Using the law of conservation of energy obtain the expression for the escape velocity
Answers
Explanation:
This is the escape speed - the minimum speed required to escape a planet's gravitational pull.
To find the escape velocity, apply energy conservation: Ui + Ki = Uf + Kf
For a planet of mass M and radius R, the potential energy of an object of mass m at the planet's surface is: U= - G m M/R.
Explanation:
How fast would you have to throw an object so it never came back down? This is the escape speed - the minimum speed required to escape a planet's gravitational pull.
To find the escape velocity, apply energy conservation: Ui + Ki = Uf + Kf
For escape, set both terms on the right to zero. We want the object to barely reach infinity, where the potential energy is zero.
For a planet of mass M and radius R, the potential energy of an object of mass m at the planet's surface is: U= - G m M/R.
Therefore:
- G m M
R
+ Kescape = 0
½ mv2escape = G m M/ R.
vescape = (
2 G M
R
) ½
For the Earth this is 11.2 km/s ≈ 25,000 mph!