A stellar bar has been detected in GN20, a massive galaxy observed 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 located at redshift 4.055, which is thought to challenge several prevailing assumptions about how and when such structures are able to form in the early universe. The findings, which were submitted to the arXiv preprint server in May 2026, were made possible by the James Webb Space Telescope's capacity to peer through the dense dust that had previously obscured the galaxy's internal architecture. Stellar bars are elongated concentrations of stars that rotate across a galaxy's centre as a single rigid unit, and they are widely understood to act as gravitational funnels, drawing gas inward in ways that can trigger intense star formation, feed a central black hole, and consolidate a dense galactic core. In the nearby universe, bars of this kind are considered commonplace — the Milky Way itself is thought to host one — yet their formation has generally been regarded as a slow process, unfolding over billions of years. The detection in GN20 is considered remarkable for several reasons. Early galaxies were expected to be too gas-rich for a bar to stabilise, since high gas fractions are believed to suppress or delay bar formation. Yet analysis of the galaxy's brightness distribution — a technique known as isophotal analysis — revealed a bar structure spanning seven kiloparsecs, a result that was subsequently confirmed through an independent mathematical analysis of the same light patterns.…