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)
--------------------(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)
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%
temperature of the Sun decreases to 50%
So,
S1
= (T/2)4 /
(r/2)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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