The minimum velocity required to escape from the gravitational force of the planet is known as the escape velocity of the planet. Consider the object ‘m’ on the surface of Earth.
Initial PE = \(-\frac {GMm}{R}\)
Initial KE = \(\frac {1}{2}\) m (Vesc)2
Total energy = \(\frac {1}{2}\)m (Vesc)2 \(-\frac {GMm}{R}\)
To escape, the KE should greater than or equal to its PE.
![](https://www.sarthaks.com/?qa=blob&qa_blobid=16903349120338883139)
Initial velocity of object = 22.4 km s-1
= 2 Vesc
Total Initial Energy
= \(\frac {1}{2}\) m(2Vesc)2 - \(\frac {GMm}{R}\)
= 2 m V2esc- \(\frac {1}{2}\)m V2esc [From(1)]
= \(\frac {3}{2}\) m V2esc .......(2)
Total Final energy = PE (at ∞) + \(\frac {1}{2}\)mVf2
= 0 + \(\frac {1}{2}\) mVf2
= \(\frac {1}{2}\)mVf2 .........(3)
By conservation of energy, (2) = (3)
Vf = \(\sqrt 3\)Vesc
= 19.4 km s-1.