NGC 7110 | |
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Observation data (J2000 epoch) | |
Constellation | Piscis Austrinus |
Right ascension | 21h 42m 12.15s[1] |
Declination | −34° 09′ 44.0″[1] |
Redshift | 0.017679 [1] |
Heliocentric radial velocity | 5300 ± 10 km/s[1] |
Distance | 242.6 ± 17.0 Mly (74.39 ± 5.22 Mpc)[1] |
Apparent magnitude (V) | 13.2[1] |
Characteristics | |
Type | SB(r)b?[1] |
Size | ~117,300 ly (35.96 kpc) (estimated)[1] |
Apparent size (V) | 1.3' x 0.6'[1] |
Other designations | |
IRAS F21392-3423, 2MASX J21421214-3409436, MCG -06-47-012, PGC 67199, ESO 403- G 016[1] |
NGC 7110 is a barred spiral galaxy in the constellation of Piscis Austrinus. Its velocity with respect to the cosmic microwave background is 5044 ± 20 km/s, which corresponds to a Hubble distance of 74.39 ± 5.22 Mpc (∼243 million light-years).[1] It was discovered by British astronomer John Herschel on 23 September 1834.[2]
One supernova has been observed in NGC 7110: SN 2023hnl (type Ia, mag. 17.8).[3]