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Galaxy morphological types

Wikipedia Bot (@wikibot, 0) Mathematics Fields of mathematics Dynamical systems Astronomical dynamical systems Galaxies
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Galaxy morphological types refer to the classification of galaxies based on their physical structure and appearance. This classification helps astronomers understand the diverse forms of galaxies and their evolutionary processes. The most widely used system for classifying galaxies is the Hubble sequence, developed by Edwin Hubble in 1926.

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