CDD Images of Globular (Star) Clusters
[The thumbnail images are links to detail pages]
Star Clusters are collections of stars that formed from the same gas cloud and are gravitationally bound to each other. A star is a sun, a large sphere of gas that makes and emits its own radiation - they form from dust and gas in space. Stars are enourmous nuclear reactors and they shine because of nuclear fusion.
There are two main types of star clusters.
Globular Clusters
- These clusters are found in the halos of galaxies and could contain between tens of thousands to millions of ancient stars (suns) that are seen as a spherical group. Globulars are spherically symmetrical groups of old stars that share a common source. They can have tens of thousands to millions of stars and are tightly bound by gravity. The Milky Way has about 150 globulars.
Open Clusters
- These are found in the disks of galaxies and could contain up to hundreds of young stars (suns) in a loosely bound (spread out) configuration.