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
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)