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Galaxy in the constellation Ursa Major From Wikipedia, the free encyclopedia
NGC 3877 is a type Sc spiral galaxy that was discovered by William Herschel on February 5, 1788.[3] It is located below the magnitude 3.7 star Chi Ursae Majoris in Ursa Major.[3][4]
NGC 3877 | |
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![]() NGC 3877 (Sloan Digital Sky Survey) | |
Observation data (J2000 epoch) | |
Constellation | Ursa Major |
Right ascension | 11h 46m 07.8s[1] |
Declination | +47° 29′ 41″[1] |
Redshift | 0.002987[1] |
Heliocentric radial velocity | 895 ± 4 km/s[1] |
Distance | 50.5 ± 4.2 Mly (15.5 ± 1.3 Mpc)[2] |
Apparent magnitude (V) | 12.1[1] |
Characteristics | |
Type | Sc[1] |
Apparent size (V) | 4'.4 × 0'.8[1] |
Other designations | |
UGC 6745, PGC 36699[1] |
The Type IIn supernova SN 1998S[3][5] is the only supernova that has been observed within NGC 3877.
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.[6][7][8]