Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  HD236783  ·  HD236789  ·  HD9145  ·  HD9146  ·  HD9311  ·  HD9365  ·  HD9518  ·  M 103  ·  NGC 581
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M 103 - Open Cluster in Cassiopeia, Monty Chandler
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M 103 - Open Cluster in Cassiopeia, Monty Chandler
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Description

Messier 103 (M 103) is a small open star cluster in the northern constellation Cassiopeia. It's about 9,000 light-years from Earth and is one of the smallest and most remote open clusters known. It contains 172 confirmed members. 

The brightest stars in the cluster have a visual magnitude of 10.5 and belong to spectral classes B5 Ib and B2 III, which means that they are a supergiant and giant star, both white-blue in color. Most of the cluster’s brightest members are young, hot, blue stars. At the centre of the cluster, there is a prominent red giant with a visual magnitude of 10.8. The star is classified as belonging to the spectral class M6 III or gM6.

Messier 103 is moving toward us at 37 km/s. The estimated age of the cluster is about 25 million years, only 30 percent of the age of the Pleiades (M45). 

M103 occupies an area 6 arc minutes in apparent size, corresponding to a linear diameter of 17.5 light years. It is easy to see, even with binoculars, and appears as a nebulous fan-shaped patch.   4-inch telescopes resolve the four brightest stars in the cluster. Large telescopes resolve more stars across the cluster, but make it harder to make out M103 from the surrounding star field because the cluster is quite loose. 

This image is from an 8" telescope and the rich star-field is very apparent, but the bright blue stars from M 103 stand out to me, as does the red giant in the center.

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M 103 - Open Cluster in Cassiopeia, Monty Chandler