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The Star Cluster NGC 2100
in the Large Magellanic Cloud
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Name: NGC 2100
Description: Open Star Cluster
Position: RA 5h 42m 8.06s Dec -69° 12' 42.83"
Constellation: Dorado
Distance: 170,000 light years
Field of view: 8.66 x 8.66 arcminutes
Orientation: North is 0.7° left of vertical
Image Credit: ESO
Release Date: September 7, 2011
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ESO’s New Technology Telescope (NTT) has captured a striking image of the open cluster NGC 2100. This brilliant star cluster is around 15 million years old, and located in the Large Magellanic Cloud, a nearby satellite galaxy of the Milky Way. The cluster is surrounded by glowing gas from the nearby Tarantula Nebula.

Observers often overlook NGC 2100 because of its close proximity to the impressive Tarantula Nebula (eso0650) and the super star cluster RMC 136 (eso1030). The glowing gas of the Tarantula Nebula even tries to steal the limelight in this image — the bright colors here are the nebula’s outskirts. This new picture was created from exposures through several different color filters using the ESO Multi Mode instrument on the New Technology Telescope at ESO’s La Silla Observatory in Chile. The stars are shown in their natural colours, while light from glowing ionized hydrogen (shown here in red) and oxygen (shown in blue) is overlaid.

The colors that appear in nebulae depend on the temperatures of the stars lighting them up. The hot young stars in the Tarantula Nebula, which lie in the super star cluster RMC 136, are above and to the right of this image, and are powerful enough to cause oxygen to glow showing up as blue nebulosity in this picture[1]. Below NGC 2100 the red glow indicates either that the outer reaches of the influence of the hot stars of RMC 136 has been reached, or that cooler, and older, stars, that are only able to excite hydrogen are the dominant influence in this region. The stars that make up NGC 2100 are older and less energetic, and hence have little or no nebulosity associated with them.

Star clusters are groups of stars that formed around the same time from a single cloud of gas and dust. The stars with the most mass tend to form in the center of the cluster, while those with less mass dominate the outer regions. This, along with the greater number of stars concentrated in the center, makes the middle of the cluster brighter than the outer regions.

NGC 2100 is an open cluster, which means its stars are relatively loosely bound by gravity. These clusters have a lifespan measured in tens or hundreds of millions of years, as they eventually disperse through gravitational interaction with other bodies. Globular clusters, which look similar to the untrained eye, contain many more older stars and are much more tightly bound, and so have far longer lifespans: many globular clusters have been measured to be almost as old as the Universe itself. So while NGC 2100 might be older than its neighbors in the Large Magellanic Cloud, it is still a youngster by the standards of star clusters.


[1] Most of the glow from oxygen comes from oxygen atoms that have lost two electrons. This strong emission is very common in nebulae but was mysterious to early astronomical spectroscopists and was initially thought to be coming from a new element given the name Nebulium.