| NGC 2446 | |
|---|---|
NGC 2446 imaged by Pan-STARRS | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 07h 48m 39.2173s |
| Declination | +54° 36′ 42.570″ |
| Redshift | 0.018906±0.0000200 |
| Heliocentric radial velocity | 5,668±6 km/s |
| Distance | 233.94 ± 7.66 Mly (71.725 ± 2.350 Mpc) |
| Group or cluster | LDC 537 |
| Apparent magnitude (V) | 13.73 |
| Characteristics | |
| Type | Sb |
| Size | ~158,200 ly (48.51 kpc) (estimated) |
| Apparent size (V) | 1.9′ × 1.0′ |
| Other designations | |
| IRAS 07446+5444, 2MASX J07483926+5436430, UGC 4027, MCG +09-13-058, PGC 21860, CGCG 262-030 | |
NGC 2446 is a spiral galaxy in the constellation of Lynx. Its velocity with respect to the cosmic microwave background is 5,766±9 km/s, which corresponds to a Hubble distance of 277.4 ± 19.4 Mly (85.04 ± 5.96 Mpc). However, eight non-redshift measurements give a closer mean distance of 233.94 ± 7.66 Mly (71.725 ± 2.350 Mpc). It was discovered by British astronomer John Herschel on 10 February 1831.
NGC 2446 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.
NGC 2446 is member of a small galaxy group known as LDC 537. The other three galaxies in the group are Z 262-54, UGC 4035, and Z 262-35.
Two supernovae have been observed in NGC 2446: