The formula to calculate the escape velocity (ev) is:
\[ ev = \sqrt{\frac{2 M G}{R}} \]
Where:
Escape velocity is the speed that an object needs to travel to escape the gravitational pull of a larger body. It is the minimum velocity required to leave the planet without further propulsion.
Let's consider an example for Earth:
Using the formula to calculate Escape Velocity:
\[ ev = \sqrt{\frac{2 \times 5.972 \times 10^{24} \times 6.674 \times 10^{-11}}{6.371 \times 10^{6}}} \approx 11186 \, \text{m/s} \]
This means that the escape velocity for Earth is approximately 11186 m/s.