NGC 2525
| NGC 2525 | |
|---|---|
NGC 2525 in 2018, imaged by the Hubble Space Telescope with SN 2018gv on Lower Left | |
| Observation data (J2000 epoch) | |
| Constellation | Puppis |
| Right ascension | 08h 05m 38.0503s |
| Declination | −11° 25′ 37.213″ |
| Redshift | 0.005270 ± 0.000005 |
| Heliocentric radial velocity | 1,580 ± 1 km/s |
| Distance | 71 Mly (21.9 Mpc) |
| Apparent magnitude (V) | 11.6 |
| Characteristics | |
| Type | SB(s)c |
| Size | ~46,200 ly (14.16 kpc) (estimated) |
| Apparent size (V) | 2.9′ × 1.9′ |
| Other designations | |
| IRAS 08032-1117, UGCA 135, MCG -02-21-004, PGC 22721 | |
NGC 2525 is a barred spiral galaxy located in the constellation Puppis. It is located at a distance of about 70 million light years from Earth, which, given its apparent dimensions, means that NGC 2525 is about 46,000 light years across. It was discovered by William Herschel on February 23, 1791.