| NGC 4674 | |
|---|---|
The barred spiral galaxy NGC 4674. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 12h 46m 03.4249s |
| Declination | −08° 39′ 18.484″ |
| Redshift | 0.005023 |
| Heliocentric radial velocity | 1506 ± 37 km/s |
| Distance | 88.8 ± 6.8 Mly (27.23 ± 2.09 Mpc) |
| Apparent magnitude (V) | 13.1 |
| Characteristics | |
| Type | SAB(s)a pec edge-on |
| Size | ~46,800 ly (14.34 kpc) (estimated) |
| Apparent size (V) | 1.6′ × 0.5′ |
| Other designations | |
| IRAS F12434-0822, 2MASS J12460346-0839198, MCG -01-33-005, PGC 43050, SDSS J124603.46-083920.5 | |
NGC 4674 is an edge-on barred spiral galaxy located in the constellation of Virgo. Its velocity relative to the cosmic microwave background is 1,846 ± 44 km/s, which corresponds to a Hubble distance of 27.23 ± 2.09 Mpc (~88.8 million light-years). NGC 4674 was discovered by British astronomer John Herschel on 5 May 1836.
NGC 4674 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
One supernova has been observed in NGC 4674: SN 1907A (type unknown, mag. 13.5) was discovered by Luyten on 9 May 1907.