| NGC 1247 | |
|---|---|
NGC 1247 (center) and Mrk 1071 (lower left) imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 12m 14.2539s |
| Declination | −10° 28′ 50.963″ |
| Redshift | 0.013166±0.0000140 |
| Heliocentric radial velocity | 3,947±4 km/s |
| Distance | 205.85 ± 7.89 Mly (63.113 ± 2.419 Mpc) |
| Group or cluster | NGC 1241 group (LGG 84) |
| Apparent magnitude (V) | 13.47 |
| Characteristics | |
| Type | Sbc edge-on |
| Size | ~251,700 ly (77.17 kpc) (estimated) |
| Apparent size (V) | 4.59′ × 0.58′ |
| Other designations | |
| IRAS 03098-1040, 2MASX J03121431-1028520, UGCA 58, MCG -02-09-014, PGC 11931 | |
NGC 1247 is a large edge-on spiral galaxy in the constellation of Eridanus. Its velocity with respect to the cosmic microwave background is 3,774±13 km/s, which corresponds to a Hubble distance of 181.6 ± 12.7 Mly (55.67 ± 3.90 Mpc). However, 16 non-redshift measurements give a farther mean distance of 205.85 ± 7.89 Mly (63.113 ± 2.419 Mpc). It was discovered by German-British astronomer William Herschel on 10 December 1798.
NGC 1247 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 1247 is a member of the NGC 1241 galaxy group (also known as LGG 84). The other four galaxies in the group are NGC 1241, NGC 1242, Mrk 1071, and MCG-02-09-006
One supernova has been observed in NGC 1247: