NGC 1572 is a large barred spiral galaxy in the constellation of Caelum. Its velocity with respect to the cosmic microwave background is 6,081±10 km/s, which corresponds to a Hubble distance of 292.5 ± 20.5 Mly (89.68 ± 6.28 Mpc). However, six non-redshift measurements give a closer mean distance of 223.69 ± 9.42 Mly (68.583 ± 2.888 Mpc). It was discovered by British astronomer John Herschel on 23 October 1835. NGC 1572 is a Seyfert II galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable.
Supernova One supernova has been observed in NGC 1572:
SN 2009la (Type Ia, mag. 15.7) was discovered by Stuart Parker on 12 November 2009, and independently by Berto Monard, on 11 November 2009.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1572 at Wikimedia Commons NGC 1572 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


