Electric heater
Steam condenser
Boiler
Refrigerator condenser coils
C. Boiler
0.1
0.23
0.42
0.51
Zeroth law of thermodynamics
First law of thermodynamics
Second law of thermodynamics
Kirchhoff's law
Grey body
Brilliant white polished body
Red hot body
Black body
Wien's law
Planck's law
Stefan's law
Fourier's law
Density
Coefficient of viscosity
Gravitational force
All of these
High thickness of insulation
High vapour pressure
Less thermal conductivity insulator
A vapour seal
Minimum energy
Maximum energy
Both (A) and (B)
None of these
P = 0, x = 0 and a = 1
P=1, x = 0, and a = 0
P = 0, T= 1, and a = 0
X = 0, a + p = 1
From one particle of the body to another without the actual motion of the particles
From one particle of the body to another by the actual motion of the heated particles
From a hot body to a cold body, in a straight line, without affecting the intervening medium
None of the above
Thermal resistance
Thermal coefficient
Temperature gradient
Thermal conductivity
Added insulation will increase heat loss
Added insulation will decrease heat loss
Convective heat loss will be less than conductive heat loss
Heat flux will decrease
It is impossible to transfer heat from low temperature source to t high temperature source
Heat transfer by radiation requires no medium
All bodies above absolute zero emit radiation
Heat transfer in most of the cases takes place by combination of conduction, convection and radiation
Conduction
Convection
Radiation
Conduction and radiation combined
k. A. (dT/dx)
k. A. (dx/dT)
k. (dT/dx)
k. (dx/dT)
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Black bodies
Polished bodies
All coloured bodies
All of the above
Same
More
Less
Depends on other factors
1 : 1
2 : 1
1 : 2
4 : 1
Conduction
Convection
Radiation
Scattering
Increases
Decreases
Remain constant
May increase or decrease depending on temperature
Absolute temperature (T)
I²
F
T
Grashoff number
Biot number
Stanton number
Prandtl number
Pb = pa - pv
Pb = pa + pv
Pb = pa × pv
Pb = pa/pv
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
Steam
Solid ice
Melting ice
Water
Conduction
Convection
Radiation
None of these
Liquids
Energy
Temperature
Entropy
Directly proportional to the surface area
Directly proportional to the difference of temperatures between the two bodies
Either (A) or (B)
Both (A) and (B)
Higher
Lower
Same
Depends upon the shape of body
Irregular surfaces
Nonuniform temperature surfaces
One dimensional cases only
Two dimensional cases only