06/23/2026
Webb’s new view of M82, added to archival data from NASA's Hubble Space Telescope, is giving us a more complete picture of this starburst galaxy. Located 12 million light-years away and undergoing rapid star formation, edge-on spiral galaxy Messier 82 (M82) is a scientifically unique sight to behold, and now NASA’s James Webb Space Telescope has revealed previously unseen details. Because Webb can see infrared light, it is able to peer through clouds of dust and gas to see the shape of this edge-on galaxy, as well as approximately 16.5 million of its stars. M82’s rapid star formation, thought to be the result of its merger with another galaxy, will only be a (relatively) brief period in its history. Ironically, the extreme star formation is causing plumes of material to be ejected above and below the disk of the galaxy - something that will disrupt future stellar birth.
Many of the features of this galaxy were blocked dust and gas at visible wavelengths of light. Webb is capturing never-before-seen detail, including the galaxy’s uniquely distorted disk, likely a result of the galaxy merger - and a staggering number of stars. These 16.5 million are likely only a small portion of the total number of stars that might reside in a galaxy like M82. Hubble data, in yellow, show tendrils of material, which represent ionized hydrogen gas, close to the galaxy’s disk.
Credit: Image: NASA, ESA, CSA, Adam Smercina (STScI, Tufts), Thomas Williams (University of Manchester); Image Processing: Alyssa Pagan (STScI).