<\/p>\n “There are only a handful of gamma-ray bursts in the last 50 years that have been detected in the first billion years of the universe<\/a>,” said Andrew Levan, of Radboud University in the Netherlands and the University of Warwick in the U.K., in a statement<\/a>. “This particular event is very rare and very exciting.”<\/p>\n You may like<\/p>\n The story begins on March 14, when the French\u2013Chinese SVOM (Space-based multi-band astronomical Variable Objects Monitor) satellite detected a blast of gamma rays from somewhere in deep space. Ninety minutes later, NASA\u2019s Neil Gehrels Swift Observatory<\/a> detected the same event but in X-rays, enabling astronomers to pinpoint where on the sky the GRB, designated GRB 250314A, had occurred.<\/p>\n Eleven hours after Swift’s detection, the Nordic Optical Telescope, which is 2.6-meter (8.5 feet) telescope on La Palma in the Canary Islands, detected the faint glimmer of light from the GRB’s afterglow as material ejected by the dying star smashed into circumstellar gas. Finally, four hours after that, the Very Large Telescope<\/a> in Chile got in on the act and confirmed the redshift<\/a> of the GRB afterglow to be a huge 7.3, meaning that we are seeing an event that happened 13 billion years ago.<\/p>\n Yet the expansion of space that redshifted the afterglow also creates the illusion of slowing down processes. Rather than the supernova reaching peak brightness in a matter of days or a few weeks, from our point of view, relative to this distant stellar explosion that detonated so long ago only for its light to be traveling through space all this time, it would reach peak brightness three-and-a-half months later.<\/p>\n Armed with this knowledge, Levan led a team to request what’s known as Director’s discretionary time on the James Webb Space Telescope (JWST<\/a>). With that granted, they were ready for July 1, when JWST used its Near-Infrared Camera to detect the light of the supernova that accompanied the GRB.<\/p>\n “Only Webb could directly show that this light is from a supernova \u2014 a collapsing massive star,” said Levan. “This observation also demonstrates that we can use Webb to find individual stars when the universe was only 5% of its current age.”<\/p>\n The JWST was even able to detect the supernova’s host galaxy<\/a>. Despite that galaxy appearing smudged over just a handful of pixels, astronomers are still able to discern something about the supernova\u2019s galactic environment.<\/p>\n \n Artist impressions of the initial GRB (left) and then the supernova that was seen 3.5 months later. (Image credit: Artwork: NASA, ESA, CSA, STScI, Leah Hustak (STScI))<\/p>\n “Webb’s observations indicate that this distant galaxy is similar to other galaxies that existed at the same time,” said Emeric Le Floc’h at CEA Paris-Saclay in France, who is a member of Levan’s team.<\/p>\n The supernova’s spectrum also looks remarkably similar to modern-day supernova explosions, and that the mass of the star that exploded was not atypical of massive stars today. However, upon closer inspection it is likely that there will be differences, given that the supernova exploded in an era where there was a much lower abundance of heavy elements. More data will be needed to tease these details out of the supernova\u2019s spectrum.<\/p>\n Nevertheless, the supernova is a record breaker \u2014 the most distant supernova ever seen, and one of only a few GRB detected (without anyone seeing their supernova explosion) from that first billion years. Previously, the oldest supernova seen (also by the JWST) blew up 1.8 billion years after the Big Bang<\/a>. It’s safe to say that this new redshift 7.3 supernova has well and truly smashed that record.<\/p>\n![\"Two](\"https:\/\/www.newsbeep.com\/il\/wp-content\/uploads\/2025\/12\/vHsjXf3Bmot6hxk9YmaBLo.jpg\")
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