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] |
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]
Two supernovae have been observed in NGC 1398: