According to Wein's law:
1. λmT= constant                 

2. λmT= constant

3. Tλm= constant                 

4. T+λm= constant

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

1. \(\dfrac{3}{2} \lambda_m\) 2. \(\dfrac{2}{3} \lambda_m\)
3. \(\dfrac{4}{9} \lambda_m\) 4. \(\dfrac{9}{4} \lambda_m\)
Subtopic:  Wien's Displacement Law |
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A black body maintained at \(200~\text{K}\) emits maximum radiation at a wavelength of \(14~\mu \text{m}.\) If its temperature is increased to \(1000~\text{K},\) at what wavelength will the maximum radiation now be emitted?
1. \(14~\mu\text{m}\)
2. \(70~\mu\text{m}\)
3. \(2.8~\mu\text{m}\)
4. \(2.8~\text{nm}\)

Subtopic:  Wien's Displacement Law |
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A piece of iron is heated in a flame. If it becomes dull red first, then becomes reddish yellow, and finally turns to white hot, the correct explanation for the above observation is possible by using:

1. Stefan's law 2. Wien's displacement law
3. Kirchhoff's law 4. Newton's law of cooling
Subtopic:  Wien's Displacement Law |
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If \(\lambda_m\) is the wavelength, corresponding to which the radiant intensity of a block is at its maximum and its absolute temperature is \(T,\) then which of the following graphs correctly represents the variation of \(T?\)

1. 2.
3. 4.
Subtopic:  Wien's Displacement Law |
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Three stars \(A,\) \(B,\) and \(C\) have surface temperatures \(T_A,~T_B\) and \(T_C\) respectively. Star \(A\) appears bluish, star \(B\) appears reddish and star \(C\) yellowish. Hence:
1. \(T_A>T_B>T_C\)
2. \(T_B>T_C>T_A\)
3. \(T_C>T_B>T_A\)
4. \(T_A>T_C>T_B\)
Subtopic:  Wien's Displacement Law |
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NEET - 2020
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The plots of intensity versus wavelength for three black bodies at temperatures \(T_1,T_2\) and \(T_3\) respectively are as shown. Their temperatures are such that:
           

1. \({T}_1>{T}_2>{T}_3 \) 2. \({T}_1>{T}_3>{T}_2 \)
3. \({T}_2>{T}_3>{T}_1 \) 4. \({T}_3>{T}_2>{T}_1\)
Subtopic:  Wien's Displacement Law |
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The energy distribution E with the wavelength λ for the black body radiation at temperature T Kelvin is shown in the figure. As the temperature is increased the maxima will:
     

1. Shift towards left and become higher
2. Rise high but will not shift
3. Shift towards right and become higher
4. Shift towards left and the curve will become broader

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A black body is at a temperature of 5760 K. The energy of radiation emitted by the body at a wavelength of 250 nm is U1, at a wavelength of 500 nm is U2 and that at 1000 nm is U3. Given Wien's constant b=2.88×106 nm-K, whichof the following is correct?
1. U3=0       
2. U1>U2
3. U2>U1     
4. U1=0

Subtopic:  Wien's Displacement Law |
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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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