A stellar bar has been detected in a massive, dust-shrouded galaxy just 1.5 billion years after the Big Bang.
Astronomers led by Leindert A. Boogaard of Leiden University have identified a stellar bar in GN20, a gas-rich starburst galaxy observed at redshift 4.055, a finding that appears to challenge several assumptions that have long underpinned models of early galactic evolution. The discovery, which was submitted to the arXiv preprint server in May 2025, was made possible by the James Webb Space Telescope's Mid-Infrared Instrument and Near-Infrared Camera, instruments sensitive enough to peer through the thick layers of dust that had previously obscured GN20's internal architecture. Stellar bars are elongated, rigidly rotating concentrations of stars that cut across galactic centres, and they are thought to play a significant role in a galaxy's evolution by funnelling gas inward, triggering star formation, and feeding central black holes. While bars are considered common in the present-day universe — the Milky Way itself is believed to host one — their formation has generally been understood to require billions of years to complete. Gas-rich environments, such as those that characterised early galaxies, were also expected to suppress or delay bar formation rather than accommodate it. The bar identified in GN20 spans approximately seven kiloparsecs and was detected through isophotal analysis, a technique that measures how the brightness of a galaxy's light stretches and rotates outward from its centre. A separate mathematical analysis of the light distribution confirmed the structure independently, and the stellar bar was found to align closely with a dust feature mapped by the NOrthern Extended Millimeter Array, lending further weight to the detection.…