For diatomic gas, the degrees of freedom \( f = 5 \) (at room temperature), and for monoatomic gas \( f = 3 \).
Using the equipartition theorem: \[ {Total KE for diatomic} = 3 { moles} \times \frac{5}{2} R T = \frac{15}{2} R T \] \[ {Total KE for monoatomic} = n { moles} \times \frac{3}{2} R T \] Equating the two energies: \[ \frac{15}{2} R T = \frac{3}{2} R T \times n \implies n = 5 \]
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Two similar metallic rods of the same length \( l \) and area of cross section \( A \) are joined and maintained at temperatures \( T_1 \) and \( T_2 \) (\( T_1>T_2 \)) at one of their ends as shown in the figure. If their thermal conductivities are \( K \) and \( \frac{K}{2} \) respectively. The temperature at the joining point in the steady state is:

According to equipartition principle, the energy contributed by each translational degree of freedom and rotational degree of freedom at a temperature T are respectively (\( k_B = \text{Boltzmann constant} \)):
Kepler's second law (law of areas) of planetary motion leads to law of conservation of