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 1241 group 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
Supernova One supernova has been observed in NGC 1247:
SN 2026xqu (Type Ia-pec, mag. 18.28) was discovered by GOTO on 6 August 2026.
See also List of NGC objects (1001–2000)
References
External links Media related to NGC 1247 at Wikimedia Commons NGC 1247 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


