| NGC 3950 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Major |
| Right ascension | 11h 53m 41.41s |
| Declination | +47d 53m 04.46s |
| Redshift | 0.074602 |
| Heliocentric radial velocity | 22,365 km/s |
| Distance | 1.030 Gly (315 Mpc) |
| Apparent magnitude (V) | 15.7 |
| Apparent magnitude (B) | 16.7 |
| Surface brightness | 13.2 |
| Characteristics | |
| Type | E, E0;cand. dwarf |
| Apparent size (V) | 0.30' x 0.3' |
| Other designations | |
| PGC 37294, MCG +08-22-030, BTS 051, HOLM 301B | |
NGC 3950 is an elliptical galaxy of type E, [1] in Ursa Major. Its redshift is 0.074602, [2] meaning NGC 3950 is 1.03 billion light-years or 316 Mpc from Earth, which is within the Hubble distance values. [3] This high redshift makes NGC 3950 one of the furthest New General Catalogue objects. [4]
NGC 3950 has apparent dimensions of 0.30 x 0.3 arcmin, meaning the galaxy is 90,000 light-years across. [5] It was discovered by Lawrence Parsons [6] [7] on April 27, 1875, and he described it as, "extremely faint, 2.6 arcmin north of h 1009". [6]
In a research article published in 1990, [8] NGC 3950 was believed to be a dwarf galaxy, and a close companion of a larger spiral galaxy, NGC 3949. [9] But further research involving measuring its redshift in 2005 showed NGC 3950 is much further away in the background. [10] Together with NGC 3949, they both form an optical galaxy pair called HOLM 301. [11]
