Thermal Radiation Formula in 60 Sec ⚡

 

❓ Concept Question

Why does a hot filament emit large amount of radiation, and how do we calculate the power radiated from a hot body?


🖼 Concept Image

Thermal Radiation Formula in 60 Sec ⚡


✍️ Short Concept

Any hot body continuously emits thermal radiation.

The amount of power emitted depends strongly on temperature and emissivity.


🔷 Step 1 — Blackbody Radiation Idea 💯

Every hot body emits energy in the form of radiation.

Power emitted is proportional to:

T4T^4

So,

Small temperature increase → huge increase in radiation.

This explains why filaments glow intensely.


🔷 Step 2 — Stefan–Boltzmann Law

Radiated power from a surface:

P=eσAT4P = e \sigma A T^4

Where:

e=emissivitye = \text{emissivity}
σ=5.67×108\sigma = 5.67 \times 10^{-8}
A=surface areaA = \text{surface area}
T=absolute temperature (Kelvin)T = \text{absolute temperature (Kelvin)}

🔷 Step 3 — Role of Emissivity

Emissivity measures how efficiently a surface radiates energy.

e=1e = 1

Perfect blackbody.

For real objects:

e<1e < 1

Example: bulb filament.

👉 Real materials never behave like ideal blackbodies.


🔷 Step 4 — Radiating Area of Wire

For a thin cylindrical wire:

Radiating surface area:

A=πdlA = \pi d l

Where:

d = diameter
l = length

⚠️ Ends of wire are usually ignored.

Only curved surface area contributes significantly.


🔷 Step 5 — JEE Golden Traps

❌ Temperature in Celsius

❌ Forgetting unit conversions

❌ Assuming emissivity = 1

Correct approach:

👉 Always convert temperature to Kelvin.


✅ Final Takeaway

Thermal radiation follows:

P=eσAT4\boxed{P = e \sigma A T^4}

Higher temperature → dramatically larger radiation.


⭐ Golden JEE Insight

Temperature dependence is extremely strong:

T4T^4

If temperature doubles:

Radiated power increases by 16 times.

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