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White Dwarfs Supernovae Massive Stars Star Formation Red Giants Binary Stars Neutron Stars Planetary Nebulae Red Supergiants White Dwarf Stars Star Clusters Binary Star Systems Star Explosions Protostars Star Types Young Stars Star Life Cycle Nuclear Fusion Variable Stars Population III Stars Black Holes Metallicity Binary Systems Star Death Star Classification Giant Stars Metal-Poor Stars Black Hole Formation Element Formation Brown Dwarfs Planetary Science Supergiant Stars Star Composition Dying Stars Nucleosynthesis Star Observation Supernova Sun Supernova Types Core-Collapse Supernovae Planetary Formation Gravitational Perturbations Energy Production Models Star Mergers Massive Star Collapse Low Metallicity Stars Neutron Star Formation Main-Sequence Lifetimes Main-Sequence Stars Planetary Consumption Star-Planet Interactions Dwarf Stars End-of-Life Stars Companion Stars Cataclysmic Variables Low-Intermediate Mass Stars Sun-like Stars Supernova Mechanisms Stellar Structure Heavy Elements Low-Mass Stars Metal-free Stars Progenitor Stars Star Interactions Cluster Dynamics Post-Main-Sequence Stars Planetary Systems Open Clusters Stellar Remnants Implications of Discovery Thermonuclear Explosions Pulsars Type Ia Supernovae Cepheid Variables Supergiants Exoplanets Magnetars Star Lifecycle Cosmic Events Stellar Mergers Hydrogen Burning Supernova Remnants Triple Star Systems Protoplanetary Disks Aging Stars Starquakes Star Collapse Wolf-Rayet Stars Supernovas Stellar Explosions Core Collapse Red Supergiant Stars Stellar Ages Star Explosion Star Systems Explosion Failed Stars Binary Neutron Stars Star Birthline
A student-selected target showcases a bipolar planetary nebula with glowing wings located roughly 2,500 to 3,800 light-years away.
