Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  M 103  ·  NGC 581  ·  PK127-01.1
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M103 Open Cluster in Cassiopeia, autonm
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M103 Open Cluster in Cassiopeia

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M103 Open Cluster in Cassiopeia, autonm
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M103 Open Cluster in Cassiopeia

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Description

Newcastle, UK

M103 Open Cluster in Cassiopeia

Messier 103 is an *open cluster where a few hundred, mainly very faint, stars figure in Cassiopeia. It is one of the more distant open clusters, 8,000 to 9,500 light-years from the solar system and ranging over about 15 light years.

It holds about 40 certain-member stars, two of which have magnitudes 10.5, and a 10.8 red giant, which is the brightest within the cluster. A bright known foreground object is the star Struve 131, not a member of the cluster.

The cluster may have 172 stars if including those down to 50% probability of a gravitational tie. M103 is about 25 million years old.



*An open cluster is a type of star cluster made of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age. More than 1,100 open clusters have been discovered within the Milky Way Galaxy, and many more are thought to exist.

They are loosely bound by mutual gravitational attraction and become disrupted by close encounters with other clusters and clouds of gas as they orbit the galactic center. This can result in a migration to the main body of the galaxy and a loss of cluster members through internal close encounters.

Open clusters generally survive for a few hundred million years, with the most massive ones surviving for a few billion years. In contrast, the more massive globular clusters of stars exert a stronger gravitational attraction on their members, and can survive for longer. Open clusters have been found only in spiral and irregular galaxies, in which active star formation is occurring.

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M103 Open Cluster in Cassiopeia, autonm