| NGC 2532 | |
|---|---|
NGC 2532 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 08h 10m 15.1840s |
| Declination | +33° 57′ 23.757″ |
| Redshift | 0.017506±0.000002 |
| Heliocentric radial velocity | 5,248±1 km/s |
| Distance | 128.97 ± 6.85 Mly (39.543 ± 2.099 Mpc) |
| Apparent magnitude (V) | 13.5g |
| Characteristics | |
| Type | SAB(rs)c |
| Size | ~84,000 ly (25.75 kpc) (estimated) |
| Apparent size (V) | 1.74′ × 1.47′ |
| Other designations | |
| IRAS 08070+3406, UGC 4256, MCG +06-18-013, PGC 22922, CGCG 178-032 | |
NGC 2532 is a barred spiral galaxy in the constellation of Lynx. Its velocity with respect to the cosmic microwave background is 5,437±13 km/s, which corresponds to a Hubble distance of 261.6 ± 18.3 Mly (80.20 ± 5.62 Mpc). However, seven non-redshift measurements give a much closer mean distance of 128.97 ± 6.85 Mly (39.543 ± 2.099 Mpc). It was discovered by German-British astronomer William Herschel on 5 February 1788.
NGC 2532 has an 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.
Three supernovae have been observed in NGC 2532: