| NGC 3877 | |
|---|---|
NGC 3877 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 11h 46m 07.7281s |
| Declination | +47° 29′ 40.369″ |
| Redshift | 0.002987 |
| Heliocentric radial velocity | 895 ± 4 km/s |
| Distance | 50.5 ± 4.2 Mly (15.5 ± 1.3 Mpc) |
| Apparent magnitude (V) | 11.2 |
| Characteristics | |
| Type | Sc |
| Size | ~80,900 ly (24.80 kpc) (estimated) |
| Apparent size (V) | 5.3′ × 1.2′ |
| Other designations | |
| IRAS 11434+4746, NGC 3877, UGC 6745, MCG +08-22-002, PGC 36699, CGCG 243-004 | |
NGC 3877 is a spiral galaxy in the northern constellation of Ursa Major, to the south of the magnitude 3.7 star Chi Ursae Majoris. It was discovered by the German-British astronomer William Herschel on February 5, 1788. This galaxy has a visual magnitude of 11.2 and spans an angular size of 5.3′ × 1.2′. It lies at a distance of 50.5 ± 4.2 million light-years (15.5 ± 1.3 Mpc).

One supernova has been observed in NGC 3877: SN 1998S (Type IIn, mag. 15.2) was discovered by the BAO Supernova Survey on 3 March 1998.
NGC 3877 is a member of the M109 Group, a group of galaxies located in the constellation Ursa Major that may contain over 50 galaxies. The brightest galaxy in the group is the spiral galaxy M109.