For an ideal solution, the total vapour pressure is given by Raoult's Law: \[ P_{\text{total}} = P_X + P_Y \] where \(P_X\) and \(P_Y\) are the partial vapour pressures of components X and Y, respectively. The partial vapour pressure of a component in a solution is given by: \[ P_X = X_X \times P_X^0 \quad \text{and} \quad P_Y = X_Y \times P_Y^0 \] where \(X_X\) and \(X_Y\) are the mole fractions of X and Y, and \(P_X^0\) and \(P_Y^0\) are the vapour pressures of pure X and Y. Given:
The vapour pressure of pure X, \(P_X^0 = 200\) mm Hg.
The vapour pressure of pure Y, \(P_Y^0 = 300\) mm Hg.
The mole ratio of X and Y is 3:2,
so: \[ X_X = \frac{3}{3+2} = \frac{3}{5} \quad \text{and} \quad X_Y = \frac{2}{3+2} = \frac{2}{5} \]
Now, calculate the partial pressures: \[ P_X = \frac{3}{5} \times 200 = 120 \, \text{mm Hg} \] \[ P_Y = \frac{2}{5} \times 300 = 120 \, \text{mm Hg} \] Thus, the total vapour pressure is: \[ P_{\text{total}} = 120 + 120 = 240 \, \text{mm Hg} \]
The correct option is (D) : \(240\)
According to Raoult's Law, the vapor pressure of an ideal solution is given by:
p_total = p_X + p_Y
where:
p_X = X_X * p_X^0 (vapor pressure of component X in the solution)
p_Y = X_Y * p_Y^0 (vapor pressure of component Y in the solution)
Here, \(X_X\) and \(X_Y\) are the mole fractions of X and Y, respectively, and \(p_X^0\) and \(p_Y^0\) are the vapor pressures of the pure components.
Given: - Vapor pressure of pure X (\(p_X^0\)) = 200 mm of Hg - Vapor pressure of pure Y (\(p_Y^0\)) = 300 mm of Hg - Mole ratio of X and Y = 3:2, hence:
- Mole fraction of X, \(X_X = \frac{3}{3+2} = \frac{3}{5} = 0.6\)
- Mole fraction of Y, \(X_Y = \frac{2}{3+2} = \frac{2}{5} = 0.4\) Now, applying Raoult's Law:
p_total = (0.6 * 200) + (0.4 * 300)
p_total = 120 + 120 = 240 mm of Hg
Therefore, the correct vapor pressure of the solution is 240 mm of Hg.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of