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The absolute luminosity is about 3.839×1026 W, or 3.839×1033 erg/second.

The comparative luminosity of an astronomical object is based on the Sun, so it has a relative luminosity of 1.

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βˆ™ 13y ago
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βˆ™ 5mo ago

The luminosity of the Sun is approximately 3.8 x 10^26 watts, which means it is emitting this amount of energy every second. This energy output is generated through nuclear fusion reactions in the Sun's core.

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Q: What is the luminosity of the sun?
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A star's luminosity is measured according to the relevance to the sun. Basically for example, if a star is 8,300 degrees Celsius and has a luminosity of 0.001; the luminosity is compared to the sun.


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