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Heat Transfer — NEET Physics PYQ MCQs with Solutions

Free NEET Physics PYQ Heat Transfer MCQs with step-by-step solutions (35 questions). Part of Thermal Properties of Matter. Practise online on Prepizo — no login needed.

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Questions with solutions

Q1 — Heat Transfer · medium · numerical
A cup of coffee cools from $90^\circ$C to $80^\circ$C in $t$ minutes, when the room temperature is $20^\circ$C. The time taken by a similar cup of coffee to cool from $80^\circ$C to $60^\circ$C at a room temperature same at $20^\circ$C, is
A. $\dfrac{13}{10}t$
B. $\dfrac{13}{5}t$  ✓ Correct
C. $\dfrac{10}{13}t$
D. $\dfrac{5}{13}t$
Solution: By Newton's law of cooling, $\dfrac{\Delta T}{t}=K\left[\dfrac{T_i+T_f}{2}-T_0\right]$. First case: $\dfrac{90-80}{t}=K\left[\dfrac{90+80}{2}-20\right]\Rightarrow\dfrac{10}{t}=65K\Rightarrow K=\dfrac{2}{13t}$. Second case: $\dfrac{80-60}{t_1}=\dfrac{2}{13t}\left[\dfrac{80+60}{2}-20\right]=\dfrac{2}{13t}\times50\Rightarrow t_1=\dfrac{13}{5}t$.
Q2 — Heat Transfer · medium · theory
Three stars $A, B, C$ have surface temperatures $T_A, T_B, T_C$ respectively. Star $A$ appears bluish, star $B$ appears reddish and star $C$ yellowish. Hence
A. $T_A > T_B > T_C$
B. $T_B > T_C > T_A$
C. $T_C > T_B > T_A$
D. $T_A > T_C > T_B$  ✓ Correct
Solution: According to Wien's displacement law, $\lambda = \dfrac{b}{T}$, i.e. $\lambda \propto \dfrac{1}{T}$. We know that $\lambda_{bluish} < \lambda_{yellowish} < \lambda_{reddish}$. Hence, $T_A > T_C > T_B$.
Q3 — Heat Transfer · medium · numerical
An object kept in a large room having air temperature of $25^\circ$C takes 12 minutes to cool from $80^\circ$C to $70^\circ$C. The time taken to cool for the same object from $70^\circ$C to $60^\circ$C would be nearly
A. 10 min
B. 12 min
C. 20 min
D. 15 min  ✓ Correct
Solution: From Newton's law of cooling, $\dfrac{T_1 - T_2}{t} = \dfrac{1}{K}\left(\dfrac{T_1 + T_2}{2} - T_0\right)$ with $T_0 = 25^\circ$C. Cooling from $80^\circ$C to $70^\circ$C in 12 min: $\dfrac{80-70}{12} = \dfrac{1}{K}\left(\dfrac{80+70}{2} - 25\right) \Rightarrow \dfrac{5}{6} = \dfrac{50}{K}$ ...(i). Cooling from $70^\circ$C to $60^\circ$C: $\dfrac{70-60}{t} = \dfrac{1}{K}\left(\dfrac{70+60}{2} - 25\right) \Rightarrow \dfrac{10}{t} = \dfrac{40}{K}$ ...(ii). Dividing (i) by (ii): $\dfrac{5}{6} \times \dfrac{t}{10} = \dfrac{50}{40} \Rightarrow t = \dfrac{5}{4} \times 12 = 15$ minutes.
Q4 — Heat Transfer · medium · numerical
A deep rectangular pond of surface area $A$, containing water (density $= \rho$, specific heat capacity $= s$), is located in a region where the outside air temperature is a steady value at the $-26^\circ$C. The thickness of the frozen ice layer in this pond, at a certain instant is $x$. Taking the thermal conductivity of ice as $K$, and its specific latent heat of fusion as $L$, the rate of increase of the thickness of ice layer, at this instant would be given by
A. $26K/\rho x(L - 4s)$
B. $26K/(\rho x^2 - L)$
C. $26K/(\rho xL)$  ✓ Correct
D. $26K/\rho x(L + 4s)$
Solution: If the cross-section is not uniform or steady state is not reached, the heat conduction equation applies to a thin layer perpendicular to the heat flow. Rate of heat flow for ice growth: $\dfrac{d\theta}{dt} = \dfrac{KA(\theta_0 - \theta_1)}{x}$, where $d\theta = \rho A\,dx\,L$, $\theta_0 = 0^\circ$C and $\theta_1 = -26^\circ$C. Thus $\dfrac{\rho A\,dx\,L}{dt} = \dfrac{KA(\theta_0 - \theta_1)}{x} \Rightarrow \dfrac{dx}{dt} = \dfrac{K[0-(-26)]}{\rho xL} = \dfrac{26K}{\rho xL}$.
Q5 — Heat Transfer · medium · numerical
The power radiated by a black body is $P$ and it radiates maximum energy at wavelength $\lambda_0$. If the temperature of the black body is now changed, so that it radiates maximum energy at wavelength $\dfrac{3}{4}\lambda_0$, the power radiated by it becomes $nP$. The value of $n$ is
A. $\dfrac{256}{81}$  ✓ Correct
B. $\dfrac{4}{3}$
C. $\dfrac{3}{4}$
D. $\dfrac{81}{256}$
Solution: By Wien's law, $\lambda_{max} T = $ constant, so $\dfrac{T_1}{T_2} = \dfrac{\lambda_{max_2}}{\lambda_{max_1}}$. With $\lambda_{max_1} = \lambda_0$ and $\lambda_{max_2} = \dfrac{3}{4}\lambda_0$, $\dfrac{T_1}{T_2} = \dfrac{3}{4}$. By Stefan's law $P \propto T^4$, so $\dfrac{P_1}{P_2} = \left(\dfrac{T_1}{T_2}\right)^4 = \left(\dfrac{3}{4}\right)^4 = \dfrac{81}{256}$. With $P_1 = P$ and $P_2 = nP$: $\dfrac{P}{nP} = \dfrac{81}{256} \Rightarrow n = \dfrac{256}{81}$.
Q6 — Heat Transfer · medium · numerical
Two rods $A$ and $B$ of different materials are welded together as shown in figure. Their thermal conductivities are $K_1$ and $K_2$. The thermal conductivity of the composite rod will be
A. $\dfrac{K_1 + K_2}{2}$  ✓ Correct
B. $\dfrac{3(K_1 + K_2)}{2}$
C. $K_1 + K_2$
D. $2(K_1 + K_2)$
Solution: The rods are in parallel with equal cross-sectional areas and the same length, so the composite conductivity is $K = \dfrac{K_1 A + K_2 A}{2A} = \dfrac{K_1 + K_2}{2}$.
Q7 — Heat Transfer · medium · numerical
A spherical black body with a radius of 12 cm radiates 450 watt power at 500 K. If the radius were halved and the temperature doubled, the power radiated in watt would be
A. 225
B. 450
C. 1000
D. 1800  ✓ Correct
Solution: Radiated power of a black body, $P=\sigma A T^4$, where $A$ is the surface area and $T$ the temperature. When the radius is halved, the new area $A'=\dfrac{A}{4}$. So $P'=\sigma\left(\dfrac{A}{4}\right)(2T)^4=\dfrac{16}{4}\,\sigma A T^4=4P=4\times450=1800$ watts.
Q8 — Heat Transfer · medium · numerical
A black body is at a temperature of 5760 K. The energy of radiation emitted by the body at wavelength 250 nm is $U_1$, at wavelength 500 nm is $U_2$ and that at 1000 nm is $U_3$. Wien's constant, $b=2.88\times10^6$ nmK. Which of the following is correct?
A. $U_3=0$
B. $U_1>U_2$
C. $U_2>U_1$  ✓ Correct
D. $U_1=0$
Solution: According to Wien's law, $\lambda_m T=b$, so $\lambda_m=\dfrac{b}{T}=\dfrac{2.88\times10^6\text{ nmK}}{5760\text{ K}}=500$ nm. Since $\lambda_m=500$ nm is the wavelength corresponding to maximum energy, $U_2>U_1$.
Q9 — Heat Transfer · medium · numerical
A body cools from a temperature $3T$ to $2T$ in 10 minutes. The room temperature is $T$. Assume that Newton's law of cooling is applicable. The temperature of the body at the end of next 10 minutes will be
A. $\dfrac{7}{4}T$
B. $\dfrac{3}{2}T$  ✓ Correct
C. $\dfrac{4}{3}T$
D. $T$
Solution: By Newton's law of cooling, $\Delta T=\Delta T_0\,e^{-\lambda t}$. For the first 10 min, $3T-2T=(3T-T)e^{-\lambda\times10}$, giving $e^{-10\lambda}=\dfrac{1}{2}$. Measuring the excess temperature over the full 20 min from the start, $T'-T=(3T-T)e^{-\lambda\times20}=2T\,(e^{-10\lambda})^2=2T\left(\dfrac{1}{2}\right)^2=\dfrac{T}{2}$. Hence $T'=T+\dfrac{T}{2}=\dfrac{3T}{2}$.
Q10 — Heat Transfer · medium · numerical
The two ends of a metal rod are maintained at temperatures $100^\circ$C and $110^\circ$C. The rate of heat flow in the rod is found to be 4.0 J/s. If the ends are maintained at temperatures $200^\circ$C and $210^\circ$C, the rate of heat flow will be
A. 44.0 J/s
B. 16.8 J/s
C. 8.0 J/s
D. 4.0 J/s  ✓ Correct
Solution: Here $\Delta T_1=110-100=10^\circ$C with $\dfrac{dQ_1}{dt}=4$ J/s, and $\Delta T_2=210-200=10^\circ$C. The rate of heat flow is directly proportional to the temperature difference, which is the same ($10^\circ$C) in both cases. Hence $\dfrac{dQ_2}{dt}=4$ J/s.
Q11 — Heat Transfer · medium · numerical
Certain quantity of water cools from $70^\circ$C to $60^\circ$C in the first 5 min and to $54^\circ$C in the next 5 min. The temperature of the surroundings is
A. $45^\circ$C  ✓ Correct
B. $20^\circ$C
C. $42^\circ$C
D. $10^\circ$C
Solution: Apply Newton's law of cooling with surrounding temperature $t^\circ$C. First case: $\dfrac{70-60}{5}=K(65-t)$, where $65^\circ$C is the average of 70 and 60. Second case: $\dfrac{60-54}{5}=K(57-t)$, where $57^\circ$C is the average of 60 and 54. Dividing, $\dfrac{10}{6}=\dfrac{65-t}{57-t}$, which gives $t=45^\circ$C.
Q12 — Heat Transfer · medium · theory
A piece of iron is heated in a flame. If first becomes dull red then becomes reddish yellow and finally turns to white hot. The correct explanation for the above observation is possible by using
A. Stefan's law
B. Wien's displacement law  ✓ Correct
C. Kirchhoff's law
D. Newton's law of cooling
Solution: As the temperature rises, the wavelength of maximum emission decreases (red $\to$ yellow $\to$ white). This is explained by Wien's displacement law, $\lambda_m T=$ constant.
Q13 — Heat Transfer · medium · numerical
If the radius of a star is $R$ and it acts as a black body, what would be the temperature of the star, in which the rate of energy production is $Q$? ($\sigma$ stands for Stefan's constant.)
A. $Q/4\pi R^2\sigma$
B. $(Q/4\pi R^2\sigma)^{-1/2}$
C. $(4\pi R^2 Q/\sigma)^{1/4}$
D. $(Q/4\pi R^2\sigma)^{1/4}$  ✓ Correct
Solution: From Stefan's law, $E=\sigma T^4$. The rate of energy production $Q=E\times A=\sigma T^4\times4\pi R^2$. Hence the temperature of the star $T=\left(\dfrac{Q}{4\pi R^2\sigma}\right)^{1/4}$.
Q14 — Heat Transfer · medium · numerical
A cylindrical metallic rod in thermal contact with two reservoirs of heat at its two ends conducts an amount of heat $Q$ in time $t$. The metallic rod is melted and the material is formed into a rod of half the radius of the original rod. What is the amount of heat conducted by the new rod when placed in thermal contact with the two reservoirs in time $t$?
A. $Q/4$
B. $Q/16$  ✓ Correct
C. $2Q$
D. $Q/2$
Solution: In steady state $Q=\dfrac{KA(\theta_1-\theta_2)t}{l}$, so $\dfrac{Q}{t}\propto\dfrac{A}{l}\propto\dfrac{r^2}{l}$. On remelting into a rod of half the radius, volume is conserved: $\pi r_1^2 l_1=\pi r_2^2 l_2$ with $r_2=\dfrac{r_1}{2}$, giving $l_2=4l_1$. Then $\dfrac{Q_1}{Q_2}=\dfrac{r_1^2}{l_1}\times\dfrac{l_2}{r_2^2}=\dfrac{r_1^2}{l_1}\times\dfrac{4l_1}{(r_1/2)^2}=16$. Hence $Q_2=\dfrac{Q_1}{16}=\dfrac{Q}{16}$.
Q15 — Heat Transfer · medium · numerical
A black body at $227^\circ$C radiates heat at the rate of 7 cal cm$^{-2}$ s$^{-1}$. At a temperature of $727^\circ$C, the rate of heat radiated in the same units will be
A. 60
B. 50
C. 112  ✓ Correct
D. 80
Solution: By Stefan's law $E=\sigma T^4$. With $T_1=227+273=500$ K and $T_2=727+273=1000$ K, $\dfrac{E_1}{E_2}=\left(\dfrac{T_1}{T_2}\right)^4\Rightarrow E_2=7\left(\dfrac{273+727}{273+227}\right)^4=7\left(\dfrac{1000}{500}\right)^4=112$ cal cm$^{-2}$ s$^{-1}$.
Q16 — Heat Transfer · medium · theory
The two ends of a rod of length $L$ and a uniform cross-sectional area $A$ are kept at two temperatures $T_1$ and $T_2$ ($T_1>T_2$). The rate of heat transfer, $\dfrac{dQ}{dt}$, through the rod in a steady state is given by
A. $\dfrac{dQ}{dt}=\dfrac{KL(T_1-T_2)}{A}$
B. $\dfrac{dQ}{dt}=\dfrac{K(T_1-T_2)}{LA}$
C. $\dfrac{dQ}{dt}=KLA(T_1-T_2)$
D. $\dfrac{dQ}{dt}=\dfrac{KA(T_1-T_2)}{L}$  ✓ Correct
Solution: For a rod of length $L$ and cross-sectional area $A$ with faces maintained at temperatures $T_1$ and $T_2$, in steady state the rate of heat flow from one face to the other is $\dfrac{dQ}{dt}=\dfrac{KA(T_1-T_2)}{L}$.
Q17 — Heat Transfer · medium · numerical
A black body is at $727^\circ$C. It emits energy at a rate which is proportional to
A. $(727)^2$
B. $(1000)^4$  ✓ Correct
C. $(1000)^2$
D. $(727)^4$
Solution: By Stefan's law, $E\propto T^4$ (or $E=\sigma T^4$). Converting to kelvin, $T=727+273=1000$ K, so $E\propto(727+273)^4=(1000)^4$.
Q18 — Heat Transfer · medium · numerical
Assuming the sun to have a spherical outer surface of radius $r$, radiating like a black body at temperature $t^\circ$C, the power received by a unit surface, (normal to the incident rays) at a distance $R$ from the centre of the sun is (where $\sigma$ is the Stefan's constant)
A. $\dfrac{4\pi r^2 t^4}{R^2}$
B. $\dfrac{r^2\sigma(t+273)^4}{4\pi R^2}$
C. $\dfrac{16\pi^2 r^2\sigma t^4}{R^2}$
D. $\dfrac{r^2\sigma(t+273)^4}{R^2}$  ✓ Correct
Solution: By Stefan's law, the power radiated at the sun's surface is $P=\sigma\times4\pi r^2 T^4$ (with $e=1$ for a black body). The intensity received at a distance $R\gg r_0$ is $I=\dfrac{P}{4\pi R^2}=\dfrac{\sigma\times4\pi r^2 T^4}{4\pi R^2}=\dfrac{\sigma r^2 T^4}{R^2}=\dfrac{r^2\sigma(t+273)^4}{R^2}$.
Q19 — Heat Transfer · medium · numerical
A black body at $1227^\circ$C emits radiations with maximum intensity at a wavelength of 5000 Å. If the temperature of the body is increased by $1000^\circ$C, the maximum intensity will be observed at
A. 4000 Å
B. 5000 Å
C. 6000 Å
D. 3000 Å  ✓ Correct
Solution: By Wien's law $\lambda_m T=$ constant, so $\dfrac{\lambda_m'}{\lambda_m}=\dfrac{T}{T'}$. Here $T=1227+273=1500$ K and $T'=1227+1000+273=2500$ K. Hence $\lambda_m'=\dfrac{1500}{2500}\times5000=3000$ Å.
Q20 — Heat Transfer · medium · numerical
Which of the following circular rods, (given radius $r$ and length $l$) each made of the same material and whose ends are maintained at the same temperature will conduct most heat?
A. $r=2r_0$; $l=2l_0$
B. $r=2r_0$; $l=l_0$  ✓ Correct
C. $r=r_0$; $l=l_0$
D. $r=r_0$; $l=2l_0$
Solution: By conduction, $H=\dfrac{\Delta Q}{\Delta t}=KA\dfrac{(T_1-T_2)}{l}$, so $H\propto\dfrac{r^2}{l}$. (a) $\dfrac{(2r_0)^2}{2l_0}=\dfrac{2r_0^2}{l_0}$; (b) $\dfrac{(2r_0)^2}{l_0}=\dfrac{4r_0^2}{l_0}$; (c) $\dfrac{r_0^2}{l_0}$; (d) $\dfrac{r_0^2}{2l_0}$. Case (b) is the largest, so it conducts the most heat.
Q21 — Heat Transfer · medium · theory
If $\lambda_m$ denotes the wavelength at which the radiative emission from a black body at a temperature $T$ K is maximum, then
A. $\lambda_m\propto T^4$
B. $\lambda_m$ is independent of $T$
C. $\lambda_m\propto T$
D. $\lambda_m\propto T^{-1}$  ✓ Correct
Solution: By Wien's displacement law, the wavelength of maximum emission of black body radiation is inversely proportional to the absolute temperature: $\lambda_m T=\text{constant}$, so $\lambda_m=\dfrac{\text{constant}}{T}$, i.e. $\lambda_m\propto\dfrac{1}{T}=T^{-1}$.
Q22 — Heat Transfer · medium · theory
We consider the radiation emitted by the human body. Which of the following statements is true?
A. The radiation is emitted during the summers and absorbed during the winters
B. The radiation emitted lies in the ultraviolet region and hence is not visible
C. The radiation emitted is in the infrared region  ✓ Correct
D. The radiation is emitted only during the day
Solution: The heat radiation emitted by the human body is infrared radiation, with wavelength of the order of $7.9\times10^{-7}$ m to $10^{-3}$ m, which lies in the infrared region.
Q23 — Heat Transfer · medium · numerical
Consider a compound slab consisting of two different materials having equal thicknesses and thermal conductivities $K$ and $2K$, respectively. The equivalent thermal conductivity of the slab is
A. $3K$
B. $\dfrac{4}{3}K$  ✓ Correct
C. $\dfrac{2}{3}K$
D. $\sqrt{2}\,K$
Solution: For two slabs of equal thickness in series, the equivalent conductivity is $K'=\dfrac{2K_1K_2}{K_1+K_2}$. With $K_1=K$ and $K_2=2K$, $K'=\dfrac{2K\times2K}{K+2K}=\dfrac{4}{3}K$.
Q24 — Heat Transfer · medium · numerical
For a black body at temperature $727^\circ$C, its radiating power is 60 W and temperature of surrounding is $227^\circ$C. If the temperature of the black body is changed to $1227^\circ$C, then its radiating power will be
A. 120 W
B. 240 W
C. 304 W
D. 320 W  ✓ Correct
Solution: By Stefan-Boltzmann's law including surroundings, $P=\sigma(T^4-T_0^4)$, so $\dfrac{P_2}{P_1}=\dfrac{T_2^4-T_0^4}{T_1^4-T_0^4}$. Here $T_1=1000$ K, $T_0=500$ K, $T_2=1500$ K and $P_1=60$ W. Thus $P_2=\dfrac{(1500)^4-(500)^4}{(1000)^4-(500)^4}\times60=\dfrac{3^4-1}{2^4-1}\times60=\dfrac{80}{15}\times60=320$ W.
Q25 — Heat Transfer · medium · numerical
Consider two rods of same length and different specific heats $(s_1, s_2)$, thermal conductivities $(K_1, K_2)$ and areas of cross-section $(A_1, A_2)$ and both having temperatures $(T_1, T_2)$ at their ends. If their rate of loss of heat due to conduction are equal, then
A. $K_1A_1=K_2A_2$  ✓ Correct
B. $\dfrac{K_1A_1}{s_1}=\dfrac{K_2A_2}{s_2}$
C. $K_2A_1=K_1A_2$
D. $\dfrac{K_2A_1}{s_2}=\dfrac{K_1A_2}{s_1}$
Solution: Rate of loss of heat by conduction is $H=\dfrac{\Delta Q}{\Delta t}=KA\dfrac{(T_1-T_2)}{l}$. For the two rods $H_1=K_1A_1\dfrac{(T_1-T_2)}{l_1}$ and $H_2=K_2A_2\dfrac{(T_1-T_2)}{l_2}$. Since $l_1=l_2$ (same length) and $H_1=H_2$, we get $K_1A_1=K_2A_2$.
Q26 — Heat Transfer · medium · theory
Wien's displacement law expresses relation between
A. wavelength corresponding to maximum energy and absolute temperature  ✓ Correct
B. radiated energy and wavelength
C. emissive power and temperature
D. colour of light and temperature
Solution: According to Wien's displacement law, the wavelength corresponding to maximum energy is inversely proportional to the absolute temperature of the body, i.e. $\lambda_m\propto\dfrac{1}{T}$ or $\lambda_m T=$ constant. As temperature increases, the wavelength carrying maximum energy decreases.
Q27 — Heat Transfer · medium · theory
Which of the following is close to an ideal black body?
A. Black lamp
B. Cavity maintained at constant temperature  ✓ Correct
C. Platinum black
D. A lamp of charcoal heated to high temperature
Solution: Materials like black velvet or lamp black come close to ideal black bodies, but the best practical realization of an ideal black body is a small hole leading into a cavity maintained at constant temperature, as this absorbs about $98\%$ of the radiation incident on it. Radiation entering the cavity has little chance of leaving before it is completely absorbed.
Q28 — Heat Transfer · medium · numerical
Rate of heat flow through a cylindrical rod is $H_1$. Temperatures of ends of rod are $T_1$ and $T_2$. If all the dimensions of rod become double and temperature difference remains same and rate of heat flow becomes $H_2$. Then,
A. $H_2=2H_1$  ✓ Correct
B. $H_2=\dfrac{H_1}{2}$
C. $H_2=\dfrac{H_1}{4}$
D. $H_2=4H_1$
Solution: Rate of heat flow $H\propto\dfrac{A}{l}$, where $A$ is area of cross-section and $l$ is length. Since $A=[L^2]$ and $l=[L]$, $H\propto l$. When all dimensions become double, $l_2=2l_1$, hence $H_2=2H_1$.
Q29 — Heat Transfer · medium · numerical
The wavelength corresponding to maximum intensity of radiation emitted by a source at temperature 2000 K is $\lambda$, then what is the wavelength corresponding to maximum intensity of radiation at temperature 3000 K?
A. $\dfrac{2}{3}\lambda$  ✓ Correct
B. $\dfrac{16}{81}\lambda$
C. $\dfrac{81}{16}\lambda$
D. $\dfrac{4}{3}\lambda$
Solution: By Wien's displacement law $\lambda_m T=$ constant, so $\lambda_1 T_1=\lambda_2 T_2$. Thus $\lambda_2=\lambda_1\left(\dfrac{T_1}{T_2}\right)=\lambda\times\dfrac{2000}{3000}=\dfrac{2}{3}\lambda$.
Q30 — Heat Transfer · medium · theory
Which one of the following processes depends on gravity?
A. Conduction
B. Convection  ✓ Correct
C. Radiation
D. None of these
Solution: In convection, the heated lighter particles move upward and colder heavier particles move downward to take their place. This depends on weight, and hence on gravity. Conduction transmits heat without bodily movement of particles, and radiation travels as electromagnetic waves even through vacuum, so neither depends on gravity.