2022 A/L Physics Past Paper · Question 08 (English Medium)

Peak wavelength of a hotter blackbody

The surface temperature of the sun is 6000 K6000\ \text{K} and it emits blackbody radiation at peak wavelength 500 nm500\ \text{nm}. For a blackbody with a surface temperature of 10 000 K10\,000\ \text{K}, what will be the value of peak wavelength of emitted radiation?

  1. (1) 30 nm30\ \text{nm}
  2. (2) 300 nm300\ \text{nm}
  3. (3) 500 nm500\ \text{nm}
  4. (4) 600 nm600\ \text{nm}
  5. (5) 800 nm800\ \text{nm}
Answer and explanation

Answer: (2) 300 nm300\ \text{nm}

What the question asks

We want: the peak wavelength of a blackbody at 10 000 K10\,000\ \text{K}, when the sun at 6000 K6000\ \text{K} peaks at 500 nm500\ \text{nm}.

What each letter means:

λm\lambda_m (nm\text{nm}): wavelength of the peak of the radiation.

TT (K\text{K}): absolute temperature of the blackbody.

CC (m K\text{m K}): the constant in Wien's displacement law.

Relevant theory

In the spectral distribution of black body radiation, the product of the wavelength

relevant to the maximum intensity and the relevant absolute temperature is constant.

Required equations

λmT=C\lambda_m T = C

Reasoning and calculation

What stays the same: the constant CC, for every blackbody.

What changes: the temperature TT, and with it the peak wavelength λm\lambda_m.

For example, watch an electric stove ring as it warms up.

At first it glows a dull red. As it gets hotter it turns orange, then yellowish white.

Red light has a long wavelength. Yellow-white light has a shorter wavelength.

So a hotter body peaks at a shorter wavelength.

λmT=C\lambda_m T = C

In words: peak wavelength times absolute temperature is always the same constant.

If TT goes up, λm\lambda_m must come down by the same factor.

The constant CC is the same for the sun and for the second blackbody.

λ1T1=λ2T2\lambda_1 T_1 = \lambda_2 T_2

Solve for the new peak wavelength:

λ2=λ1T1T2\lambda_2 = \dfrac{\lambda_1 T_1}{T_2}

Put in the numbers:

λ2=500 nm×6000 K10 000 K\lambda_2 = \dfrac{500\ \text{nm} \times 6000\ \text{K}}{10\,000\ \text{K}}

λ2=300 nm\lambda_2 = 300\ \text{nm}

Reading the options

The value 300 nm300\ \text{nm} is option (2).

Option (5), 800 nm800\ \text{nm}, comes from using the ratio upside down.

Checks

Dimension check:

The unit of λ2\lambda_2 is nm×K÷K=nm\text{nm} \times \text{K} \div \text{K} = \text{nm}, a length, as it should be.

(l1∗t1)/t2(l1 * t1) / t2

Does it make sense?

The temperature went up from 6000 K6000\ \text{K} to 10 000 K10\,000\ \text{K}.

So the peak wavelength must go down. 300 nm300\ \text{nm} is less than 500 nm500\ \text{nm}.

Conclusion

λ2=300 nm\lambda_2 = 300\ \text{nm}

λ2=λ1T1T2=500×600010 000=300 nm\lambda_2 = \dfrac{\lambda_1 T_1}{T_2} = \dfrac{500 \times 6000}{10\,000} = 300\ \text{nm}.

The answer is (2).

Hotter means a shorter peak wavelength. The product λmT\lambda_m T never changes.

Write λ1T1=λ2T2\lambda_1 T_1 = \lambda_2 T_2 and solve.

Exam tip

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