Boneyard Tools

Stellar Luminosity Calculator

Enter a star's radius and effective temperature to find its luminosity from the Stefan-Boltzmann law, both in watts and as a multiple of the Sun.

How to use the luminosity calculator

  1. Enter the star's radius in metres, or start from the Sun preset.
  2. Enter the effective surface temperature in kelvin.
  3. Read the luminosity in watts and in solar luminosities.

Examples

Luminosity of the Sun

radius = 6.957e8 m, temperature = 5772 K
L = about 3.83e26 W (1 solar luminosity)

A hotter, larger star

radius = 1.3914e9 m, temperature = 10000 K
L = about 1.38e28 W (36 solar luminosities)

Frequently asked questions

What is luminosity?

Luminosity is the total power a star radiates into space across all wavelengths, measured in watts. It does not depend on how far away the star is.

What is the Stefan-Boltzmann luminosity formula?

L = 4 x pi x r^2 x sigma x T^4, where r is the radius, sigma is the Stefan-Boltzmann constant and T is the effective surface temperature in kelvin.

Why does temperature matter so much?

Luminosity scales with temperature to the fourth power, so doubling the temperature makes a star 16 times brighter for the same size.

What temperature should I use?

Use the effective temperature in kelvin, the blackbody temperature that reproduces the star's output. The Sun's is about 5772 K.

What is a solar luminosity?

One solar luminosity is the Sun's output, about 3.828e26 watts. Expressing results in solar units makes it easy to compare stars at a glance.

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