NGC 1398
Galaxy in the constellation Fornax
From Wikipedia, the free encyclopedia
NGC 1398 is an isolated barred spiral galaxy exhibiting a double ring structure. It is located 65 million light years from the Earth, in the constellation of Fornax.[2][3] The galaxy, with a diameter of approximately 292,000 light years, is bigger than the Milky Way. Over 100 billion stars are in the galaxy.[4] The discovery credit for NGC 1398 is often given to Friedrich Winnecke of Karlsruhe, Germany, who observed it on 17 December 1868, while he was searching for comets.[5] German astronomer Wilhelm Tempel had first observed it on 9 October 1861, but he did not publish his observation until 1882.[6]
Right ascension03h 38m 52.0633s[1]
Declination−26° 20′ 15.583″[1]
| NGC 1398 | |
|---|---|
| Observation data (J2000 epoch) | |
| Constellation | Fornax |
| Right ascension | 03h 38m 52.0633s[1] |
| Declination | −26° 20′ 15.583″[1] |
| Redshift | 0.004657[1] |
| Distance | 61.8 ± 4.3 Mly (18.96 ± 1.33 Mpc)[1] |
| Apparent magnitude (V) | 10.63[1] |
| Characteristics | |
| Type | (R')SB(r)ab[1] |
| Size | ~291,900 ly (89.51 kpc) (estimated)[1] |
| Apparent size (V) | 7.1′ × 5.4′[1] |
| Other designations | |
| ESO 482-22, IRAS 03367-2629, MCG -04-09-040, PGC 13434[1] | |
Supernovae
Gallery
- NGC 1398 imaged by the Mount Lemmon Observatory
- NGC 1398 imaged by GALEX
- DSS image of NGC 1398
- NGC 1398 imaged by the Hubble Space Telescope
- NGC 1398 imaged by Pan-STARRS
- NGC 1398 imaged by Dark Energy Survey[10]