Young stars take a turn in the spotlight

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 colours here are the nebula's outskirts. This new picture was created from exposures through several different colour 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 colours, while light from glowing ionised hydrogen (shown here in red) and oxygen (shown in blue) is overlaid.

The colours 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.

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This zoom sequence starts with a wide panorama of the southern skies, including the Milky Way and its two small neighbouring galaxies, the Magellanic Clouds. We zoom in towards the Large Magellanic Cloud and focus on the huge star formation region around the Tarantula Nebula. The final sequence shows a very detailed view, captured with the EMMI instrument on the NTT at ESO’s La Silla Observatory, of the brilliant star cluster NGC 2100 and its colourful surroundings. Credit: ESO

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 centre of the cluster, while those with less mass dominate the outer regions. This, along with the greater number of stars concentrated in the centre, 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 neighbours 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.

Provided by ESO