NGC 2022 is a planetary nebula in the constellation of Orion, located at a distance of 8210 light-years from the Sun.
NGC 2022 is a vast orb of gas in space, cast off by an aging star. The star is visible in the orb's center, shining through the gases it formerly held onto for most of its stellar life. When stars like the Sun grow advanced in age, they expand and glow red. These so-called red giants then begin to lose their outer layers of material into space. More than half of such a star's mass can be shed in this manner, forming a shell of surrounding gas. At the same time, the star's core shrinks and grows hotter, emitting ultraviolet light that causes the expelled gases to glow. This type of object is called, somewhat confusingly, a planetary nebula, though it has nothing to do with planets. The name derives from the rounded, planet-like appearance of these objects in early telescopes. (REF: https://science.nasa.gov/missions/hubble/hubbles-portrait-of-stars-gaseous-glow/)
Observation data: J2000 epochRight ascension: 05h 42m 06.19056sDeclination: +09° 05′ 10.5843″Distance: 8.21 klyApparent magnitude (V): 11.6Apparent dimensions (V): 28″Constellation: Orion
Tech Specs: Orion 8” RC Telescope, ZWO ASI2600MC camera running at -10F, 81 x 60 seconds, Celestron CGEM-DX pier mounted, ZWO EAF and ASIAir Pro, processed in DSS and PixInsight. Image Date: January 31, 2024. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).