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Millions of Stars in Cigar Galaxy

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Hourglass-shaped plumes of gas shoot outward from above and below a bright disk-shaped center. The plumes are yellow near the galaxy’s bright center and gradually become redder as you move farther away. M82 is set against the black background of space, which has many distant galaxies that appear as small white and orange spirals, ovals, and points of light. On the right of M82 is a blue-white star with diffraction spikes.
NASA, ESA, CSA, Adam Smercina (STScI, Tufts), Thomas Williams (University of Manchester); Image processing: Alyssa Pagan (STScI)

NASA’s James Webb Space Telescope recently observed edge-on starburst galaxy Messier 82 (M82), nicknamed the Cigar Galaxy. Webb’s new view of M82, added to archival data from NASA’s Hubble Space Telescope, gives us a more complete picture of this starburst galaxy. 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.

Read the full story.

Image credit: NASA, ESA, CSA, Adam Smercina (STScI, Tufts), Thomas Williams (University of Manchester); Image processing: Alyssa Pagan (STScI)

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