If the temperature of the sun becomes twice its present temperature, then:

1. Radiated energy would be predominantly in the infrared range.
2. Radiated energy would be primarily in the ultraviolet range.
3. Radiated energy would be predominantly in the X-ray region
4. Radiated energy would become twice as strong as it is now.


 

Subtopic:  Wien's Displacement Law |
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The maximum energy in the thermal radiation from a hot source occurs at a wavelength of 11×10-5 cm. According to Wein's law, the temperature of the source (on Kelvin scale) will be n times the temperature of another source (on Kelvin scale) for which the wavelength at maximum energy is 5.5×10-5 cm. The value n is 
(a) 2                     (b) 4
(c) 12                    (d) 1

Subtopic:  Wien's Displacement Law |
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How is the temperature of stars determined by ?

(1) Stefan’s law                       

(2) Wein’s displacement law

(3) Kirchhoff’s law                   

(4) Ohm’s law

Subtopic:  Wien's Displacement Law |
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On increasing the temperature of a substance gradually, which of the following colours will be noticed by you ?

(1) White                     

(2) Yellow

(3) Green                     

(4) Red

Subtopic:  Wien's Displacement Law |
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A black body has a maximum wavelength at a temperature of 2000 K. Its corresponding wavelength at temperatures of 3000 K will be: 

1. \({3 \over 2} \lambda_m\) 2. \({2 \over 3} \lambda_m\)
3. \({4 \over 9} \lambda_m\) 4. \({9 \over 4} \lambda_m\)
Subtopic:  Wien's Displacement Law |
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A black body at a temperature of 1640 K has the wavelength corresponding to maximum emission equal to 1.75 μm. Assuming the moon to be a perfectly black body, the temperature of the moon, if the wavelength corresponding to maximum emission is 14.35 μm is

(1) 100 K                 

(2) 150 K

(3) 200 K                 

(4) 250 K

Subtopic:  Wien's Displacement Law |
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A particular star (assuming it as a black body) has a surface temperature of about 5×104 K. The wavelength in nanometers at which its radiation becomes maximum is -
(b = 0.0029 mK) 
(1) 48               

(2) 58

(3) 60                 

(4) 70

Subtopic:  Wien's Displacement Law |
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The intensity of radiation emitted by the sun has its maximum value at a wavelength of 510 nm and that emitted by the north star has the maximum value at 350 nm. If these stars behave like black bodies, then the ratio of the surface temperature of the sun and north star is

(1) 1.46                 

(2) 0.69

(3) 1.21                 

(4) 0.83

Subtopic:  Wien's Displacement Law |
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The amount of radiation emitted by a perfectly black body is proportional to 

(1) Temperature on ideal gas scale

(2) Fourth root of temperature on ideal gas scale

(3) Fourth power of temperature on ideal gas scale

(4) Source of temperature on ideal gas scale

Subtopic:  Stefan-Boltzmann Law |
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The temperature of an object is \(400^{\circ}\mathrm{C}\). The temperature of the surroundings may be assumed to be negligible. What temperature would cause the energy to radiate twice as quickly? (Given, \(2^{\frac{1}{4}} \approx 1.18\))
1. \(200^{\circ}\mathrm{C}\)
2. 200 K
3. \(800^{\circ}\mathrm{C}\)         
4. 800 K

Subtopic:  Stefan-Boltzmann Law |
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