Hydra–Centaurus Supercluster
| Hydra–Centaurus Supercluster | |
|---|---|
Three-dimensional map of the Hydra Supercluster | |
| Observation data (Epoch J2000) | |
| Right ascension | 13h 14m 00.0s |
| Declination | −33° 18′ 00″ |
| Parent structure | Laniakea Supercluster |
| Redshift | 0.016000 (4,797 km/s) |
| Distance | ~39–69.4 Mpc (127–226 Mly) |
| Other designations | |
| Cen-Hya Supercluster, Hydra-Cen Supercluster, Hydra-Centaurus Supercluster, SCI 128 | |
The Hydra–Centaurus Supercluster (SCl 128), or the Hydra and Centaurus Superclusters, was a previously defined supercluster in two parts, which prior to the identification of Laniakea Supercluster in 2014 is the closest neighbour of the former Virgo Supercluster. Its center is located about 39 Mpc (127 Mly) away, with it extending to a maximum distance of around 69 Mpc (225 Mly).