| NGC 6925 | |
|---|---|
NGC 6925 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Microscopium |
| Right ascension | 20h 34m 20.5638s |
| Declination | −31° 58′ 50.965″ |
| Redshift | 0.009303±0.00000500 |
| Heliocentric radial velocity | 2,789±1 km/s |
| Distance | 92.94 ± 2.66 ± 13.57 Mly (28.497 ± 0.817 ± 4.162 Mpc) |
| Group or cluster | NGC 6925 group (LGG 437) |
| Apparent magnitude (V) | 11.3 |
| Apparent magnitude (B) | 12.09 |
| Characteristics | |
| Type | SA(s)bc |
| Size | ~163,600 ly (50.16 kpc) (estimated) |
| Apparent size (V) | 3.100′ × 1.116′ |
| Other designations | |
| ESO 463- G 004, IRAS 20312-3209, 2MASX J20342056-3158512, IC 5015, MCG -05-48-022, PGC 64980 | |
NGC 6925 is an unbarred spiral galaxy in the constellation Microscopium. Its velocity with respect to the cosmic microwave background is 2,572±15 km/s, which corresponds to a Hubble distance of 123.7 ± 8.7 Mly (37.93 ± 2.66 Mpc). However, 34 non-redshift measurements give a much closer mean distance of 92.94 ± 2.66 Mly (28.497 ± 0.817 Mpc). It was discovered by British astronomer John Herschel on 31 July 1834.
NGC 6925 is lens-shaped, as it lies almost edge on to observers on Earth. It lies 3.7 degrees west-northwest of Alpha Microscopii.
NGC 6925 is the main galaxy in a group of galaxies that bears its name. The NGC 6925 group (also known as LGG 437) has at least four galaxies, including NGC 6923, IC 5020 and ESO 462-31.
One supernova has been observed in NGC 6925. SN 2011ei (Type IIb, mag. 18) was discovered by Stuart Parker in New Zealand on 25 July 2011.