A stellar bar has been detected in a massive galaxy from just 1.5 billion years after the Big Bang, challenging foundational models of galactic evolution.
Astronomers led by Leindert A. Boogaard of Leiden University have identified a stellar bar in GN20, a distant, dust-shrouded galaxy observed at a cosmic epoch when such structures were not expected to exist. The findings, which were submitted to the arXiv preprint server on 14 May 2026, draw on imaging from the James Webb Space Telescope's Near-Infrared Camera and Mid-Infrared Instrument, both of which are capable of penetrating the dense layers of dust that had previously obscured the galaxy's internal architecture. Stellar bars are elongated, rigidly rotating concentrations of stars that extend across a galaxy's centre.
They are thought to act as gravitational funnels, drawing gas inward in a process that can accelerate star formation, supply material to a central black hole, and consolidate a galaxy's core. Bars of this kind are common in the present-day universe — the Milky Way itself is known to host one — but their formation has traditionally been modelled as a gradual process requiring several billion years to complete. Three distinct lines of evidence are said to support the detection. An isophotal analysis — which measures how contours of equal brightness are distributed and oriented across the galaxy — revealed a bar-like elongation spanning approximately seven kiloparsecs.
A separate mathematical decomposition of the light profile confirmed the structure independently. Crucially, the stellar bar was found to be strongly aligned with a corresponding dust feature mapped by the NOrthern Extended Millimeter Array (NOEMA), lending further weight to the claim.