SRM NIRF Ranking 2024 - SRM Institute of Science and Technology

Heat Transfer By Radiation - Practice Questions & MCQ

Edited By admin | Updated on Sep 18, 2023 18:34 AM | #JEE Main

Quick Facts

  • 16 Questions around this concept.

Solve by difficulty

Two spheres of the same material have radii 1 m and 4 m and temperatures 4000 K and 2000 K respectively. The ratio of the energy radiated per second by the first sphere to that by the second is :

A charged particle of charge q is accelerating with acceleration a then the total radiant flux emitted by charge particle at any instant is proportional to 

Concepts Covered - 1

Radiation

Radiation - The process of the transfer of heat from one place to another place without any requirement of the medium is called radiation. It means that the radiation does not need any material medium to propagate.

Characteristics of Radiation - 

  •  The process of the transfer of heat from one place to another place without heating the medium is called radiation.
    - The wavelength of thermal radiations ranges from $7.8 \times 10^{-7} \mathrm{~m}$ to $4 \times 10^{-7} \mathrm{~m}$. The radiation heat transfer belongs to the infra-red region of the electromagnetic spectrum. That is why thermal radiations are also called infra-red radiations.
    - Every body whose temperature is above zero Kelvin emits thermal radiation. Practically it is not possible to reach 0 Kelvin in finite number of steps, so every material in this universe emit radiation.
    - The intensity of thermal radiation is inversely proportional to the square of the distance of the point of observation from the source

    $
    \left(I \propto \frac{1}{d^2}\right)
    $

    - As it is an electromagnetic wave, they follow laws of reflection, refraction, interference, diffraction, and polarisation.
    - Radiation pressure - When these thermal radiations fall on a surface then exert pressure on that surface, which is called Radiation pressure.
    - Radiation spectrum is obtained by quartz or rock salt prism because these materials do not have free electrons and interatomic vibrational frequency is greater than the radiation frequency, hence they do not absorb heat radiations.
    - Interaction of Radiation with Matter-

       When thermal radiations (Q) fall on a body, they are partly reflected, partly absorbed and partly transmitted as shown in the below figure.

           

So we can write

$
\begin{aligned}
& Q=Q_a+Q_t+Q_r \\
& \text { or } \quad \frac{Q}{Q}=\frac{Q_a}{Q}+\frac{Q_t}{Q}+\frac{Q_r}{r}
\end{aligned}
$

or $\quad 1=\mathrm{a}+\mathrm{r}+\mathrm{t}$
Where

$
\begin{aligned}
& \frac{Q_a}{Q}=a=\text { Absorptance } \\
& \frac{Q_r}{Q}=r=\text { Reflactance } \\
& \frac{Q_t}{Q}=t=\text { Transmittance }
\end{aligned}
$


So
1. If $a=t=0$ and $r=1$ then body is perfect reflector
2. If $r=t=0$ and $a=1$ then body is perfectly black body.
3. If, $a=r=0$ and $t=1$ thenbody is perfect transmitter
4. If $t=0 \Rightarrow r+a=1$ or $a=1-r$

  1. i.e. good reflectors are bad  absorbers.

  • Prevost Theory of Heat Exchange-
  1.   Every body emits heat radiations at all finite temperature (Except 0 K) as well as it absorbs radiations from the surroundings.
  2. The amount of heat emitted/absorbed depends on the nature of the body,  the temperature of the body and the cross-section of the body through which heat exchange is taking place.
  3. The exchange of energy along various bodies takes place via radiation.
  4.  How the temperature of the body will vary will depend on the temperature of the surrounding

     I. If surrounding temperature= body temperature
then $Q_{\text {emission }}=Q_{\text {absorbed }}$
i.e the body will emit and absorbed at the same rate
the temperature of the body remains constant (thermal equilibrium)
II. If surrounding temperature > body temperature
then $Q_{\text {emission }}<Q_{\text {absorbed }}$
i.e temperature of the body increases and it appears hotter.
III. If surrounding temperature < body temperature
then $Q_{\text {emission }}>Q_{\text {absorbed }}$
i.e temperature of the body decreases and consequently the body appears colder.

 

Study it with Videos

Radiation

"Stay in the loop. Receive exam news, study resources, and expert advice!"

Books

Reference Books

Radiation

Physics Part II Textbook for Class XI

Page No. : 294

Line : 9

E-books & Sample Papers

Get Answer to all your questions

Back to top