Star clusters

The nebula NGC 3603

Star clusters

Stars tend to form together in one of two types of cluster. Globular clusters typically have a thousand or more old stars that form a symmetrical, sphere-like shape. The stars in open clusters are relatively young and fewer in number.

The stars in any one cluster are related to one another by their common origin – they are all believed to have formed at roughly the same time from the same cloud of gas and dust.

When the stars in an open cluster are less tightly packed, they are called an association.

Image: Thousands of stars inside the giant nebula NGC 3603 (credit: NASA, ESA, and the Hubble Heritage STScI/AURA-ESA/Hubble Collaboration)

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The nebula NGC 3603

Introduction

Stars often grow up in a group.

About Star clusters

Star clusters or star clouds are groups of stars. Two types of star clusters can be distinguished: globular clusters are tight groups of hundreds of thousands of very old stars which are gravitationally bound, while open clusters, more loosely clustered groups of stars, generally contain fewer than a few hundred members, and are often very young. Open clusters become disrupted over time by the gravitational influence of giant molecular clouds as they move through the galaxy, but cluster members will continue to move in broadly the same direction through space even though they are no longer gravitationally bound; they are then known as a stellar association, sometimes also referred to as a moving group.

Star clusters visible to the naked eye include Pleiades, Hyades and the Beehive Cluster.

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