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NGC 411 (Open Cluster)


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NGC 411
Open Cluster (散開星団)
OC OCL

別名 (Other names)
ESO 51-SC19 in SMC

明るさ (Brightness)
12.2等級

星座 (Constellation)
きょしちょう座 (Tuc) (Tucana)

NGC 411 is an open cluster in the constellation Tucana.

NGC 411 (Open Cluster) : Picture

NGC411
NGC 411
(C) NASA/ESA/Hubble
Globular clusters are roughly spherical collections of extremely old stars, and around 150 of them are scattered around our galaxy. Hubble is one of the best telescopes for studying these, as its extremely high resolution lets astronomers see individual stars, even in the crowded core. The clusters all look very similar, and in Hubble’s images it can be quite hard to tell them apart – and they all look much like NGC 411, pictured here.

And yet appearances can be deceptive: NGC 411 is in fact not a globular cluster, and its stars are not old. It isn’t even in the Milky Way. NGC 411 is classified as an open cluster located in the Small Magellanic Cloud, a small sister galaxy near our own. Less tightly bound than a globular cluster, the stars in open clusters tend to drift apart over time as they age, whereas globulars have survived for well over 10 billion years of galactic history. NGC 411 is a relative youngster — not much more than a tenth of this age. Far from being a relic of the early years of the universe, the stars in NGC 411 are in fact a fraction of the age of the sun.

The stars in NGC 411 are all roughly the same age, having formed at one time from one cloud of gas. But they are not all the same size. Hubble’s image shows a wide range of colors and brightness in the cluster’s stars; these tell astronomers many facts about the stars, including their mass, temperature and evolutionary phase. Blue stars, for instance, have higher surface temperatures than red ones.
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