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Thermal Properties of Matter

Previous year questions with solutions · 2000 – 2026

48Questions
30Papers covered
1.11%Weightage 2026▼ 50% vs last year
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’01
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’06
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’26
Year-wise statistics questions · papers · average per paper · weightage
YearQuestionsPapersAvg / paperWeightage
2026120.51.11% ▼ 50% vs last year
20251112.22% ▲ 11.1% vs last year
20242212.00% ▲ 100% vs last year
2022120.51.00% ▼ 50% vs last year
20211112.00% ▼ 10% vs last year
20201112.22% ▼ 50% vs last year
20192124.44% ▲ 100% vs last year
20181112.22% ▼ 50% vs last year
20172124.44% ▼ 20% vs last year
2016522.55.56% ▲ 66.7% vs last year
2015321.53.33% ▼ 25% vs last year
20142124.44% ▲ 33.3% vs last year
2013321.53.33% ▼ 11.1% vs last year
2012321.53.75% ▲ 1.2% vs last year
2010321.53.70% ▼ 9.3% vs last year
20092124.08% ▲ 91.8% vs last year
20081112.13% ▼ 50% vs last year
20072124.26% ▲ 112.8% vs last year
20061112.00% ▼ 6% vs last year
20051112.13% ▼ 2.1% vs last year
20041112.17% ▲ 13% vs last year
20031111.92% ▼ 81.9% vs last year
200251510.64% ▲ 421.3% vs last year
20011112.04% ▼ 54.1% vs last year
20002124.44%

48 questions · newest paper first · page 2 of 2

Ques. 31AIPMT 2010 (Prelims)

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
Ques. 32AIPMT 2009

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
Ques. 33AIPMT 2009

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
Ques. 34AIPMT 2008

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
Ques. 35AIPMT 2007

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
Ques. 36AIPMT 2007

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
Ques. 37AIPMT 2006

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
Ques. 38AIPMT 2005

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
Ques. 39AIPMT 2004

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
Ques. 40AIPMT 2003

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
Ques. 41AIPMT 2002

Unit of Stefan's constant is

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

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
Ques. 43AIPMT 2002

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
Ques. 44AIPMT 2002

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.
Ques. 45AIPMT 2002

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.
Ques. 46AIPMT 2001

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
Ques. 47AIPMT 2000

Gravitational force is required for

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

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