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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.
The amount of kinetic energy (KE) possessed by a moving object is dependent upon mass and speed. The equation for kinetic energy is. KE = 0.5 â¢ m â¢ v2. where m is the mass of the object (with standard units of kilograms) and v is the speed of the object (with standard units of m/s).The total mechanical energy possessed by an object is the sum of its kinetic and potential energies.here m is the mass of the object (with standard units of kilograms) and v is the speed of the object (with standard units of m/s). The total mechanical energy possessed by an object is the sum of its kinetic and potential energies.