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sun temperature - перевод на голландский
![The effective temperature of the [[Sun]] (5777 [[kelvin]]s) is the temperature a black body of the same size must have to yield the same total emissive power.](https://commons.wikimedia.org/wiki/Special:FilePath/EffectiveTemperature 300dpi e.png?width=200 "The effective temperature of the [[Sun]] (5777 [[kelvin]]s) is the temperature a black body of the same size must have to yield the same total emissive power.")
![[[Joseph Louis Gay-Lussac]]](https://commons.wikimedia.org/wiki/Special:FilePath/Gaylussac.jpg?width=200 "[[Joseph Louis Gay-Lussac]]")
![[[Guillaume Amontons]]](https://commons.wikimedia.org/wiki/Special:FilePath/Guillaume Amontons, wood cutting.png?width=200 "[[Guillaume Amontons]]")
![[[Johann Heinrich Lambert]]](https://commons.wikimedia.org/wiki/Special:FilePath/JHLambert.jpg?width=200 "[[Johann Heinrich Lambert]]")
![[[Jacques Alexandre César Charles]]](https://commons.wikimedia.org/wiki/Special:FilePath/Jacques Charles.jpg?width=200 "[[Jacques Alexandre César Charles]]")
![[[Macquorn Rankine]]](https://commons.wikimedia.org/wiki/Special:FilePath/Rankine William signature.jpg?width=200 "[[Macquorn Rankine]]")
![A Sun [[server rack]] at the Computer Museum of America in [[Roswell, Georgia]]](https://commons.wikimedia.org/wiki/Special:FilePath/Computer Museum of America (43).jpg?width=200 "A Sun [[server rack]] at the Computer Museum of America in [[Roswell, Georgia]]")
![Sun in [[Markham, Ontario]], Canada](https://commons.wikimedia.org/wiki/Special:FilePath/SunCanada.jpg?width=200 "Sun in [[Markham, Ontario]], Canada")
![Sun [[server rack]]s at [[Seneca College]] (York Campus)](https://commons.wikimedia.org/wiki/Special:FilePath/SunRackMountServers.jpg?width=200 "Sun [[server rack]]s at [[Seneca College]] (York Campus)")
![[[VirtualBox]], purchased by Sun](https://commons.wikimedia.org/wiki/Special:FilePath/VirtualBox2.png?width=200 "[[VirtualBox]], purchased by Sun")
Определение
Википедия
The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation. Effective temperature is often used as an estimate of a body's surface temperature when the body's emissivity curve (as a function of wavelength) is not known.
When the star's or planet's net emissivity in the relevant wavelength band is less than unity (less than that of a black body), the actual temperature of the body will be higher than the effective temperature. The net emissivity may be low due to surface or atmospheric properties, including greenhouse effect.
