| NGC 3241 | |
|---|---|
NGC 3241 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Antlia |
| Right ascension | 10h 24m 16.9527s |
| Declination | −32° 28′ 57.830″ |
| Redshift | 0.010070±0.0000130 |
| Heliocentric radial velocity | 3,019±4 km/s |
| Distance | 135.97 ± 9.83 Mly (41.688 ± 3.015 Mpc) |
| Group or cluster | LDC 729 |
| Apparent magnitude (V) | 13.06 |
| Characteristics | |
| Type | SA(r)ab |
| Size | ~133,000 ly (40.79 kpc) (estimated) |
| Apparent size (V) | 2.2′ × 1.5′ |
| Other designations | |
| ESO 436- G 016, IRAS 10220-3213, 2MASX J10241695-3228574, MCG -05-25-002, PGC 30498 | |
NGC 3241 is a spiral galaxy in the constellation of Antlia. Its velocity with respect to the cosmic microwave background is 3,347±23 km/s, which corresponds to a Hubble distance of 161.0 ± 11.3 Mly (49.37 ± 3.47 Mpc). However, eight non-redshift measurements give a closer mean distance of 135.97 ± 9.83 Mly (41.688 ± 3.015 Mpc). It was discovered by British astronomer John Herschel on 16 February 1836.
NGC 3241 has a possible active galactic nucleus, i.e. it has a compact region at the center of its galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
NGC 3241 is a member of a galaxy group known as LDC 729. This group contains 210 galaxies, including 72 from the New General Catalogue and 26 from the Index Catalogue.
Two supernovae have been observed in NGC 3241.