| NGC 5248 | |
|---|---|
NGC 5248 imaged with a 32-inch telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Boötes |
| Right ascension | 13h 37m 32.0235s |
| Declination | +08° 53′ 06.907″ |
| Redshift | 1151 ± 1 km/s |
| Distance | 69.1 ± 4.9 Mly (21.19 ± 1.51 Mpc) |
| Apparent magnitude (V) | 10.97 |
| Characteristics | |
| Type | SAB(rs)bc |
| Size | ~84,600 ly (25.93 kpc) (estimated) |
| Apparent size (V) | 6.2′ × 4.5′ |
| Other designations | |
| Caldwell 45, IRAS 13350+0908, UGC 8616, MCG +02-35-015, PGC 48130, CGCG 073-054 | |
NGC 5248 (also known as Caldwell 45) is a compact intermediate spiral galaxy in the constellation Boötes. Its velocity with respect to the cosmic microwave background is 1437 ± 20 km/s, which corresponds to a Hubble distance of 69.1 ± 4.9 Mly (21.19 ± 1.51 Mpc). However, 17 non redshift measurements give a much closer distance of 42.52 ± 3.16 Mly (13.038 ± 0.969 Mpc). It was discovered on 15 April 1784 by German-British astronomer William Herschel.
NGC 5248 is a member of the NGC 5248 Group of galaxies, itself one of the Virgo III Groups strung out to the east of the Virgo Supercluster of galaxies.