NGC 7808 is a lenticular galaxy in the constellation of Cetus. Its velocity with respect to the cosmic microwave background is 8521 ± 24 km/s, which corresponds to a Hubble distance of 125.67 ± 8.80 Mpc (~410 million light-years). It was discovered by American astronomer Frank Muller in 1886. NGC 7808 is an active Seyfert I galaxy. One supernova has been observed in NGC 7808: SN 2023qnz (Type Ia, mag. 20.14) was discovered by Pan-STARRS on 22 August 2023.
Star-forming ring NGC 7808 contains an outer star-forming ring, observed in ultraviolet rays. According to a 2019 study, the star formation is only above one solar mass per year. It is expected to decrease over time. Nevertheless, star-forming rings like in NGC 7808 still contain enigmatic features and can help astronomers to learn more about the evolutionary processes taken by these galaxies.
See also List of NGC objects (7001–7840)
References
External links Media related to NGC 7808 at Wikimedia Commons NGC 7808 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


