explain the equations of motion.
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Newton's second law, which states that the force F acting on a body is equal to the mass m of the body multiplied by the acceleration a of its centre of mass, F = ma, is the basic equation of motion in classical mechanics.
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There are three equations of motion that can be used to derive components such as displacement(s), velocity (initial and final), time(t) and acceleration(a).
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Definition of Equations of Motion
First Equation of Motion : v=u+at.
Second Equation of Motion : s=ut+\frac{1}{2}at^2.
Third Equation of Motion : v^2=u^2+2as.
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