**30.** Two spherical bodies of same materials having radii 0.2 m and 0.8 m are placed in the same atmosphere. The temperature of the smaller body is 800 K and the temperature of the bigger body is 400 K. If the energy radiated from the smaller body is \( E \), the energy radiated from the bigger body is (assume the effect of the surrounding to be negligible): - (1) 256 \( E \) - (2) \( E \) - (3) 64 \( E \) - (4) 16 \( E \)

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Published July 8, 2025
Physics
Thermal Physics
Heat Transfer
Radiation

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Detailed Explanation

Key concept – Stefan–Boltzmann law

For a perfect emitter (black body), the power radiated is

P=σAT4P = \sigma A T^4

where

  • σ\sigma is the Stefan–Boltzmann constant,
  • AA is the surface area,
  • TT is the absolute temperature in kelvin.

Because both spheres are of the same material and the surroundings are neglected, the emissivity factor is the same for both, so it cancels out in any ratio.

How a student should think step-by-step

  1. Recognise the formula → Radiation power PP depends on surface area and T4T^4.
  2. Write the surface area for a sphereA=4πr2A = 4\pi r^2.
  3. Set up a ratio of powers to avoid writing nasty constants.
    P2P1=σ(4πr22)T24σ(4πr12)T14=r22r12  T24T14\frac{P_2}{P_1} = \frac{\sigma (4\pi r_2^2) T_2^4}{\sigma (4\pi r_1^2) T_1^4} = \frac{r_2^2}{r_1^2}\;\frac{T_2^4}{T_1^4}
  4. Substitute the numbers (r1=0.2m,  T1=800K;  r2=0.8m,  T2=400Kr_1 = 0.2\,\text{m},\; T_1 = 800\,\text{K};\; r_2 = 0.8\,\text{m},\; T_2 = 400\,\text{K}) and simplify.
  5. Interpret the result → Compare with the given options.

Simple Explanation (ELI5)

Imagine two hot iron balls

  • One ball is tiny (radius of 0.2 m) but very hot at 800 K.
  • The other is big (radius of 0.8 m) but only warm at 400 K.

Both balls glow and throw out light and heat just like an electric bulb does.
How much heat they throw out each second depends on how large their glowing skin is and how hot that skin is.

Think of it like:

  1. Skin size → the larger the skin, the more spots to shine from.
  2. Temperature → the hotter it is, the brighter each spot shines, and this brightness grows very, very fast (temperature to the power four!).

Even though the big ball has more skin, it is cooler. The question is: does the big cool ball shine more, less, or the same as the small hot ball?

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Step-by-Step Solution

Step-by-step calculation

Surface area of a sphere:

A=4πr2A = 4\pi r^2

Power radiated by sphere:

P=σAT4=σ(4πr2)T4P = \sigma A T^4 = \sigma (4\pi r^2) T^4

Ratio of powers

Let the smaller sphere be (1) and the bigger sphere be (2).

P2P1=r22r12  T24T14\frac{P_2}{P_1} = \frac{r_2^2}{r_1^2} \; \frac{T_2^4}{T_1^4}

Substitute values:

P2P1=(0.8)2(0.2)2×(400800)4\frac{P_2}{P_1} = \frac{(0.8)^2}{(0.2)^2} \times \left( \frac{400}{800} \right)^4

Compute each factor separately:

(0.8)2(0.2)2=0.640.04=16\frac{(0.8)^2}{(0.2)^2} = \frac{0.64}{0.04} = 16 (400800)4=(12)4=116\left( \frac{400}{800} \right)^4 = \left( \frac{1}{2} \right)^4 = \frac{1}{16}

Multiply:

P2P1=16×116=1\frac{P_2}{P_1} = 16 \times \frac{1}{16} = 1

Therefore

P2=P1=EP_2 = P_1 = E

Hence, the energy radiated from the bigger body is EE.

Correct option: (2)

Examples

Example 1

The cooling of molten lava droplets compared to larger lava pools

Example 2

Designing incandescent lamp filaments of different diameters and temperatures

Example 3

Estimating the power output of stars with different radii and surface temperatures

Example 4

Heat loss calculations for small vs. large satellites in space

Visual Representation

References

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