Escape velocity of a body from earth is 11.2 km/s. If the radius of a planet be one-third the radius of earth and mass be one-sixth that of earth, the escape velocity from the planet is:
11.2 km/s
8.4 km/s
4.2 km/s
7.9 km/s
Solution: The escape velocity \( V_e \) from a celestial body is given by the formula:
\[ V_e = \sqrt{\frac{2GM}{R}}, \]
where:
- \( G \) is the gravitational constant,
- \( M \) is the mass of the body,
- \( R \) is the radius of the body.
Given Values for Earth: Escape velocity from Earth, \( V_{e,\text{earth}} = 11.2 \, \text{km/s} \). For Earth, let:
Mass \( M_e \) and radius \( R_e \) be constants.
For the Planet: The radius of the planet \( R_p = \frac{1}{3} R_e \). The mass of the planet \( M_p = \frac{1}{6} M_e \).
Calculating Escape Velocity for the Planet: Substituting the values into the escape velocity formula:
\[ V_{e,\text{planet}} = \sqrt{\frac{2G \left( \frac{1}{6} M_e \right)}{\frac{1}{3} R_e}}. \]
Simplifying the expression:
\[ V_{e,\text{planet}} = \sqrt{\frac{2GM_e}{R_e}} \times \sqrt{\frac{1}{6} \times 3}. \]
Thus, it can be expressed as:
\[ V_{e,\text{planet}} = V_{e,\text{earth}} \times \sqrt{\frac{1}{2}}. \]
Substituting \( V_{e,\text{earth}} = 11.2 \, \text{km/s} \):
\[ V_{e,\text{planet}} = 11.2 \times \sqrt{\frac{1}{2}} = 11.2 \times 0.7071 \approx 7.9 \, \text{km/s}. \]
Thus, the escape velocity from the planet is: 7.9 km/s.
Net gravitational force at the center of a square is found to be \( F_1 \) when four particles having masses \( M, 2M, 3M \) and \( 4M \) are placed at the four corners of the square as shown in figure, and it is \( F_2 \) when the positions of \( 3M \) and \( 4M \) are interchanged. The ratio \( \dfrac{F_1}{F_2} = \dfrac{\alpha}{\sqrt{5}} \). The value of \( \alpha \) is 

Which one of the following graphs accurately represents the plot of partial pressure of CS₂ vs its mole fraction in a mixture of acetone and CS₂ at constant temperature?
