2023 A/L Physics Past Paper · Question 06 (English Medium)

Radiation when the temperature is doubled

If the absolute temperature of a blackbody is increased by 22 times, the energy radiated by the blackbody per unit time per unit area will increase by

  1. (1) two times.
  2. (2) four times.
  3. (3) eight times.
  4. (4) sixteen times.
  5. (5) thirty two times.
Answer and explanation

Answer: (4) sixteen times.

What the question asks

We want: how many times as big the energy radiated per unit time per unit area becomes, when the absolute temperature of a blackbody is made 22 times as big.

The paper says "increased by 22 times". It means the temperature becomes 22 times as big. The options are read the same way.

What each letter means:

EE (W m−2\text{W m}^{-2}): energy radiated per unit time per unit area.

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

σ\sigma (W m−2 K−4\text{W m}^{-2}\,\text{K}^{-4}): Stefan's constant.

Relevant theory

The total power radiated from a unit area of a hot black body is directly proportional to

the fourth power of the absolute temperature of the body.

Required equations

E=σT4E = \sigma T^4

Reasoning and calculation

What stays the same: the constant σ\sigma and the blackbody.

What changes: the absolute temperature TT, and with it the energy EE.

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

At first it glows a dull red. Then it glows bright orange, and every patch of it sends out much more heat and light each second.

It is not just a little more. The law says the energy goes with TT to the fourth power, so a small rise in TT makes a big rise in EE.

Write the law for the first temperature and for the second, then divide.

E1=σT14E2=σT24E_1 = \sigma T_1^4 \qquad E_2 = \sigma T_2^4

E2E1=(T2T1)4\dfrac{E_2}{E_1} = \left(\dfrac{T_2}{T_1}\right)^4

The constant σ\sigma cancels.

The new temperature is 22 times the old one.

T2T1=2\dfrac{T_2}{T_1} = 2

Put it in:

E2E1=24=16\dfrac{E_2}{E_1} = 2^4 = 16

Reading the options

The energy becomes 1616 times as big. That is option (4).

Options (1), (2), (3) and (5) are 212^1, 222^2, 232^3 and 252^5. Each uses the wrong power.

Checks

Dimension check:

E2E1\dfrac{E_2}{E_1} is W m−2\text{W m}^{-2} divided by W m−2\text{W m}^{-2}. The units cancel, so it is a pure number, as a count of times should be.

n∗n∗n∗nn * n * n * n

Does it make sense?

The temperature went up, so the energy must go up.

The factor must be more than 22, because the energy goes with the fourth power of TT. 1616 is more than 22.

Conclusion

E2E1=16\dfrac{E_2}{E_1} = 16

E2E1=(T2T1)4=24=16\dfrac{E_2}{E_1} = \left(\dfrac{T_2}{T_1}\right)^4 = 2^4 = 16.

The answer is (4).

Stefan's law has T4T^4. If TT becomes nn times as big, EE becomes n4n^4 times as big.

Write the ratio (T2T1)4\left(\dfrac{T_2}{T_1}\right)^4 and put in the number.

Exam tip

தமிழ் · සිංහල