M34 open cluster

M34, or Messier 34, is an open star cluster located in the constellation Perseus, about 1,500 light-years away from Earth. It’s one of the nearest and best-studied open clusters and is relatively young, with an estimated age of around 200 to 250 million years.
Containing about 100 stars, M34 is visible to the naked eye in dark skies and easy to observe through binoculars or small telescopes. The cluster’s stars are loosely bound by gravity, which is typical for open clusters, and they share a common origin, having formed from the same molecular cloud. M34 spans about 15 light-years across, and its brighter stars are mostly main-sequence stars, though it does contain a few red giants.
Due to its brightness, proximity, and wide star distribution, M34 is popular among amateur astronomers and offers a good opportunity for studying stellar evolution and dynamics within open clusters.
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