| NGC 2565 | |
|---|---|
NGC 2565 imaged by SDSS | |
| Observation data (J2000 epoch) | |
| Constellation | Cancer |
| Right ascension | 08h 19m 48.3092s |
| Declination | +22° 01′ 53.087″ |
| Redshift | 0.011948 |
| Heliocentric radial velocity | 3,582±1 km/s |
| Distance | 183.5 ± 12.9 Mly (56.26 ± 3.95 Mpc) |
| Group or cluster | NGC 2545 group (LGG 156) |
| Apparent magnitude (V) | 12.6 |
| Characteristics | |
| Type | (R')SBbc? |
| Size | ~106,600 ly (32.68 kpc) (estimated) |
| Apparent size (V) | 1.9′ × 0.9′ |
| Other designations | |
| IRAS 08168+2211, UGC 4334, MCG +04-20-026, Mrk 386, PGC 23362, CGCG 119-057 | |
NGC 2565 is a barred spiral galaxy in the constellation of Cancer. Its velocity with respect to the cosmic microwave background for is 3,814±16 km/s, which corresponds to a Hubble distance of 183.5 ± 12.9 Mly (56.26 ± 3.95 Mpc). Additionally, 34 non-redshift measurements give a distance of 169.79 ± 4.64 Mly (52.057 ± 1.422 Mpc). It was discovered by German-British astronomer J. Gerhard Lohse (bio-fr) in 1886.
NGC 2565 is a galaxy whose nucleus shines brightly in the ultraviolet. It is listed in the Markarian catalogue as Mrk 386.
NGC 2565 is surrounded by a ring, and is a starburst galaxy, as indicated by its entry in the NASA/IPAC Extragalactic Database.
NGC 2565 is a member of the NGC 2545 group (also known as LGG 156). The other galaxies in the group are NGC 2545, UGC 4308, CGCG 119-044, and CGCG 119-56.
Two supernovae have been observed in NGC 2565: