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The solar luminosity (L☉) is a unit of radiant flux (power emitted in the form of photons) conventionally used by astronomers to measure the luminosity of stars, galaxies and other celestial objects in terms of the output of the Sun.
Measurement, Determination & Overview
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solar luminosity sun irradiance variations bibcode doi s2cid power constant 10 unit emitted one defined astronomical exactly causes variation arxiv
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Solar luminosity | related to Determination | Solar | 0.60 | section |
| Solar luminosity | related to Determination | Slow | 0.60 | section |
| Solar luminosity | related to Determination | The | 0.60 | section |
| Solar luminosity | related to Determination | Milankovitch | 0.60 | section |
| Solar luminosity | related to Determination | Earthly | 0.60 | section |
| Solar luminosity | related to Determination | Earth's | 0.60 | section |
| Solar luminosity | related to Determination | Irradiance | 0.60 | section |
| Solar luminosity | related to Determination | Sun | 0.60 | section |
| Solar luminosity | related to Determination | Earth | 0.60 | section |
| Solar luminosity | related to External links | LISIRD | 0.60 | section |
| Solar luminosity | related to External links | LASP Interactive Solar Irradiance | 0.60 | section |
| Solar luminosity | related to External links | DatacenterStellar Luminosity CalculatorSolar LuminosityVariation | 0.60 | section |
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