used Hubble, ESA's Euclid, and Subaru data plus a globular‑cluster–based search method to infer a massive dark halo with almost no ongoing star formation, likely because a cluster environment stripped its gas.
— If confirmed, these nearly starless 'dark' galaxies become clean laboratories to test dark matter behavior and galaxy‑formation theory and provide a new observational route (globular clusters) to find more such objects.
EditorDavid
2026.03.07
100% relevant
Lead author Dayi Li’s study using Hubble, Euclid, and Subaru data identified four globular clusters and a faint halo in the Perseus Cluster consistent with a massive dark‑matter halo that lacks stars.
← Back to All Ideas