Stefan's Law (OCR A Level Physics): Revision Note
Exam code: H556
Stefan's Law
An object's luminosity depends on:
its surface temperature
its surface area
The relationship between these is known as Stefan's law or the Stefan-Boltzmann law, which states:
The total energy emitted by a black body per unit area per second is proportional to the fourth power of the absolute temperature of the body
Stefan's law equation is given by:
Where:
L = luminosity of the star (W)
r = radius of the star
σ = the Stefan-Boltzmann constant
T = surface temperature of the star (K)
This equation shows that the luminosity of a star is directly proportional to:
the square of its radius
its surface area
the fourth power of its surface temperature
Worked Example
The surface temperature of Proxima Centauri, the nearest star to Earth, is 3000 K, and its luminosity is 6.506 × 1023 W.
Calculate the radius of Proxima Centauri, in km.
Answer:
Step 1: List the known quantities
Surface temperature, T = 3000 K
Luminosity, L = 6.506 × 1023 W
Stefan's constant, σ = 5.67 × 10−8 W m−2 K−4
Step 2: Write down Stefan's law
Step 3: Rearrange the equation for radius r
Step 4: Substitute the values into the equation
Step 5: Write the final answer in the correct unit
The radius of Proximal Centauri is
or
(4 s.f.)
Examiner Tips and Tricks
Remember to convert temperatures into Kelvin.
Check the values you obtain in your calculations. Do they make sense? Do they fit in with the magnitudes of other stars/objects that you know about?
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