A wall has two layers A and B each made of a different material. Both layers have the same thickness, the thermal conductivity of the material of A is twice that of B. Under thermal equilibrium, the temperature difference across the wall is 36oC. The temperature difference across the layer A will be:
6oC
12oC
18oC
24oC
Water falls from a height of 500 m. What is the rise in temperature of water at the bottom if the whole energy is used up in heating water ?
0.96o C
1.02o C
1.16o C
0.25o C
An ungraduated thermometer of uniform bore is attached to a centimetre scale and is found to read 10.3 cm in melting ice, 26.8 cm in boiling water and 6.5 cm. in freezing mixture. The temperature of the freezing mixture will be :
-23.003o C
-23.03o C
-23.3o C
-23.33o C
A block of steel heated to 100oC is left in a room to cool. Which of the curves shown in the figure, represents the correct behaviour ?
A
B
C
None
A spherical black body with a radius 12 cm radiates 450 W power at 500 K. If the radius were halved and the temperature doubled, the power radiated in watt would be:
225
450
900
1800
For a gas, the difference between two principal specific heats is 4150 J kg-1 K-1 . What is the specific heat of the gas at constant volume if the ratio of specific heats is 1.4 ?
5186 J kg-1 K-1
10375 J kg-1 K-1
1060 J kg-1 K-1
8475 J kg-1 K-1
An ideal black body at room temperature is thrown into a furnace. It is observed that:
Initially, it is the darkest body and at later times the brightest.
It is the darkest body at all times.
It cannot be distinguished at all times.
Initially, it is the darkest body and at later times it cannot be distinguished.
Variation of radiant energy emitted by sun, filament of tungsten lamp and welding arc as a function of its wavelength is shown in figure. Which of the following options is the correct match ?
Sun - T3, tungsten filament - T1, welding arc - T2
Sun - T2, tungsten filament - T1, welding arc - T3
Sun - T3, tungsten filament - T2, welding arc - T1
Sun - T1, tungsten filament - T2, welding arc - T3
The earth radiates in the infra-red region of the spectrum. The spectrum is correctly given by :
Planck's law of radiation
Stefan's law of radiation
Rayleigh Jeans law
Wien's law
In determining the temperature of a distant star, one makes use of:
Kirchhoff's law
Stefan's law
Wien's displacement law
Millman's theorem