Peering into the Core of a Globular Cluster
Astronomers have used NASA/ESA Hubble Space Telescope to peer into the centre of a dense swarm of stars called Omega Centauri. Located some 17, 000 light-years from Earth, Omega Centauri is a massive globular star cluster, containing several million stars swirling in locked orbits around a common centre of gravity. The stars are packed so densely in the cluster's core that it is difficult for ground-based telescopes to make out individual stars. Hubble's high resolution is able to pick up where ground-based telescopes leave off, capturing distinct points of light from stars at the very centre of the cluster.
Credit:About the Image
About the Object
| Name: | NGC 5139, Omega Centauri |
|---|---|
| Type: | Milky Way : Star : Grouping : Cluster : Globular |
| Distance: | 17000 light years |
| Constellation: | Centaurus |
| Category: | Star Clusters |
Coordinates
| Position (RA): | 13 26 51.06 |
|---|---|
| Position (Dec): | -47° 28' 54.02" |
| Field of view: | 2.45 x 2.44 arcminutes |
| Orientation: | North is 36.7° right of vertical |
Colours & filters
| Band | Wavelength | Telescope |
|---|---|---|
| Ultraviolet U | 336 nm |
Hubble Space Telescope
WFPC2 |
| Optical H-alpha | 656 nm |
Hubble Space Telescope
WFPC2 |
| Optical R | 675 nm |
Hubble Space Telescope
WFPC2 |

