| NGC 3904 | |
|---|---|
| Observation data (J2000.0 epoch) | |
| Constellation | Hydra |
| Right ascension | 11h 49m 13,2s |
| Declination | −29° 16′ 36″ |
| Redshift | 0.005257 |
| Heliocentric radial velocity | 1576 ± 8 |
| Distance | 72 million LY |
| Apparent magnitude (V) | 10.96 |
| Characteristics | |
| Type | E2 |
| Apparent size (V) | 2.70 x 2.0 |
| Other designations | |
| PGC 36918 | |
NGC 3904 is an elliptical galaxy in the constellation Hydra. It was observed both by astronomers William Herschel in 1791 and John Herschel in 1834, respectively. The galaxy's radial velocity, relative to the cosmic microwave background is measured at around 1915 ± 25 km/s, corresponding to a Hubble distance of around 28.25 ± 2.02 MPC.
NGC 3904 exhibits no detectable neutral hydrogen or radio emissions, indicating a lack of ongoing star formation. It also hosts a system of globular clusters with relatively lower metallicity and bluer colors than those in bigger elliptical galaxies.
One supernova has been observed within the galaxy NGC 3904:
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