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In astronomy, the bolometric correction is the correction made to the absolute visual magnitude of an object in order to convert it to an absolute bolometric magnitude. It is large for stars which radiate most of their energy outside of the visible range. A uniform scale for the correction has not yet been standardized.
Standards, Setting the correction scale & Description
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bolometric correction absolute magnitude sun scale bol displaystyle text different range adopted systematic zero made visual large stars energy visible
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Bolometric correction | is a | correction made to the absolute visual magnitude of an object in order to convert it to an absolute bolometric magnitude | 0.90 | text |
| Bolometric correction | is a | correction made to the absolute magnitude of an object in order to convert an object's visible magnitude to its bolometric magnitude.Alternatively | 0.90 | text |
| Bolometric correction | related to Description | Mathematically | 0.60 | section |
| Bolometric correction | related to Description | BC | 0.60 | section |
| Bolometric correction | related to Description | The | 0.60 | section |
| Bolometric correction | related to External links | HR | 0.60 | section |
| Bolometric correction | related to External links | Astronomy/SteMag | 0.60 | section |
| Bolometric correction | related to External links | Sun | 0.60 | section |
| Bolometric correction | related to Setting the correction scale | The | 0.60 | section |
| Bolometric correction | related to Setting the correction scale | Sun | 0.60 | section |
| Bolometric correction | related to Setting the correction scale | Hence | 0.60 | section |
| Bolometric correction | related to Setting the correction scale | This | 0.60 | section |
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