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| the angular distance of a heavenly body above the horizon |
| a star in an intermediate stage of evolution, characterized by a large volume, low surface temperature, and reddish hue |
| globular cluster | |
| —n | |
| astronomy a densely populated spheroidal star cluster with the highest concentration of stars near its centre, found in the galactic halo and in other galaxies | |
| globular cluster (glŏb'yə-lər) Pronunciation Key
A spherical mass made up of thousands to hundreds of thousands of densely packed stars of nearly the same age (typically very old). Globular clusters occupy the inner regions of a galactic halo and revolve around the nucleus of galaxies in highly elliptical orbits inclined to the disk of the spiral arms. There are approximately 150 of these clusters in the Milky Way. It is believed that globular clusters can provide information about the evolution and lifespan of stars. Compare open cluster. |