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Question: One kg of a diatomic gas is at a pressure of \(8 \times {10^4}N/{m^2}\). The density of the gas is \...

One kg of a diatomic gas is at a pressure of 8×104N/m28 \times {10^4}N/{m^2}. The density of the gas is 4kg/m34kg/{m^3}. What is the energy of the gas due to its thermal motion?
(A) 3×104J3 \times {10^4}J
(B) 5×104J5 \times {10^4}J
(C) 6×104J6 \times {10^4}J
(D) 7×104J7 \times {10^4}J

Explanation

Solution

To answer this question, we have to use the formula for kinetic energy of a molecule of the gas. Then, we have to manipulate this formula in terms of the given parameters to get the final answer.

Formula used:
The formulae used to solve this question are given by
E=32kBT\Rightarrow E = \dfrac{3}{2}{k_B}T
kB=RNA\Rightarrow {k_B} = \dfrac{R}{{{N_A}}}
PV=nRT\Rightarrow PV = nRT
Here EE is the kinetic energy of a gas molecule at an absolute temperature of TT, kB{k_B} is the Boltzmann’s constant, NA{N_A} is the Avogadro’s constant,RR is the universal gas constant, nn is the number of moles.

Complete step by step solution:
We know that the kinetic energy of a molecule of gas due to its thermal motion is given by
E=32kBT\Rightarrow E = \dfrac{3}{2}{k_B}T
If the given gas has NN molecules, then the total kinetic energy of the gas is
ET=NE\Rightarrow {E_T} = NE
ET=3N2kBT\Rightarrow {E_T} = \dfrac{{3N}}{2}{k_B}T
We know that kB=RNA{k_B} = \dfrac{R}{{{N_A}}}
So that
ET=3N2RNAT\Rightarrow {E_T} = \dfrac{{3N}}{2}\dfrac{R}{{{N_A}}}T
ET=32×R×NNA×T\Rightarrow {E_T} = \dfrac{3}{2} \times R \times \dfrac{N}{{{N_A}}} \times T
As we know from the Avogadro’s law that
N=nNA\Rightarrow N = n{N_A}
Putting this in the above expression
ET=32×R×nNANA×T\Rightarrow {E_T} = \dfrac{3}{2} \times R \times \dfrac{{n{N_A}}}{{{N_A}}} \times T
ET=32nRT\Rightarrow {E_T} = \dfrac{3}{2}nRT ………………………..(i)
From the ideal gas equation, we have
PV=nRT\Rightarrow PV = nRT
So (i) becomes
ET=32PV\Rightarrow {E_T} = \dfrac{3}{2}PV ……………………….(ii)
As the density ρ=MV\rho = \dfrac{M}{V}
So V=MρV = \dfrac{M}{\rho }
Putting in (ii) we get
ET=32PMρ\Rightarrow {E_T} = \dfrac{3}{2}\dfrac{{PM}}{\rho }
Now, according to the question, we have the pressure P=8×104N/m2P = 8 \times {10^4}N/{m^2} , mass of the gas M=1kgM = 1kg and the density of the gas ρ=4kg/m3\rho = 4kg/{m^3}. Substituting these in the above expression, we get
ET=32×8×104×14\Rightarrow {E_T} = \dfrac{3}{2} \times \dfrac{{8 \times {{10}^4} \times 1}}{4}
On solving we finally get
ET=3×104J\Rightarrow {E_T} = 3 \times {10^4}J
Thus, the energy of the gas due to the thermal motion is equal to 3×104J3 \times {10^4}J.
Hence, the correct answer is option (A).

Note:
Don’t get confused by the atomicity of the gas given in the question. We have derived the final expression for the total kinetic energy of the gas starting from the very basic formula for the energy of a gas molecule, which is the same for all the gases regardless of its atomicity.