| NGC 941 | |
|---|---|
NGC 941 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 02h 28m 27.847s |
| Declination | −01° 09′ 05.61″ |
| Redshift | 0.005398 |
| Heliocentric radial velocity | 1613.8 km/s |
| Distance | 54.9 Mly (16.83 Mpc) |
| Apparent magnitude (V) | 12.20 |
| Apparent magnitude (B) | 12.8 |
| Absolute magnitude (V) | −19.1 |
| Characteristics | |
| Type | SAB(rs)c |
| Other designations | |
| UGC 1954, MCG +00-07-022, PGC 9414 | |
NGC 941 is an intermediate spiral galaxy in the constellation Cetus. It is an estimated 16.83 MPc (55 million light-years) from the Milky Way and has a diameter of approximately 55,000 light years. The galaxies NGC 926, NGC 934, NGC 936, NGC 955 are located in the same sky area. NGC 941 was discovered by German-British astronomer William Herschel on 6 January 1785.
The morphological classification of NGC 941 is SAB(rs)c, indicating a spiral galaxy with a weak bar structure (SAB), an incomplete inner ring (RS), and moderately wound spiral arms (c).
One supernova has been observed in NGC 941.