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CSIR-NET 2014 (119)

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CSIR-NET 2014

119. If both the Sun-Earth distance and the temperature of the Sun's photo sphere decrease by 50% then the Solar constant.

A) decreases to 25% of its original value 
B) increases to 400% of its original value
C) decrease to 50% of its original value
D) remains unchanged


Solution:

The energy falling per unit area = (E*R2)/r2

  --------------------(1)


R- Radius of the Sun


r- Radius of Earth’s orbit around the Sun ( Sun -Earth distance)


S= (E*R2)/r2


but E = σ * T4 --------------------(2)    (According to Stefan’s law)


S= (σ * T4*R2) / r2 -----------------------(3)


T- temperature of the Sun


The relation between the temperature of the Sun (T) 

and the Sun-Earth distance (r)


Solar constant (S) = T4 / r2 -----------------(4)


From above problem, Sun-Earth distance and 

temperature of the Sun decreases to 50%


So, S1 = (T/2)4 / (r/2)
 


S1 = (T4/16) / (r2/4) 
 


S1 = T4 / 4*r2


S1 = 1/4 *(T4/r2) ---------------(5)


Substituent eq (4) in eq (5)


Then, S1 = 1/4 *(S) 
 


Therefore Solar constant decreases 25% of its original value












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