The escape velocity \( V_e \) from a spherical body is given by the formula:
\(V_e = \sqrt{\frac{2GM}{R}}\)
Where:
Substituting the expression for mass \( M \) in terms of density \( \rho \) (where \( M = \frac{4}{3} \pi R^3 \rho \)), we get:
\(V_e = \sqrt{\frac{2G}{R} \left(\frac{4}{3} \pi R^3 \rho \right)}\)
This simplifies to:
\(V_e \propto R \sqrt{\rho}\)
Therefore, the ratio of escape velocities for two bodies with different radii and densities is:
\(1 : 2 \sqrt{2}\)
A full wave rectifier circuit with diodes (\(D_1\)) and (\(D_2\)) is shown in the figure. If input supply voltage \(V_{in} = 220 \sin(100 \pi t)\) volt, then at \(t = 15\) msec: 
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