Globular Cluster NGC 288
The globular cluster NGC 288 was first sighted on October 27, 1785 by the German-British astronomer Wilhelm Herschel with its 18.7 inch reflector. The cluster is a very loose association with a Shapley – Sawyer concentration class of X. [196, 277]
Like most globular clusters, NGC 288 is in an elliptical orbit around the galactic center, from which it is currently at a distance of 12 kpc (approx. 39'000 light years). The distance to us is only 8.5 kpc (approx. 27'000 light years). This orbit takes him through the galactic bulge and every time he passes it he loses stars. This creates a tidal tail on both sides of the cluster, which, however, due to the orbit and the position of the cluster in the apocenter, can hardly be made out from the earth. [369, 370, 371]
The different colors and brightnesses of the stars that can be seen in Fig. 1 tell the story of how they developed differently within the cluster. The many weaker points of light are normal stars with low mass, which fuse hydrogen to helium in the same way as our sun does. The brighter stars are divided into two classes: The yellow are red giants, which are in a later stage of their life and are now bigger, cooler and brighter. The bright blue stars are even more massive stars and are powered inside by the fusion of helium. Stars in a globular cluster all form at about the same time from the same gas cloud and are usually very old: 10 to 12 billion years. It is assumed that the stars in less dense clusters can develop differently. 
The globular cluster NGC 288 is located in the constellation Sculptor, about 2 ° southeast of the well-known Silver Dollar (NGC 253). Due to its southern location of -26.5° declination, it is only clearly visible in Central Europe from September to November.