NGC 178 is a Magellanic spiral galaxy in the constellation of Cetus. The compiler of the New General Catalogue, John Louis Emil Dreyer noted that NGC 178 was "faint, small, much extended 0°, brighter middle". It was discovered on November 3, 1885, by Ormond Stone. Due to its high rate of star formation NGC 178 is a starburst galaxy. It is forming new stars at a rate of 0.55 M☉ per year. The peculiar morphology of this galaxy may be a sign of it being a galaxy merger.
See also Spiral galaxy List of NGC objects (1–1000)
References
External links Media related to NGC 178 at Wikimedia Commons NGC 178 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images SEDS


