| NGC 5247 | |
|---|---|
| Image of NGC 5247 made in infrared light with the HAWK-I camera on ESO's Very Large Telescope at Paranal Observatory. | |
| Observation data (J2000 epoch) | |
| Constellation | Virgo |
| Right ascension | 13h 38m 03.040s [1] |
| Declination | –17° 53′ 02.50″ [1] |
| Redshift | 0.004520 [2] |
| Heliocentric radial velocity | +1,357 [3] km/s |
| Distance | 60.34 Mly (18.50 Mpc) [3] |
| Apparent magnitude (V) | 10.5 [2] |
| Characteristics | |
| Type | SA(s)bc [2] |
| Apparent size (V) | 5′.6 × 4′.9 [2] |
| Other designations | |
| UGCA 368, [2] PGC 48171 [2] | |
NGC 5247 is a face-on unbarred spiral galaxy located some 60 [3] million light years away in the constellation Virgo. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. [4] This is a grand design spiral galaxy that displays no indications of distortion caused by interaction with other galaxies. [5] It has two spiral arms that bifurcate after wrapping halfway around the nucleus. [6] The disk is estimated to be 4.9 ± 2.0 kly (1.5 ± 0.6 kpc) in thickness and it is inclined by roughly 28° to the line of sight. [5]
Two supernovae have been observed in NGC 5247: