For a rocket to escape from the surface of the object, it must overcome the pull of gravity.
The key is now whether the projectile comes to a halt before it escapes the pull of gravity. Note that
More generally, since the speed of light is the maximum with which things can propogate through the Universe, this means that nothing can travel fast enough to escape from the surface of such an object.
The imaginary surface which separates the Universe into these regions is referred to as the Event Horizon.
Note that since the escape speed is sqrt[ 2 G M / R ], we see that c = sqrt[ 2 G M / R ] ===> c**2 = 2 G M / R or that the radius of the event horizon is given by R = 2 G M / c**2.
This is referred to as the Schwarzschild Radius in honor of Karl Schwarzschild who was the first person to work out the theory. The Scwarzschild radius is an exceedginly small number. The Schwarschild radius for a solar mass black hole is
That is, the Sun would have to collapse to a diameter of 6 kilometers in order to become a black hole. Comment -- A 10 M(Sun) black hole has a radius = 3 [10M(Sun)/M(Sun)] kilometers = 3 [10] kilometers = 30 kilometers.
Properties of black holes