Celestial hemisphere:  Northern  ·  Constellation: Cygnus (Cyg)  ·  Contains:  M 39  ·  NGC 7092
M39 / NGC 7092 Open Cluster in Cygnus, autonm
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M39 / NGC 7092 Open Cluster in Cygnus

M39 / NGC 7092 Open Cluster in Cygnus, autonm
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M39 / NGC 7092 Open Cluster in Cygnus

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Description

Newcastle, UK

Messier 39 (NGC 7092) *Open Cluster in Cygnus

When observed in a small telescope at low power the cluster shows around two dozen members.

It has a total integrated magnitude (brightness) of 5.5. It is centered about 1,010 light-years away.

This cluster has an estimated mass of 232 Solar Mass and a linear tidal radius of 8.6±1.8 pc. Of the 15 brightest components, six form binary star systems; one more is suspected. HD 205117 is a probable eclipsing binary system with a period of 113.2 days that varies by 0.051 in visual magnitude. Both members seem to be subgiants. Within are at least five chemically peculiar stars and ten suspected short-period variable stars.


*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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M39 / NGC 7092 Open Cluster in Cygnus, autonm