A spaceship is orbiting the Earth around the circular orbit of radius R=2.5Ro, where Ro is the Earth’s radius. What should be the additional velocity V to be supplied to the spaceship in the direction away from the center of the Earth (along the radius of the orbit) so the ship may completely escape the Earth gravity?
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I think you would need the mass of the spaceship to determine this, unless i am missing something.
An energy perspective is most useful here. You need sufficient kinetic energy directed radially outward to raise the potential energy of the spacecraft from what it is at R to what it would be at infinity. \[dU = 0 - \left( - \frac{G M m}{R} \right) = \frac{G M m}{R}\] Set that equal to the additional kinetic energy: \[dE_k = \frac{1}{2} m v^2 = \frac{G M m}{R}\] Now solve for v. G is Newton's constant and M is the mass of the Earth. Fortunately the mass of the spacecraft drops out, so you don't need to know it.
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