Using the James Webb Space Telescope (JWST), astronomers have observed enigmatic rings in the planetary nebula NGC 1,514, visible in the mid-infrared band. Results of the new observations, published Feb. 28 on the arXiv pre-print server, shed more light on the properties and nature of these rings.
Planetary nebulae (PNe) are expanding shells of gas and dust that have been ejected from a star during the process of its evolution from a main sequence star into a red giant or white dwarf. They are relatively rare, but are important for astronomers studying the chemical evolution of stars and galaxies.
NGC 1,514 (also known as Crystal Ball Nebula) is a large and complex elliptical planetary nebula at a distance of about 1,500 light years away. It originated from a binary star designated HD 281679. The bright, visible component of the system is a giant star of spectral type A0III, while the nebula-generating companion is now a hot, sub-luminous O-type star.