Ideal gas kinetic energy is a crucial concept in physics that accounts for the movement and interaction of gas molecules. In the case of an ideal gas, kinetic energy is directly proportional to the gas temperature. A proportion of this kind helps comprehend such essential matters as pressure or temperature. Should we investigate about ideal gas kinetic energy, it is possible to infer about minute actions triggering large-scale events; hence making it among the most significant.
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In this article, we will cover the concept of the 'Kinetic Energy of Ideal Gas’. This concept is the part of chapter kinetic theory of gases, which is a important chapter in Class 11 physics. It is not only essential for board exams but also for competitive exams like the Joint Entrance Examination (JEE Main), National Eligibility Entrance Test (NEET), and other entrance exams such as SRMJEE, BITSAT, WBJEE, VITEEE and more. Over the last ten years of the JEE Main exam (from 2013 to 2023), twenty-one questions have been asked on this concept. And for NEET two questions were asked from this concept.
Let's read this entire article to gain an in-depth understanding of the Kinetic Energy of Ideal Gas.
In ideal gases, the molecules are considered point particles. The point particles can have only translational motion and thus only translational energy. So for an ideal gas, the internal energy can only be translational kinetic energy.
Hence kinetic energy (or internal energy) of n mole ideal gas
$E=\frac{1}{2} n M v_{m s}^2=\frac{1}{2} n M \times \frac{3 R T}{M}=\frac{3}{2} n R T$
1. kinetic energy of 1 molecule
$E=\frac{3}{2} k T$
$ \text { where } \mathrm{k}=\text { Boltzmann's constant and } k=1.38 \times 10^{-23} \mathrm{~J} / \mathrm{K}$
I.e. Kinetic energy per molecule of gas does not depend upon the mass of the molecule but only depends upon the temperature of the gas.
2. kinetic energy of 1-mole ideal gas
$E=\frac{3}{2} R T$
i.e. Kinetic energy per mole of gas depends only upon the temperature of the gas.
3. At T = 0, E = 0 i.e. at absolute zero the molecular motion stops.
As we know
P=\frac{1}{3} \frac{m N}{V} v_{m s}^2=\frac{1}{3} \frac{M}{V} v_{m s}^2 \Rightarrow P=\frac{1}{3} \rho v_{m s}^2......(1)
And K.E. per unit volume=
$
E=\frac{1}{2}\left(\frac{M}{V}\right) v_{m s}^2=\frac{1}{2} \rho v_{m s}^2
$... (2)
So from equation (1) and (2), we can say that $P=\frac{2}{3} E$
i.e. the pressure exerted by an ideal gas is numerically equal to two-thirds of the mean kinetic energy of translation per unit volume of the gas.
According to this law, for any system in thermal equilibrium, the total energy is equally distributed among its various degrees of freedom.
I.e Each degree of freedom is associated with energy $E=\frac{1}{2} k T$
1. At a given temperature T, all ideal gas molecules will have the same average translational kinetic energy as $\frac{3}{2} k T$
2. Different energies of a system of the degree of freedom f are as follows
(i) Total energy associated with each molecule $=\frac{f}{2} k T$
(ii) Total energy associated with $N$ molecules $=\frac{1}{2} N k T$
(iii) Total energy associated with 1 mole $=\frac{1}{2} R T$
(iv) Total energy associated with $n$ mole $=\frac{n f}{2} R T$
We can understand better through video.
Q 1. A gas molecule of mass M at the surface of the Earth has kinetic energy equivalent to 00C. If it were to go up straight without colliding with any other molecules, how high it would rise ? Assume that the height attained is much less than the radius of the earth. (kB is Boltzmann constant)
1) 0
2) $\frac{273 k_B}{2 M g}$
3) $\frac{546 k_B}{3 M g}$
4) $\frac{819 k_B}{2 M g}$
Solution:
The kinetic energy of gas due to translation per mole
$\begin{aligned}
& E=\frac{3}{2} P V \\
& =\frac{3}{2} R T
\end{aligned}$
wherein
R = Universal gas constant
T = temperature of gas
K.E at temperature $T=3 / 2 K_b T$
$\mathrm{T}$ is in Kelvin
$
\begin{aligned}
& \mathrm{T}=273 \mathrm{~K} \\
& \text { Kinetic energy }=T=3 / 2 K_b(273) \\
& =819 K_b / 2 \\
& h=819 K_B / 2 \mathrm{mg}
\end{aligned}
$
Hence, the answer is option (4).
Q 2. An ideal gas occupies a volume of 2m3 at a pressure of 3 x 106 Pa. The energy (in Joule) of the gas is
1) 9000000
2) 60000
3) 300
4) 100000000
Solution:
The kinetic energy of gas due to translation per mole
$E=\frac{3}{2} P V=\frac{3}{2} R T$
wherein
R = Universal gas constant
T = temperature of gas
$
\begin{aligned}
& p=3 \times 10^6 p_a \\
& v=2 m^3 \\
& E=\frac{f}{2} n R T=\frac{f}{2} p v
\end{aligned}
$
Let gas be monoatomic
$
\begin{aligned}
& f=3 \\
& E=\frac{3}{2} \times 3 \times 10^6 \times 2 \\
& E=9 \times 10^6 \mathrm{~J}
\end{aligned}
$
Hence, the answer is option (1).
Example 3: Two kg of a monoatomic gas is at a pressure of $4 \times 10^4 \mathrm{~N} / \mathrm{m}^2$. The density of the gas is $8 \mathrm{Kg} / \mathrm{m}^3$. What is the order of energy (in Joule) of the gas due to its thermal motion?
1) 105
2) 103
3) 106
4) 104
Solution:
$\begin{aligned}
& \text { Thermal energy }=N \frac{3}{2} K T=\frac{N}{N_A} \frac{3}{2} R T=\frac{3}{2} n R T=\frac{3}{2} P V=\frac{3}{2} P\left(\frac{\mathrm{m}}{8}\right) \\
& \text { Thermal energy }=\frac{3}{2} \times 4 \times 10^4 \times\left(\frac{2}{8}\right)=1.5 \times 10^4
\end{aligned}$
Hence, the answer is the option (4).
Example 4: A gas mixture consists of 3 moles of oxygen and 5 moles of argon at temperature T. Considering only translational and rotational modes, the total internal energy (in RT) of the system is:
1) 20
2) 12
3) 4
4) 15
Solution:
Total internal energy
$\begin{aligned}
& U=\frac{f_o}{2} n_o R T+\frac{f_a}{2} n_a R T \\
& =\frac{5}{2} 3 R T+\frac{3}{2} 5 R T \\
& =15 R T
\end{aligned}$
Hence, the answer is option (4).
Example 5: An $\mathrm{HCl}$ molecule has rotational, translational and vibrational motions. If the RMS velocity of $\mathrm{HCl}$ molecules in its gaseous phase is $\bar{v}$, $m$ is its mass and $k_B$ is Boltzmann constant, then its temperature will be :
1) $\frac{m \bar{v}^2}{6 k_B}$
2) $\frac{m \bar{v}^2}{3 k_B}$
3) $\frac{m \bar{v}^2}{7 k_B}$
4) $\frac{m \bar{v}^2}{5 k_B}$
Solution:
The kinetic energy of gas due to translation per mole
$\begin{aligned}
& E=\frac{3}{2} P V \\
& =\frac{3}{2} R T
\end{aligned}$
wherein
R = Universal gas constant
T = temperature of gas
HCl has 3 translational, 2 rotational, and 1 vibrational degree of freedom
$\begin{aligned}
& \text { Translational Kinetic energy }=K . E_{\text {Translation }}=\frac{3}{2} K_B T \\
& \frac{1}{2} m \bar{v}^2=\frac{3}{2} K_B T \\
& T=\frac{m \overline{v^2}}{3 k_B}
\end{aligned}$
Hence, the answer is the option (2).
An important aspect of motion and interaction among gas particles is the kinetic energy for an ideal gas; hence it becomes necessary to get acquainted with the concept of kinetic energy for an ideal gas. According to this concept, the higher the temperature of a given volume of gas, the more intense its kinetic movements would become. This correlation accounts for a number of properties displayed by gases including their pressure-volume relationships and temperatures thereby making it stand out in describing thermodynamic processes.
Q 1. What are real-life applications of the pressure of Ideal Gas?
Ans: Pressure is used in many everyday situations such as when inflating a balloon or filling a tire with air.
Q 2. What is the pressure at absolute zero?
Ans: If the temperature could be reduced to absolute zero, the pressure of the ideal gas would be 0, implying that the gas would exert no force on the walls of its container.
Q 3. Can the pressure of an ideal gas be zero?
Ans: No
Q4: How does temperature affect the kinetic energy of an ideal gas?
Ans: The kinetic energy of an ideal gas is directly proportional to its temperature. As the temperature increases, the average kinetic energy of the gas molecules increases, meaning the molecules move faster.
Q5: Why is kinetic energy important for understanding ideal gases?
Ans: Kinetic energy is crucial for understanding ideal gases because it helps explain how temperature and pressure are related to the motion of gas molecules. It forms the basis for the kinetic theory of gases, which provides a microscopic explanation for macroscopic gas properties.
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