Escape velocity of a projectile from the Earth, \(v_{esc}\) = \(11.2 \; km/s\)
Projection velocity of the projectile, \(v_p\) = \(3v_{esc}\)
Mass of the projectile = \(m\)
Velocity of the projectile far away from the Earth = \(v_f\)
Total energy of the projectile on the Earth = \(\frac{1}{2}mv^2_p - \frac{1}{2}mv^2_{esc}\)
Gravitational potential energy of the projectile far away from the Earth is zero.
Total energy of the projectile far away from the Earth= \(\frac{1}{2}mv^2_f\)
From the law of conservation of energy, we have
\(\frac{1}{2}mv^2_p - \frac{1}{2}mv^2_{esc}\) = \(\frac{1}{2}mv_f^2\)
\(v_r\) = \(\sqrt{v_p ^2 - v_{esc}^2}\)
=\(\sqrt{(3v_{esc}) ^2 - (v_{esc})^2}\)
=\(\sqrt 8 v_{esc}\)
=\(\sqrt 8 \times 11.2\) = \(31.68 \; km/s\)
Escape speed is the minimum speed, which is required by the object to escape from the gravitational influence of a plannet. Escape speed for Earth’s surface is 11,186 m/sec.
The formula for escape speed is given below:
ve = (2GM / r)1/2
where ,
ve = Escape Velocity
G = Universal Gravitational Constant
M = Mass of the body to be escaped from
r = Distance from the centre of the mass