Definition
A globular cluster is a dense spherical collection of 105–106 stars orbiting a galaxy. Their origin is poorly understood. About 160 globular clusters are known in the Milky Way, while the giant elliptical galaxy M87 may have up to 10,000. In the case of the Milky Way, they are composed of old (∼12 Gyr) and thus low-mass stars, with low abundances of elements heavier than He, similar to those of field halo stars. Their high internal density (up to 1,000 stars per pc3 in the cluster core) favors dynamical interactions between stars and makes the survival of any planetary system problematic.
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© 2014 Springer-Verlag Berlin Heidelberg
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Prantzos, N. (2014). Globular Cluster. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_651-3
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DOI: https://doi.org/10.1007/978-3-642-27833-4_651-3
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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