| NGC 4448 | |
|---|---|
Hubble Space Telescope (visible, near-infrared) | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 28m 15.428s |
| Declination | +28° 37′ 13.08″ |
| Redshift | 0.002205 |
| Heliocentric radial velocity | 661±6 km/s |
| Distance | 76.81 ± 0.65 Mly (23.55 ± 0.20 Mpc) |
| Group or cluster | Coma I |
| Apparent magnitude (V) | 11.2 |
| Characteristics | |
| Type | SB(r)ab |
| Apparent size (V) | 3.9′ × 1.4′ |
| Other designations | |
| NGC 4448, UGC 7591, PGC 40988 | |
NGC 4448 is a barred spiral galaxy in the constellation of Coma Berenices. It was discovered April 11, 1785 by German-British astronomer William Herschel. This galaxy has an apparent visual magnitude of 11.2 and spans an angular size of 3.9′ × 1.4′. The core of NGC 4448 can be spotted in a small telescope at an angle of 30′ to the northeast of the star Gamma Comae Berenices. It is located at a distance of 76.8 million light-years (23.55 Mpc) from the Milky Way, where it is a member of the Coma I Group of galaxies.
The morphological classification of this galaxy is SB(r)ab, indicating a barred spiral galaxy (SB) with an inner ring structure (r) and somewhat tightly-wound arms (ab). It is inclined at an angle of about 70° to the plane of the sky and so is being viewed nearly edge on.