Double Cluster

open star cluster From Wikipedia, the free encyclopedia

Double Cluster

The Double Cluster, is NGC 884 and NGC 869, a group of two open star clusters in the Perseus constellation. It has many blue and red stars.

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The Double Cluster

Both are visible with the naked eye. NGC 869 and NGC 884 lie at a distance of 7,500 light years.[1] That is relatively close-by (the Milky Way galaxy has a diameter of roughly 100,000 light years.)

Stars

RS Persei and T Persei

These are two red supergiant stars in the star cluster. They are 770 and 510 times larger than the Sun respectively.[2]

SU Persei and AV Persei

These are also red supergiant stars. They both are 780 and 770 times larger than the Sun respectively.[3]

S Persei

A red hypergiant 1,212 times larger than the Sun.[4]

References

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