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| NGC 7110 | |
|---|---|
 The barred spiral galaxy NGC 7110 | |
| Observation data (J2000 epoch) | |
| Constellation | Piscis Austrinus |
| Right ascension | 21h 42m 12.1278s[1] |
| Declination | −34° 09′ 44.767″[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′ × 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. 17.831) was discovered by ATLAS on 2 May 2023.[3]