Kinetic Theory of Gases
Important Questions for WBCHSE Class 11 Physics
Complete Study Guide with Formulas and Derivations
1
1-Mark Questions (VSA / MCQ)
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Define Mean Free Path of a gas molecule.
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What is the value of average velocity of gas molecules in thermal equilibrium?
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On which factor does the average Kinetic Energy of a gas depend?
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State the number of degrees of freedom for a monoatomic gas.
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Under what conditions of temperature and pressure does a real gas behave like an ideal gas?
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What is the total translational kinetic energy of 1 mole of an ideal gas at temperature T?\[E = \frac{3}{2}RT\]
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Define Absolute Zero temperature in terms of kinetic theory.
2
2-Mark Questions (Short Answer)
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State the Law of Equipartition of Energy.
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Why does the moon have no atmosphere? Explain based on rms speed.
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Deduce Boyle's Law from the kinetic theory of gases.
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Explain the kinetic interpretation of Temperature.
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State Graham's Law of Diffusion and write its mathematical form.\[\frac{r_1}{r_2} = \sqrt{\frac{M_2}{M_1}}\]
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Calculate the ratio of \(v_{rms}\) to \(v_{av}\) for a gas at a given temperature.\[\frac{v_{rms}}{v_{av}} = \sqrt{\frac{3}{8/\pi}} \approx 1.085\]
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Define molar specific heat at constant volume (\(C_v\)) and constant pressure (\(C_p\)).
3-5
3 & 5-Mark Questions (Long Answer / Derivations)
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State the basic postulates/assumptions of the Kinetic Theory of Gases.
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Derive the expression for the pressure exerted by an ideal gas (\(P = \frac{1}{3} \rho \bar{v}^2\)).📝 Key Derivation Steps:
- Consider a gas molecule with velocity components \(v_x, v_y, v_z\)
- Change in momentum during collision with wall: \(2mv_x\)
- Force exerted = rate of change of momentum
- Pressure = Force/Area = \(\frac{1}{3} \rho \bar{v}^2\)
Where \(\rho\) is density and \(\bar{v}^2\) is mean square speed.
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Using the law of equipartition of energy, calculate the ratio of specific heats (\(\gamma = C_p/C_v\)) for diatomic gases.📌 Important:
For a diatomic gas at moderate temperatures:
- Degrees of freedom = 5 (3 translational + 2 rotational)
- \(C_v = \frac{5}{2}R\), \(C_p = C_v + R = \frac{7}{2}R\)
- \(\gamma = \frac{C_p}{C_v} = \frac{7}{5} = 1.4\)
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Define and derive expressions for:
- Root Mean Square (rms) speed: \(v_{rms} = \sqrt{\frac{3kT}{m}} = \sqrt{\frac{3RT}{M}}\)
- Average speed: \(v_{av} = \sqrt{\frac{8kT}{\pi m}} = \sqrt{\frac{8RT}{\pi M}}\)
- Most Probable speed: \(v_{mp} = \sqrt{\frac{2kT}{m}} = \sqrt{\frac{2RT}{M}}\)
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Numerical: At what temperature will the rms speed of oxygen molecules be sufficient for escaping from the earth's atmosphere?
Escape velocity from Earth: \(v_e = 11.2 \text{ km/s} = 11200 \text{ m/s}\)
Using \(v_{rms} = \sqrt{\frac{3RT}{M}}\) and setting \(v_{rms} = v_e\):
\[T = \frac{M v_e^2}{3R} = \frac{0.032 \times (11200)^2}{3 \times 8.314} \approx 1.6 \times 10^5 \text{ K}\] -
Numerical: A vessel contains a mixture of 2 moles of Hydrogen and 3 moles of Helium. Calculate the total internal energy of the system at temperature T.
For Hydrogen (diatomic): \(U_H = 2 \times \frac{5}{2}RT = 5RT\)
For Helium (monoatomic): \(U_{He} = 3 \times \frac{3}{2}RT = 4.5RT\)
Total internal energy: \(U = U_H + U_{He} = 9.5RT\)
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