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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.
1. Know the formula for calculating kinetic energy. The formula for calculating kinetic energy (KE) is the following: KE = 0.5 * mv 2. Here m stands for mass, the measure of how much matter is in an object, and v stands for velocity of the object, or the rate at which the object changes its position.o find the velocity of an object when you only know the kinetic energy and the mass, just plug the kinetic energy and mass into the same equation and solve for the velocity, remembering to state your answer in m/s.