Stellar Luminosity Calculator
Calculate stellar luminosity using Stefan-Boltzmann law. Find absolute magnitude, main sequence lifetime, and stellar parameters.
Inputs
Results
Luminosity
1.004 Solar Luminosities
Absolute Magnitude
4.83
Main Sequence Lifetime
10,000,000,000 billion years
How to Use This Calculator
- Enter Stellar Radius (solar radii) — the Sun is 1 R☉; giants like Betelgeuse exceed 1,000 R☉.
- Enter Surface Temperature (K) from spectral classification: O stars >30,000 K, G stars ~5,000–6,000 K, M stars <3,500 K.
- Enter Stellar Mass (solar masses) to compute the Main Sequence Lifetime via the mass-luminosity relation.
- Read Luminosity (solar luminosities) and Absolute Magnitude to compare with catalog values.
- Use Main Sequence Lifetime (billion years) to understand how much longer the star will remain hydrogen-burning.
How the result changes with Surface Temperature
| Surface Temperature | Luminosity | Absolute Magnitude | Main Sequence Lifetime |
|---|---|---|---|
| 10,900 | 12.717 Solar Luminosities | 2.07 | 10,000,000,000 billion years |
| 35,650 | 1,455.231 Solar Luminosities | -3.08 | 10,000,000,000 billion years |
| 65,350 | 16,431.456 Solar Luminosities | -5.71 | 10,000,000,000 billion years |
| 90,100 | 59,373.526 Solar Luminosities | -7.1 | 10,000,000,000 billion years |
What each input means
- Stellar Radius
- Radius of the star
- Surface Temperature
- Effective surface temperature in Kelvin
- Stellar Mass
- Mass of the star
How this is calculated
Formula
L = 4πR²σT⁴ (Stefan-Boltzmann Law)Worked example, using the default values
- Identify Input ParametersStellar Radius = 1, Surface Temperature = 5778, Stellar Mass = 1 = 3 input(s) provided
- Calculate LuminosityLuminosity1.004 = 1.004
- Calculate Absolute MagnitudeAbsolute Magnitude4.83 = 4.83
- Calculate Main Sequence LifetimeMain Sequence Lifetime10000000000 = 10000000000
- Calculate Apparent MagnitudeApparent Magnitude4.83 = 4.83
- Calculate Surface FluxSurface Flux63200699.73 = 63200699.73
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