Also known informally as the Southern Ring Nebula, NGC 3132 is a planetary nebula formed when a dying star ejected its outer layers. JWST's Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI) captured the nebula's glowing gas arcs, concentric rings, and dark dust lanes, which are the result of the central star's interactions with a companion star. The new images reveal how the dying star's stellar winds have shaped the surrounding material into its distinctive structures.
Planetary nebulae like the Southern Ring provide valuable insights into how stars evolve and die. The JWST data will help astronomers study the composition of the nebula's gas and dust, as well as the dynamics of the central star system. These observations may also shed light on the role of binary star systems in the formation of planetary nebulae, offering clues about the final stages of stellar life in the universe.
