| NGC 1325 | |
|---|---|
| Hubble Space Telescope image of NGC 1325 | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 25.576m [1] |
| Declination | −21° 32′ 38.61″ [1] |
| Heliocentric radial velocity | 1,588 [2] |
| Distance | 75.0 Mly (23.01 Mpc)h−1 0.73 [2] |
| Group or cluster | Eridanus Cluster [3] |
| Apparent magnitude (V) | 11.5 [4] |
| Characteristics | |
| Type | SBbc [5] |
| Apparent size (V) | 4.47′ × 1.66′ [5] |
| Notable features | Flocculent spiral galaxy |
| Other designations | |
| IRAS 03221-2143, NGC 1325, UGCA 70, PGC 12737, ESO 548-7, MCG -4-9-4 [5] | |
References: [6] | |
NGC 1325 is a flocculent spiral galaxy situated in the constellation of Eridanus. Located about 75 million light years away, [2] it is a member of the Eridanus Cluster of galaxies, [3] a cluster of about 200 galaxies. It was discovered by William Herschel on 19 December 1799.
NGC 1325 has a Hubble classification of SBbc, which indicates it is a barred spiral galaxy with moderately wound arms. [5] Its angular size on the night sky is 4.5' x 1.7'. [5] The disk of the galaxy is inclined at an angle of 71° with the main axis aligned along a position angle of 232°. [3] The rotation curve for the galaxy is flat across much of the radius from the core. [7] The galaxy is moving away from the Milky Way with a heliocentric radial velocity of 1,588 km/s. [2]
Two supernovae have been observed in NGC 1325: