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The Hubble sequence is a morphological classification scheme for galaxies published by Edwin Hubble in 1926. 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.
Classes of galaxies, Shortcomings & Physical significance
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galaxies hubble spiral galaxy sequence lenticular classification appearance spirals ellipticals elliptical classes irregular scheme bulge structure ellipticity stars barred lenticulars
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Hubble sequence | is a | morphological classification scheme for galaxies published by Edwin Hubble in 1926 | 0.90 | text |
| Hubble sequence | is a | most commonly used system for classifying galaxies | 0.90 | text |
| Hubble sequence | related to Irregulars | Galaxies | 0.60 | section |
| Hubble sequence | related to Irregulars | Hubble | 0.60 | section |
| Hubble sequence | related to Irregulars | Irr | 0.60 | section |
| Hubble sequence | related to Irregulars | II | 0.60 | section |
| Hubble sequence | related to Physical significance | Elliptical | 0.60 | section |
| Hubble sequence | related to Physical significance | This | 0.60 | section |
| Hubble sequence | related to Physical significance | Hubble | 0.60 | section |
| Hubble sequence | related to Physical significance | In | 0.60 | section |
| Hubble sequence | related to Physical significance | The | 0.60 | section |
| Hubble sequence | related to Physical significance | Universe | 0.60 | section |
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