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STELLAR CHEMISTRY
Young Stars Take a Turn in the Spotlight
by Staff Writers
Munich, Germany (SPX) Sep 09, 2011


The brilliant star cluster NGC 2100 lies in the Large Magellanic Cloud, a small satellite galaxy of the Milky Way. This image was taken with the EMMI instrument on the ESO New Technology Telescope (NTT) at the La Silla Observatory in Chile. This star cluster lies close to the Tarantula Nebula and some of the colourful outer parts of the nebula appear in this image. The smaller cluster, close to the right-hand edge of the picture and just below centre, is NGC 2092. More images and detailed captions available at ESO

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 and the super star cluster RMC 136. 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 EMMI instrument on the New Technology Telescope at ESO's La Silla Observatory in Chile. The stars are shown in their natural colors, 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.

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 life spans: 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.

Data for this image of the under-appreciated young cluster were selected from the depths of ESO's data archives by Hidden Treasures entrant David Roma as part of the astrophotography competition held by ESO in 2010.

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Related Links
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Stellar Chemistry, The Universe And All Within It






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