Galaxy morphological classification scheme advocated by Edwin Hubble
The Hubble sequence is a morphological classification scheme for galaxies published by Edwin Hubble in 1926.[1][2][3][4] It is often colloquially known as the Hubble tuning-fork diagram because the shape in which it is traditionally represented resembles a tuning fork.
It was invented by John Henry Reynolds and Sir James Jeans.[5]
The tuning fork scheme divided regular galaxies into three broad classes – ellipticals, lenticulars and spirals – based on their visual appearance (originally on photographic plates). A fourth class contains galaxies with an irregular appearance. The Hubble sequence is the most commonly used system for classifying galaxies, both in professional astronomical research and in amateur astronomy.
^Hubble, E.P. (1926). "Extra-galactic nebulae". Contributions from the Mount Wilson Observatory / Carnegie Institution of Washington. 324: 1–49. Bibcode:1926CMWCI.324....1H.
^Block, David L.; Freeman, Ken C. (2015) [14 November 2014]. Freeman, Kenneth; Elmegreen, Bruce; Block, David; Woolway, Matthew (eds.). Lessons from the Local Group. 2014 International conference honoring David Block and Bruce Elmegreen, focusing on the Local Group as an example of galactic-scale processes (softcover ed.). Switzerland: Springer Cham / Springer International Publishing (published 10 September 2016). pp. 1–20. Bibcode:2015llg..book....1B. doi:10.1007/978-3-319-10614-4_1. ISBN978-3-319-37812-1; (hardcover ed.) ISBN978-3-319-10613-7 (published 3 December 2014); "ADS abstract". NASA / Astrophysics Data System. Harvard University. 2015. Bibcode:2015llg..book....1B.