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For an object of mass the energy required to escape the Earth's gravitational field is GMm / r, a function of the object's mass (where r is the radius of the Earth, G is the gravitational constant, and M is the mass of the Earth, M =5.9736Ã10 24 kg).or a mass equal to a Saturn V rocket, the escape velocity relative to the launch pad is 253.5 am/s (8 nanometers per year) faster than the escape velocity relative to the mutual center of mass.
2. Plug the mass and velocity into the equation. If you don't know the mass or velocity of the object, then you'll have to calculate it. But let's say that you do know both quantities and are working to solve the following problem: Determine the kinetic energy of a 55 kg. woman running with a speed of 3.87m/s.