| Display title | Astronomy:Mass–luminosity relation |
| Default sort key | Mass-luminosity relation |
| Page length (in bytes) | 17,297 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 376001 |
| Page content language | en - English |
| Page content model | wikitext |
| Indexing by robots | Allowed |
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| Counted as a content page | Yes |
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| Edit | Allow all users (infinite) |
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| Page creator | imported>JTerm |
| Date of page creation | 13:29, 6 February 2024 |
| Latest editor | imported>JTerm |
| Date of latest edit | 13:29, 6 February 2024 |
| Total number of edits | 1 |
| Recent number of edits (within past 90 days) | 0 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | In astrophysics, the mass–luminosity relation is an equation giving the relationship between a star's mass and its luminosity, first noted by Jakob Karl Ernst Halm. The relationship is represented by the equation:
$ {\displaystyle {\frac {L}{L_{\odot }}}=\left({\frac {M}{M_{\odot }}}\right)^{a}} $
where... |
