Open Star Clusters
Like dazzling jewels set against the black velvet of deep space, open (or galactic) star clusters showcase glittering new stars as they emerge from their dusky birth in giant molecular clouds.
The Basics
• As a giant cloud of gas and dust coalesces in the arms of a spiral galaxy, tiny clumps in the cloud collapse and ignite into groups of hundreds to thousands of young stars. The hottest of these stars light up the remaining gas and dust, resulting in glowing gas clouds like the Carina and Orion nebulae.
• After several million years, the hottest stars of the new cluster blow off the remaining gas and dust. What remains is a group of dazzling new stars loosely held together by gravity.
• Over many tens of millions of years, as the cluster revolves around the galaxy, it encounters other stars and dust clouds that disrupt the cluster and eject its members into the spiral arms of the galaxy. There, they continue to revolve about the galactic center by themselves or in loose “stellar associations”. Some of the stars of Ursa Major are part of an association and were once members of an open cluster.
A Deeper Look
• Open star clusters are only found near the arms of spiral and irregular galaxies, where there is abundant gas and dust. Elliptical galaxies no longer have enough gas and dust to sustain the creation of new stars.
• The greatest concentration of open clusters in our skies lies along the Milky Way in Cygnus, Scutum, Scorpius, and Sagittarius. For that reason, open clusters are sometimes called “galactic clusters”.
• Most open clusters stay together for a few tens of millions of years. One of the oldest is the lovely Beehive cluster. It was massive enough at birth to hold itself together for nearly four hundred million years.
• There are nearly 1000 known open clusters in our skies, and likely 10,000 more hidden behind the disk of our galaxy. Some famous open clusters: Pleiades (M45), Beehive (M44), Hyades, and the Double Cluster in the constellation Perseus.
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