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Thermal Properties of Matter

Previous year questions with solutions · 2000 – 2026

48Questions
30Papers covered
1.11% ↓50%Weightage in 2026
’00
’01
’02
’03
’04
’05
’06
’07
’08
’09
’10
’12
’13
’14
’15
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’21
’22
’24
’25
’26
Year-wise statistics questions · papers · average per paper · weightage
YearQuestionsPapersAvg / paperWeightage
2026120.51.11% ↓50%
20251112.22% ↑11.1%
20242212.00% ↑100%
2022120.51.00% ↓50%
20211112.00% ↓10%
20201112.22% ↓50%
20192124.44% ↑100%
20181112.22% ↓50%
20172124.44% ↓20%
2016522.55.56% ↑66.7%
2015321.53.33% ↓25%
20142124.44% ↑33.3%
2013321.53.33% ↓11.1%
2012321.53.75% ↑1.2%
2010321.53.70% ↓9.3%
20092124.08% ↑91.8%
20081112.13% ↓50%
20072124.26% ↑112.8%
20061112.00% ↓6%
20051112.13% ↓2.1%
20041112.17% ↑13%
20031111.92% ↓81.9%
200251510.64% ↑421.3%
20011112.04% ↓54.1%
20002124.44%

48 questions · newest paper first · page 2 of 2

31

Assuming the sun to have a spherical outer surface of radius r, radiating like a black body at temperature t 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 is the Stefan's constant.

  1. r2 (t + 273)44 2
  2. 16 2r2 4R2
  3. r2 (t + 273)4R2
  4. 4 2 4R2
AIPMT 2010 (Prelims)
32

A black body at 227 C radiates heat at the rate of 7 cal/cm2 s. At a temperature of 727 C, the rate of heat radiated in the same units will be

  1. 50
  2. 112
  3. 80
  4. 60
AIPMT 2009
33

The two ends of a rod of length L and a uniform cross-sectional area A are kept at two temperatures T1 and T2 (T1 > T2). The rate of heat transfer, dQdt through the rod in a steady state is given by :

  1. dQdt = k(T1 - T2)LA
  2. dQdt = kLA(T1 - T2)
  3. dQdt = kA(T1 - T2)L
  4. dQdt = kL(T1 - T2)A
AIPMT 2009
34

On a new scale of temperature (which is linear) and called the W scale, the freezing and boiling points of water are 39 and 239 respectively. What will be the temperature on the new scale, corresponding to a temperature of 39 on the Celsius scale ?

  1. 200
  2. 139
  3. 78
  4. 117
AIPMT 2008
35

Assuming the sun to have a spherical outer surface of radius r, radiating like a black body at temperature t 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 is the Stefan's constant.

  1. r2 (t+273)44 2
  2. 16 2r2 4R2
  3. r2 (t+273)4R2
  4. 4 2 4R2
AIPMT 2007
36

A black body is at 727 . It emits energy at a rate which is proportional to

  1. (1000)4
  2. (1000)2
  3. (727)4
  4. (727)2
AIPMT 2007
37

A black body at 1227 emits radiations with maximum intensity at a wavelength of 5000 A. If the temperature of the body is increased by 1000 , the maximum intensity will be observed at

  1. 3000 A
  2. 4000 A
  3. 5000 A
  4. 6000 A
AIPMT 2006
38

Which of the following 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?

  1. r = r0, l = l0
  2. r = 2r0, l = l0
  3. r = r0, l = 2l0
  4. r = 2r0, l = 2l0
AIPMT 2005
39

If m denotes the wavelength at which the radiative emission from a black body at a temperature T K is maximum, then

  1. m T4
  2. m is independent of T
  3. m T
  4. m T-1
AIPMT 2004
40

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

  1. 23K
  2. 2K
  3. 3K
  4. 43K
AIPMT 2003
41

Unit of Stefan's constant is

  1. watt m2 K4
  2. watt m2/K4
  3. watt/m2 K
  4. watt/m2K4
AIPMT 2002
42

Consider two rods of same length and different specific heats (S1, S2), conductivities (K1, K2) and area of cross-sections (A1, A2) and both having temperatures T1 and T2 at their ends. If rate of loss of heat due to conduction is equal, then

  1. K1A1 = K2A2
  2. K1A1S1 = K2A2S2
  3. K2A1 = K1A2
  4. K2A1S2 = K1A2S1
AIPMT 2002
43

For a black body at temperature 727 , its radiating power is 60 watt and temperature of surrounding is 227 . If temperature of black body is changed to 1227 then its radiating power will be

  1. 304 W
  2. 320 W
  3. 240 W
  4. 120 W
AIPMT 2002
44

Which of the following is closest to an ideal black body?

  1. lamp black
  2. cavity maintained at constant temperature
  3. platinum black
  4. a lump of charcoal heated to high temperature.
AIPMT 2002
45

The Wien's displacement law expresses relation between

  1. wavelength corresponding to maximum energy and temperature
  2. radiation energy and wavelength
  3. temperature and wavelength
  4. colour of light and temperature.
AIPMT 2002
46

A cylindrical rod has temperatures T1 and T2 at its ends. The rate of flow of heat is Q1 cal/s. If all the linear dimensions are doubled keeping the temperatures constant, then the rate of flow of heat Q2 will be

  1. 4Q1
  2. 2Q1
  3. Q14
  4. Q12
AIPMT 2001
47

Gravitational force is required for

  1. stirring of liquid
  2. convection
  3. conduction
  4. radiation
AIPMT 2000
48

A black body emits maximum energy at wavelength m at 2000 K. Its corresponding wavelength at 3000 K will be

  1. 32 m
  2. 23 m
  3. 1681 m
  4. 8116 m
AIPMT 2000