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Vocabulary and key derivation terms for the proof of the law of conservation of mechanical energy in a freely falling body.
Law of conservation of mechanical energy
The law stating that energy can neither be created nor be destroyed, but it can be converted from one form to another form; hence, the total energy remains constant in a closed system.
Potential energy (P.E) at Point A
mgh, representing the energy at a height h above the ground where the body is initially released.
Kinetic energy (K.E) at Point A
0, because the initial velocity of the body at release is vA=0, making 21m(0)2=0.
Total energy (T.E) at Point A
mgh, calculated by adding potential energy and kinetic energy (P.E+K.E=mgh+0).
Potential energy (P.E) at Point B
mg(h−x)=mgh−mgx, where x is the distance the body has traveled downward from Point A, leaving it at a height of h−x.
Kinetic energy (K.E) at Point B
mgx, determined by using vB2−u2=2as (with u=0, a=g, and s=x) to get vB2=2gx, yielding 21m(2gx)=mgx.
Total energy (T.E) at Point B
mgh, calculated by adding potential energy and kinetic energy: (mgh−mgx)+mgx=mgh.
Potential energy (P.E) at Point C
0, because the body hits the ground where the height is h=0, giving mg(0)=0.
Kinetic energy (K.E) at Point C
mgh, determined by using vC2−u2=2as (with u=0, a=g, and s=h) to get vC2=2gh, yielding 21m(2gh)=mgh.
Total energy (T.E) at Point C
mgh, calculated by adding potential energy and kinetic energy (P.E+K.E=0+mgh).
Kinematic equation for velocity calculation
v2−u2=2as, used with u=0 and a=g to find the velocity squared (v2) at different points during free fall.