NGC 3780 is a spiral galaxy in the constellation of Ursa Major. Its velocity with respect to the cosmic microwave background is 2,557±12 km/s, which corresponds to a Hubble distance of 123.0 ± 8.6 Mly (37.71 ± 2.65 Mpc). However, 10 non-redshift measurements give a closer mean distance of 109.65 ± 9.10 Mly (33.620 ± 2.789 Mpc). It was discovered by German-British astronomer William Herschel on 14 April 1789. NGC 3780 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms. It also has an active galaxy nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
NGC 3780 group According to A. M. Garcia, NGC 3780 is the namesake of a small group of galaxies. The NGC 3780 group (also known as LGG 247) includes at least four galaxies, including NGC 3888, UGC 6596, and UGC 6774.
Supernovae Three supernovae have been observed in NGC 3780:
SN 1978H (Type II, mag. 16.5) was discovered by Swiss astronomer Paul Wild on 7 November 1978. SN 1992bt (Type II, mag. 16) was discovered by the Leuschner Observatory Supernova Search on 19 December 1992. SN 2024btj (Type II, mag. 18.53) was discovered by the Xingming Observatory Sky Survey (XOSS) on 5 February 2024.
See also List of NGC objects (3001–4000)
References
External links Media related to NGC 3780 at Wikimedia Commons NGC 3780 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


