Solids
Liquids
Gases
None of these
C. Gases
Varies with temperature
Varies with the wave length of incident ray
Varies with both
Does not vary with temperature and wave length of the incident ray
Directly proportional to the surface area of the body
Directly proportional to the temperature difference on the two faces of the body
Dependent upon the material of the body
All of the above
Thermometer
Thermistor
Thermocouple
None of these
The time taken to attain the final temperature to be measured
The time taken to attain 50% of the value of initial temperature difference
The time taken to attain 63.2% of the value of initial temperature difference
Determined by the time taken to reach 100°C from 0°C
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
0.1
0.3
0.7
1.7
Q = 2πkr1 r2 (T1 - T2)/ (r2 - r1)
Q = 4πkr1 r2 (T1 - T2)/ (r2 - r1)
Q = 6πkr1 r2 (T1 - T2)/ (r2 - r1)
Q = 8πkr1 r2 (T1 - T2)/ (r2 - r1)
Higher
Lower
Same
Depends upon the shape of body
Move actually
Do not move actually
Affect the intervening medium
Does not affect the intervening medium
kcal/m²
kcal/hr °C
kcal/m² hr °C
kcal/m hr °C
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Equal to
Directly proportional to
Inversely proportional to
None of these
Conduction
Convection
Radiation
None of these
Directly proportional to thermal conductivity
Inversely proportional to density of substance
Inversely proportional to specific heat
All of the above
Fourier equation
Stefan-Boltzmann equation
Newton Reichmann equation
Joseph-Stefan equation
Glass
Water
Plastic
Air
A grey body is one which absorbs all radiations incident on it.
At thermal equilibrium, the emissivity and absorptivity are same.
The energy absorbed by a body to the total energy falling on it, is called emissivity.
A perfect body is one which is black in colour.
J/m² sec
J/m °K sec
W/m °K
Option (B) and (C) above
h = k/ ρS
h = ρS/k
h = S/ρk
h = kρ/S
More than those for liquids
Less than those for liquids
More than those for solids
Dependent on the viscosity
Shorter wavelength
Longer wavelength
Remain same at all wavelengths
Wavelength has nothing to do with it
Emissivity
Transmissivity
Reflectivity
Intensity of radiation
Universal gas constant
Kinematic viscosity
Thermal conductivity
Planck's constant
Wien's law
Planck's law
Stefan's law
Fourier's law
Stanton number
Nusselt number
Biot number
Peclet number
Grey body
Brilliant white polished body
Red hot body
Black body
Thermal conductivity to the equivalent thickness of the film of fluid
Temperature drop through the films of fluids to the thickness of film of fluids
Thickness of film of fluid to the thermal conductivity
Thickness of film of fluid to the temperature drop through the films of fluids
The total radiation from a black body per second per unit area is directly proportional to the fourth power of the absolute temperature
The wave length corresponding to the maximum energy is proportional to the absolute temperature
The ratio of the emissive power and absorptive power of all bodies is the same and is equal to the emissive power of a perfectly black body
None of the above
Electric heater
Steam condenser
Boiler
Refrigerator condenser coils
6
9
27
81