On the left is the starburst galaxy M82 as noticed by NASA’s Hubble Area Telescope in 2006. The small field on the galaxy’s core corresponds to the world captured to date by the NIRCam (Close to-Infrared Digicam) instrument on NASA’s James Webb Area Telescope. The pink filaments as seen by Webb are the polycyclic fragrant hydrocarbon emission, which traces the form of the galactic wind. Within the Hubble picture, mild at .814 microns is coloured pink, .658 microns is red-orange, .555 microns is inexperienced, and .435 microns is blue (filters F814W, F658N, F555W, and F435W, respectively). Within the Webb picture, mild at 3.35 microns is coloured pink, 2.50 microns is inexperienced, and 1.64 microns is blue (filters F335M, F250M, and F164N, respectively). NASA, ESA, CSA, STScI, A. Bolatto (College of Maryland)