To find the escape velocity of planet B, we first recall the expression for escape velocity from a planet.
ve = √(2GM / R)
where:
The mass of a spherical planet can be written in terms of its density and radius as:
M = ρ × (4/3)πR³
Substituting this expression for mass into the escape velocity formula:
ve = √(2G × (4/3)πρR³ / R)
ve = √(8πGρR² / 3)
Thus, escape velocity depends on the square root of density and directly on the radius.
Given:
Using the relation ve ∝ √ρ × R, we write:
veB / veA = √(ρB / ρA) × (RB / RA)
Substituting the given ratios:
veB / veA = √(0.1) × 0.1 = √(0.001)
Hence:
veB = √(0.001) × 10 km/s
veB = 1 / √10 km/s
Final Answer:
Escape velocity of planet B = 1 / √10 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 
