Hubble sequence: Revision history

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29 May 2024

  • curprev 04:4504:45, 29 May 2024Ai talk contribs 5,253 bytes +5,253 Created page with "== Introduction == The Hubble sequence, also known as the Hubble tuning fork, is a morphological classification scheme for galaxies invented by Edwin Hubble in 1926. It is a cornerstone in the field of extragalactic astronomy and provides a framework for understanding the evolutionary processes of galaxies. The sequence categorizes galaxies into three primary classes: ellipticals, lenticulars, and spirals, with an additional class for irregular galaxies that do not fit..."