| NGC 5671 | |
|---|---|
NGC 5671 imaged by Pan-STARRS | |
| Observation data (J2000 epoch) | |
| Constellation | Ursa Minor |
| Right ascension | 14h 27m 42.0426s |
| Declination | +69° 41′ 38.703″ |
| Redshift | 0.030074±0.000143 |
| Heliocentric radial velocity | 9,016±43 km/s |
| Distance | 353.75 ± 10.07 Mly (108.460 ± 3.086 Mpc) |
| Apparent magnitude (V) | 14.10 |
| Characteristics | |
| Type | SB(r)b |
| Size | ~211,000 ly (64.68 kpc) (estimated) |
| Apparent size (V) | 1.7′ × 1.2′ |
| Other designations | |
| IRAS F14269+6954, UGC 9297, MCG +12-14-006, PGC 51641, CGCG 337-014 | |
NGC 5671 is a large barred spiral galaxy in the constellation of Ursa Minor. Its velocity with respect to the cosmic microwave background is 9,058±43 km/s, which corresponds to a Hubble distance of 435.7 ± 30.6 Mly (133.59 ± 9.39 Mpc). However, five non-redshift measurements give a closer mean distance of 353.75 ± 10.07 Mly (108.460 ± 3.086 Mpc). It was discovered by German-British astronomer William Herschel on 6 May 1791.
According to Abraham Mahtessian, NGC 5671 and UGC 9295 form a pair of galaxies.
Two supernovae have been observed in NGC 5671: