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Question: If the temperature of the hot body is raised by \[5\% \] the rate of heat radiated would be increase...

If the temperature of the hot body is raised by 5%5\% the rate of heat radiated would be increased by how much percentage?
(A) 12%12\%
(B) 22%22\%
(C) 32%32\%
(D) 42%42\%

Explanation

Solution

The heat energy radiated is directly proportional to the fourth power of the temperature of the black body. The percentage increase is the difference between the new value and the old value divided by the new value.
Formula used: In this solution we will be using the following formulae;
H=σAT4H = \sigma A{T^4} where HH is the heat energy radiated, σ\sigma is the Stefan Boltzmann constant, AA is area of the surface of the blackbody, and TT is the absolute temperature of the black body.
PI=NVOVOVPI = \dfrac{{NV - OV}}{{OV}} where PIPI is the percentage increase of a particular value, NVNV is the new value, and OVOV is the old value.

Complete Step-by-Step solution:
Generally, the heat energy radiated by a black body is directly related to the fourth power of the temperature of that black body as given by the Stefan’s law as
H=σAT4H = \sigma A{T^4} where σ\sigma is the Stefan Boltzmann constant, AA is area of the surface of the blackbody, and TT is the absolute temperature of the black body
Temperature increasing by 5 percent signifies the final temperature to be
T=T+5100TT' = T + \dfrac{5}{{100}}T which by adding and simplifying gives,
T=2120TT' = \dfrac{{21}}{{20}}T
TT=2120\Rightarrow \dfrac{{T'}}{T} = \dfrac{{21}}{{20}}
Percentage error can be defined as
PI=NVOVOVPI = \dfrac{{NV - OV}}{{OV}} where PIPI is the percentage increase of a particular value, NVNV is the new value, and OVOV is the old value.
Hence, percentage increase in the heat energy radiated would be defined as
PI=HHH×100%PI = \dfrac{{H' - H}}{H} \times 100\%
Where
H=σAT4H' = \sigma AT{'^4}
Hence,
HH=σAT4σAT4=T4T4=(TT)4\dfrac{{H'}}{H} = \dfrac{{\sigma AT{'^4}}}{{\sigma A{T^4}}} = \dfrac{{T{'^4}}}{{{T^4}}} = {\left( {\dfrac{{T'}}{T}} \right)^4}
By inserting known values, we have
HH=(2120)4\dfrac{{H'}}{H} = {\left( {\dfrac{{21}}{{20}}} \right)^4}
Hence, by multiplying both sides by HH, we get
H=(2120)4HH' = {\left( {\dfrac{{21}}{{20}}} \right)^4}H
Going back to the definition, and inserting the value above into it we have
PI=(2120)4HHH×100%PI = \dfrac{{{{\left( {\dfrac{{21}}{{20}}} \right)}^4}H - H}}{H} \times 100\%
Dividing numerator and denominator by HH, we get
PI=[(2120)41]×100%PI = \left[ {{{\left( {\dfrac{{21}}{{20}}} \right)}^4} - 1} \right] \times 100\%
PI=[(1.05)41]×100%PI = \left[ {{{\left( {1.05} \right)}^4} - 1} \right] \times 100\%
Hence, finding the fourth power, we get
PI=[1.221]×100%PI = \left[ {1.22 - 1} \right] \times 100\%
Computing the above relation, we get
PI=22%PI = 22\%

Hence, the correct option is B.

Note: For clarity; you might have seen a text where heat radiated from a blackbody is written as
H=εσAT4H = \varepsilon \sigma A{T^4} where ε\varepsilon is the emissivity of the body. This equation and the one above are identical, this is because for a black body, the emissivity is equal to 1, and hence can drop out of the equation. This equation is more generally used for heat radiated by any type of body.