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Open cluster information


Open cluster
The Pleiades is one of the most famous open clusters.
Characteristics
TypeLoose cluster of stars
Size range< 30 ly in diameter
Density~ 1.5 stars / cubic ly
External links
inline Media category
inline Q11387
Additional Information

An open cluster is a type of star cluster made of tens 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.[1] Each one is loosely bound by mutual gravitational attraction and becomes disrupted by close encounters with other clusters and clouds of gas as they orbit the Galactic Center. This can result in a loss of cluster members through internal close encounters and a dispersion into the main body of the galaxy.[2] 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.[3]

Young open clusters may be contained within the molecular cloud from which they formed, illuminating it to create an H II region.[4] Over time, radiation pressure from the cluster will disperse the molecular cloud. Typically, about 10% of the mass of a gas cloud will coalesce into stars before radiation pressure drives the rest of the gas away.

Open clusters are key objects in the study of stellar evolution. Because the cluster members are of similar age and chemical composition, their properties (such as distance, age, metallicity, extinction, and velocity) are more easily determined than they are for isolated stars.[1] A number of open clusters, such as the Pleiades, the Hyades and the Alpha Persei Cluster, are visible with the naked eye. Some others, such as the Double Cluster, are barely perceptible without instruments, while many more can be seen using binoculars or telescopes. The Wild Duck Cluster, M11, is an example.[5]

  1. ^ a b Cite error: The named reference seds was invoked but never defined (see the help page).
  2. ^ Cite error: The named reference Karttunen_et_al_03 was invoked but never defined (see the help page).
  3. ^ Cite error: The named reference payne-gaposchkin79 was invoked but never defined (see the help page).
  4. ^ Cite error: The named reference apj62 was invoked but never defined (see the help page).
  5. ^ Cite error: The named reference neata09 was invoked but never defined (see the help page).

and 28 Related for: Open cluster information

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Open cluster

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An open cluster is a type of star cluster made of tens to a few thousand stars that were formed from the same giant molecular cloud and have roughly the...

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Pleiades

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45, and other names by different cultures, is an asterism and an open star cluster containing middle-aged, hot B-type stars in the north-west of the...

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Beehive Cluster

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The Beehive Cluster (also known as Praesepe (Latin for "manger", "cot" or "crib"), M44, NGC 2632, or Cr 189), is an open cluster in the constellation Cancer...

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Open Cluster Framework

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Open Cluster Framework (OCF) is a set of standards for computer clustering. The project started as a working group of the Free Standards Group, now part...

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Messier 93

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Messier 93 or M93, also known as NGC 2447 or the Critter Cluster, is an open cluster in the modestly southern constellation Puppis, the imagined poop...

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Star cluster

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millions of old stars which are gravitationally bound. Open clusters are more loosely clustered groups of stars, generally containing fewer than a few...

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List of open clusters

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This is a list of open clusters located in the Milky Way. An open cluster is an association of up to a few thousand stars that all formed from the same...

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Messier 7

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and sometimes known as the Ptolemy Cluster, is an open cluster of stars in the constellation of Scorpius. The cluster is easily detectable with the naked...

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Butterfly Cluster

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The Butterfly Cluster (cataloged as Messier 6 or M6, and as NGC 6405) is an open cluster of stars in the southern constellation of Scorpius. Its name derives...

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Globular cluster

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A globular cluster is a spheroidal conglomeration of stars that is bound together by gravity, with a higher concentration of stars towards their centers...

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Open cluster family

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astronomy, an open cluster family is a group of approximately coeval (age range ∼ {\displaystyle \sim } 30 Myr) young open star clusters located in a relatively...

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Wild Duck Cluster

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The Wild Duck Cluster (also known as Messier 11, or NGC 6705) is an open cluster of stars in the constellation Scutum (the Shield). It was discovered by...

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Messier 67

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or NGC 2682) and sometimes called the King Cobra Cluster or the Golden Eye Cluster is an open cluster in the southern, equatorial half of Cancer. It was...

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Messier 103

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Messier 103 (also known as M103, or NGC 581) is a small open cluster of many faint stars in Cassiopeia. It was discovered on 27 March 1781 by Pierre Méchain...

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Messier object

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when all of the objects can be viewed over a single night.   Open cluster   Globular cluster   Diffuse nebula   Planetary nebula   Supernova remnant   Galaxy...

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Robert Julius Trumpler

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is most noted for observing that the brightness of the more distant open clusters was lower than expected, and the stars appeared more red. This was explained...

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Messier 26

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is an open cluster of stars in the southern constellation of Scutum. It was discovered by Charles Messier in 1764. This 8th magnitude cluster is a challenge...

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NGC 457

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known as the Dragonfly Cluster, E.T. Cluster, Owl Cluster, Kachina Doll Cluster or Phi Cassiopeiae Cluster) is an open star cluster in the constellation...

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Messier 52

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Messier 52 or M52, also known as NGC 7654 or the Scorpion Cluster, is an open cluster of stars in the highly northern constellation of Cassiopeia. It...

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Messier 34

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Messier 34 (also known as M34, NGC 1039, or the Spiral Cluster) is a large and relatively near open cluster in Perseus. It was probably discovered by Giovanni...

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NGC 2264

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and the Christmas Tree Cluster. Two other objects are within this designation but not officially included, the Snowflake Cluster, and the Fox Fur Nebula...

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Open cluster remnant

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In astronomy, an open cluster remnant (OCR) is the final stage in the evolution of an open star cluster. Viktor Ambartsumian (1938) and Lyman Spitzer (1940)...

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Messier 35

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35 or M35, also known as NGC 2168 or the Shoe-Buckle Cluster, is a relatively close open cluster of stars in the west of Gemini, at about the declination...

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Messier 37

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(also known as M37, NGC 2099, or the Salt and Pepper Cluster) is the brightest and richest open cluster in the constellation Auriga. It was discovered by...

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Messier 25

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as IC 4725, is an open cluster of stars in the southern constellation of Sagittarius. The first recorded observation of this cluster was made by Philippe...

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Cluster

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halo of the parent galaxy Open cluster, a spherical collection of stars that orbits a galaxy in the galactic plane Cancer cluster, in biomedicine, an occurrence...

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Messier 21

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Messier 21 or M21, also designated NGC 6531 or Webb's Cross, is an open cluster of stars located to the north-east of Sagittarius in the night sky, close...

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Messier 36

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Messier 36 or M36, also known as NGC 1960 or the Pinwheel Cluster, is an open cluster of stars in the somewhat northern Auriga constellation. It was discovered...

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