What it is
Using NIRSpec spectroscopy, JWST confirmed MoM-z14, a luminous galaxy at a spectroscopic redshift of 14.44, seen just 280 million years after the Big Bang. The source is bright (UV magnitude -20.2) yet extremely compact, with a half-light radius of about 74 parsecs, and shows a steep, dust-free ultraviolet spectrum. The survey implies the number density of such early bright galaxies is more than 100 times higher than pre-JWST models predicted.
Why it matters
MoM-z14 is the most distant spectroscopically confirmed galaxy known, pushing the observational frontier deeper into cosmic history. The finding that bright galaxies at redshift 14 to 15 are more than 100 times more common than expected sharpens a genuine puzzle: standard models struggle to explain how galaxies grew so luminous so fast, within 280 million years of the Big Bang. Its nitrogen-rich chemistry hints at exotic early stellar populations.
Underlined numbers link to their source. Every metric and quoted figure is listed under Sources and data below.
Filed underJWST, early universe, high-redshift galaxy, reionization, cosmology